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Catalogues
2015-06-12T08:29:27Z
<p>Xdupac: /* (2015) Second Catalogue of Compact Sources */</p>
<hr />
<div>{{DISPLAYTITLE:2015 Catalogues}}<br />
<br />
== (2015) Second Catalogue of Compact Sources ==<br />
<br />
'''The Second Planck Catalogue of Compact Sources will be available in the next stage of the 2015 Planck release, foreseen end of June 2015.'''<br />
<br />
== (2015) Second SZ Catalogue ==<br />
<br />
The Planck SZ catalogue is constructed as described in [[Compact_Source_catalogues#Planck_Sunyaev-Zeldovich_catalogue|SZ catalogue]] and in sections 2 and 3 of {{PlanckPapers|planck2014-a36}}. Three pipelines are used to detect SZ clusters: two independent implementations of the Matched Multi-Filter (MMF1 and MMF3), and PowellSnakes (PwS). The main catalogue is constructed as the union of the catalogues from the three detection methods. The completeness and reliability of the catalogues have been assessed through internal and external validation as described in section 4 of {{PlanckPapers|planck2014-a36}}.<br />
<br />
The size of a detection is given in terms of the scale size, &theta;<sub>s</sub>, and the flux is given in terms of the total integrated Comptonization parameter, Y = Y<sub>5R500</sub>. The parameters of the GNFW profile assumed by the detection pipelines are written in the headers of the catalogues. For the sake of convenience, the conversion factor from Y to Y<sub>500</sub> is also provided in the header.<br />
<br />
The union catalogue contains the coordinates of a detection, its signal-to-noise ratio, an estimate of Y and its uncertainty, together with a summary of the validation information, including external identification of a cluster and its redshift if they are available. The pipeline from which the information is taken is called the reference pipeline. If more than one pipeline makes the same detection, the information is taken from the the pipeline that makes the most significant detection. Where the redshift is known, we provide the SZ mass for the reference pipeline.<br />
<br />
The individual catalogues contain the coordinates and the signal-to-noise ratio of the detections, and information on the size and flux of the detections. The entries are cross-referenced to the detections in the union catalogue. The full information on the degeneracy between &theta;<sub>s</sub> and Y is included in the individual catalogues in the form of the two-dimensional probability distribution for each detection. It is computed on a well-sampled grid to produce a two-dimensional image for each detection. It is provided in this form so it can be combined with a model or external data to produce tighter constraints on the parameters. The individual catalogues also contain Planck measurements of the SZ mass observable, M<sub>SZ</sub>, as calculated using a Y-M scaling relation and an assumed redshift to break the Y-&theta;<sub>s</sub> degeneracy. These are provided for each detection as functions of assumed redshift, in the range 0.01 < z < 1, along with the upper and lower 68% confidence limits.<br />
<br />
The selection function of the union catalogue, the intersection catalogue and the individual catalogues are provided in additional files. The selection function files contains the probability of detection for clusters of given intrinsic parameters &theta;<sub>500</sub> and Y<sub>500</sub>. The file includes the definition of the survey area in the form of a HEALPix mask, and is evaluated for a range of signal-to-noise thresholds between 4.5 and 10.<br />
<br />
=== Union catalogue ===<br />
<br />
The union catalogue is contained in ''{{PLASingleFile|fileType=cat | name=HFI_PCCS_SZ-union_R2.08.fits | link=HFI_PCCS_SZ-union_R2.08.fits}}''.<br />
<br />
{| border="1" cellpadding="3" cellspacing="0" align="center" style="text-align:left" width=800px<br />
|- bgcolor="ffdead" <br />
!colspan="4" | Extension 0: Primary header, no data<br />
|- bgcolor="ffdead" <br />
! FITS Keyword || Data Type || Units || Description<br />
|- <br />
|INSTRUME || String || || Instrument (HFI)<br />
|- <br />
| VERSION || String || || Version of catalogue<br />
|- <br />
| DATE || String || || Date file created: yyyy-mm-dd<br />
|- <br />
| ORIGIN || String || || Name of organization responsible for the data (HFI-DPC)<br />
|- <br />
| TELESCOP || String || || Telescope (PLANCK)<br />
|- <br />
| CREATOR || String || || Pipeline version<br />
|- <br />
| DATE-OBS || String || || Start date of the survey: yyyy-mm-dd<br />
|- <br />
| DATE-END || String || || End date of the survey: yyyy-mm-dd<br />
|- <br />
| PROCVER || String || || Data version<br />
|- <br />
| PP_ALPHA || Real*4 || || GNFW pressure profile &alpha; parameter<br />
|- <br />
| PP_BETA || Real*4 || || GNFW pressure profile &beta; parameter<br />
|- <br />
| PP_GAMMA || Real*4 || || GNFW pressure profile &gamma; parameter<br />
|- <br />
| PP_C500 || Real*4 || || GNFW pressure profile c<sub>500</sub> parameter<br />
|- <br />
| PP_Y2YFH || Real*4 || || Conversion factor from Y to Y<sub>500</sub><br />
<br />
|- bgcolor="ffdead" <br />
!colspan="4" | Extension 1: BINTABLE, EXTNAME = PSZ2_UNION<br />
|- bgcolor="ffdead" <br />
! Column Name || Data Type || Units || Description<br />
|-<br />
|INDEX || Int*4 || || Index used to cross-reference with individual catalogues<br />
|-<br />
|NAME || String || || Source name (see note 1)<br />
|-<br />
|GLON || Real*8 || degrees || Galactic longitude<br />
|-<br />
|GLAT || Real*8 || degrees || Galactic latitude<br />
|-<br />
|RA || Real*8 || degrees || Right ascension (J2000) transformed from (GLON,GLAT)<br />
|-<br />
|DEC || Real*8 || degrees || Declination (J2000) transformed from (GLON,GLAT)<br />
|-<br />
|POS_ERR || Real*4 || arcmin || Position uncertainty (95% confidence interval)<br />
|-<br />
|SNR || Real*4 || || Signal-to-noise ratio of the detection<br />
|-<br />
|PIPELINE || Int*4 || || Pipeline from which information is taken (reference pipeline): 1= MMF1; 2 = MMF3; 3 = PwS<br />
|-<br />
|PIPE_DET || Int*4 || || Pipelines which detect this object (see note 2)<br />
|-<br />
|PCCS2 || Bool || || Indicates whether detection matches with any in PCCS2 catalogues<br />
|-<br />
|PSZ || Int*4 || || Index of matching detection in PSZ1, or -1 if new detection<br />
|-<br />
|IR_FLAG || Int*1 || || Flag denoting heavy infrared contamination<br />
|-<br />
|Q_NEURAL || Real*4 || || Neural network quality flag (see note 3)<br />
|-<br />
|Y5R500 || Real*4 || 10<sup>-3</sup>&nbsp;arcmin<sup>2</sup> || Mean marginal Y<sub>5R500</sub> as determined by reference pipeline<br />
|-<br />
|Y5R500_ERR || Real*4 || 10<sup>-3</sup>&nbsp;arcmin<sup>2</sup> || Uncertainty on Y<sub>5R500</sub> as determined by reference pipeline<br />
|-<br />
|VALIDATION || Int*4 || || External validation status (see note 4)<br />
|-<br />
|REDSHIFT_ID || String || || External identifier of cluster associated with redshift measurement (see note 5)<br />
|-<br />
|REDSHIFT || Real*4 || || Redshift of cluster (see note 5)<br />
|-<br />
|MSZ || Real*4 || 10<sup>14</sup>&nbsp;M<sub>sol</sub> || SZ mass proxy (see note 6)<br />
|-<br />
|MSZ_ERR_UP || Real*4 || 10<sup>14</sup>&nbsp;M<sub>sol</sub> || Upper bound of 68% SZ mass proxy confidence interval (see note 6)<br />
|-<br />
|MSZ_ERR_LOW || Real*4 || 10<sup>14</sup>&nbsp;M<sub>sol</sub> || Lower bound of 68% SZ mass proxy confidence interval (see note 6)<br />
|-<br />
|MCXC || String || || Identifier of X-ray counterpart in the MCXC, if one is present <br />
|-<br />
|REDMAPPER || String || || Identifier of optical counterpart in the RedMAPPer catalogue, if one is present <br />
|-<br />
|ACT || String || || Identifier of SZ counterpart in the ACT catalogues, if one is present <br />
|-<br />
|SPT || String || || Identifier of SZ counterpart in the SPT catalogues, if one is present <br />
|-<br />
|WISE_FLAG || Int*4 || || Confirmation flag of WISE overdensity (see note 7)<br />
|-<br />
|AMI_EVIDENCE || Real*4 || || Bayesian evidence for AMI counterpart detection (see note 8)<br />
|-<br />
|COSMO || Bool || || Indicates whether detection is in the cosmology sample<br />
|-<br />
|COMMENT|| String || || Comments on this detection<br />
|}<br />
<br />
'''Notes'''<br />
# Format is <tt>PSZ2 Glll.ll&plusmn;bb.b</tt> where (l,b) are the Galactic coordinates truncated to 2 decimal places.<br />
# The three least significant decimal digits are used to represent detection or non-detection by the pipelines. Order of the digits: hundreds = MMF1; tens = MMF3; units = PwS. If it is detected then the corresponding digit is set to 1, otherwise it is set to 0.<br />
# Neural network quality flag is 1-Q<sub>bad</sub>, following the definitions in Aghanim et al. 2014.<br />
# Summary of the external validation, encoding the most robust external identification: 10 = ENO follow-up; 11 = RTT follow-up; 12 = PanSTARRs; 13 = RedMAPPer non-blind; 14 = SDSS high-z; 15 = AMI; 16 = WISE; 20 = legacy identification from the PSZ1; 21 = MCXC; 22 = SPT; 23 = ACT; 24 = RedMAPPer; 25 = legacy identification from PSZ1 with externally updated redshift; 30 = NED; -1 = no known external counterpart.<br />
# Redshift source is the most robust external identification listed in the VALIDATION field.<br />
# M<sub>SZ</sub> is the hydrostatic mass assuming the best-fit Y-M scaling relation of Arnaud 2010 as a prior. The uncertainties are statistical and based on the Planck measurement uncertainties only. Not included in the uncertainties are the statistical errors on the scaling relation, the intrinsic scatter in the relation, or systematic errors in data selection for the scaling relation fit.<br />
# Assigned by visual inspection: 0 = no significant galaxy overdensity; 1 = possible galaxy overdensity; 2 = probable galaxy overdensity; 3 = significant galaxy overdensity detected; -1 = possible galaxy overdensity (affected by bright star artefacts); -2 = no significant galaxy overdensity (affected by bright star artefacts); -3 = no assessment possible (affected by bright star artefacts); -10 = not analysed.<br />
# Defined in the paper.<br />
<br />
=== Individual catalogues ===<br />
<br />
The individual pipeline catalogues are contained in the FITS files <br />
* {{PLASingleFile | fileType=cat | name=HFI_PCCS_SZ-MMF1_R2.08.fits | link=HFI_PCCS_SZ-MMF1_R2.08.fits }} (MMF1 pipeline)<br />
* {{PLASingleFile | fileType=cat | name=HFI_PCCS_SZ-MMF3_R2.08.fits | link=HFI_PCCS_SZ-MMF3_R2.08.fits }} (MMF3 pipeline)<br />
* {{PLASingleFile | fileType=cat | name=HFI_PCCS_SZ-PwS_R2.08.fits | link=HFI_PCCS_SZ-PwS_R2.08.fits }} (PowellSnakes pipeline)<br />
<br />
Their structure is as follows:<br />
<br />
{| border="1" cellpadding="3" cellspacing="0" align="center" style="text-align:left" width=800px<br />
|+ '''FITS file structure'''<br />
|- bgcolor="ffdead" <br />
! colspan="4" | Extension 0: Primary header, no data<br />
|- bgcolor="ffdead" <br />
! FITS Keyword || Data Type || Units || Description<br />
|- <br />
|INSTRUME || String || || Instrument (HFI)<br />
|- <br />
| VERSION || String || || Version of catalogue<br />
|- <br />
| DATE || String || || Date file created: yyyy-mm-dd<br />
|- <br />
| ORIGIN || String || || Name of organization responsible for the data (HFI-DPC)<br />
|- <br />
| TELESCOP || String || || Telescope (PLANCK)<br />
|- <br />
| CREATOR || String || || Pipeline version<br />
|- <br />
| DATE-OBS || String || || Start time of the survey: yyyy-mm-dd<br />
|- <br />
| DATE-END || String || || End time of the survey: yyyy-mm-dd<br />
|- <br />
| PROCVER || String || || Data version<br />
|- <br />
| PP_ALPHA || Real*4 || || GNFW pressure profile &alpha; parameter<br />
|- <br />
| PP_BETA || Real*4 || || GNFW pressure profile &beta; parameter<br />
|- <br />
| PP_GAMMA || Real*4 || || GNFW pressure profile &gamma; parameter<br />
|- <br />
| PP_C500 || Real*4 || || GNFW pressure profile c<sub>500</sub> parameter<br />
|- <br />
| PP_Y2YFH || Real*4 || || Conversion factor from Y to Y<sub>500</sub><br />
<br />
|- bgcolor="ffdead" <br />
! colspan="4" | Extension 1: BINTABLE, EXTNAME = PSZ2_INDIVIDUAL<br />
|- bgcolor="ffdead" <br />
! Column Name || Data Type || Units || Description<br />
|-<br />
|INDEX || Int*4 || || Index from union catalogue<br />
|-<br />
|NAME || String || || Source name (see note 1)<br />
|-<br />
|GLON || Real*8 || degrees || Galactic longitude<br />
|-<br />
|GLAT || Real*8 || degrees || Galactic latitude<br />
|-<br />
|RA || Real*8 || degrees || Right ascension (J2000) transformed from (GLON, GLAT)<br />
|-<br />
|DEC || Real*8 || degrees || Declination (J2000) transformed from (GLON, GLAT)<br />
|-<br />
|POS_ERR || Real*4 || arcmin || Position uncertainty (95% confidence interval)<br />
|-<br />
|SNR || Real*4 || || Signal-to-noise ratio of detection<br />
|-<br />
|TS_MIN || Real*4 || || Minimum value of &theta;<sub>s</sub> in grid in second extension HDU (see note 2)<br />
|-<br />
|TS_MAX || Real*4 || || Maximum value of &theta;<sub>s</sub> in grid in second extension HDU (see note 2)<br />
|-<br />
|Y_MIN || Real*4 || || Minimum value of Y in grid in second extension HDU (see note 2)<br />
|-<br />
|Y_MAX || Real*4 || || Maximum value of Y in grid in second extension HDU (see note 2)<br />
|- bgcolor="ffdead" <br />
! Keyword || Data Type || Value || Description<br />
|- <br />
| PIPELINE || String || || Name of detection pipeline<br />
<br />
|- bgcolor="ffdead" <br />
! colspan="4" | Extension 2: IMAGE, EXTNAME = PSZ2_PROBABILITY (see note 2)<br />
|- bgcolor="ffdead" <br />
! Keyword || Data Type || Value || Description<br />
|- <br />
| NAXIS1 || Integer || 256 || Dimension 1<br />
|- <br />
| NAXIS2 || Integer || 256 || Dimension 2 <br />
|- <br />
| NAXIS3 || Integer || N<sub>det</sub> || Dimension 3 = Number of detections<br />
|- bgcolor="ffdead" <br />
! Keyword || Data Type || Value || Description<br />
|- <br />
| PIPELINE || String || || Name of detection pipeline<br />
<br />
|- bgcolor="ffdead"<br />
! colspan="4" | Extension 3: IMAGE, EXTNAME = PSZ2_MSZ_ARRAY (see note 3)<br />
|- bgcolor="ffdead" <br />
! Keyword || Data Type || Value || Description<br />
|- <br />
| NAXIS1 || Integer || 100 || Dimension 1<br />
|- <br />
| NAXIS2 || Integer || 4 || Dimension 2 <br />
|- <br />
| NAXIS3 || Integer || N<sub>det</sub> || Dimension 3 = Number of detections<br />
<br />
|- bgcolor="ffdead" <br />
! Keyword || Data Type || Value || Description<br />
|- <br />
| PIPELINE || String || || Name of detection pipeline<br />
|}<br />
<br />
<br />
'''Notes'''<br />
# Format <tt>PSZ2 Glll.ll&plusmn;bb.bb</tt> where (l, b) are the Galactic coordinates truncated to 2 decimal places.<br />
# Extension 2 contains a three-dimensional image with the two-dimensional probability distribution in &theta;<sub>s</sub> and Y for each detection. The probability distributions are evaluated on a 256 &times; 256 linear grid between the limits specified in extension 1. The limits are determined independently for each detection. The dimension of the 3D image is 256 &times; 256 &times; N<sub>det</sub>, where N<sub>det</sub> is the number of detections. The first dimension is &theta;<sub>s</sub> and the second dimension is Y.<br />
# Extension 3 contains a three-dimensional image with the information on the M<sub>SZ</sub> observable per cluster as a function of assumed redshift. The image dimensions are 100 &times; 4 &times; N<sub>det</sub>, where N<sub>det</sub> is the number of detections. The first dimension is the assumed redshift. The second dimension has size 4: the first element is the assumed redshift value corresponding to the M<sub>SZ</sub> values. The second element is the M<sub>SZ</sub> lower 68% confidence bound, the third element is the M<sub>SZ</sub> estimate and the fourth element is the M<sub>SZ</sub> upper 68% confidence bound, all in units of 10<sup>14</sup>&nbsp;M<sub>sol</sub>. These uncertainties are based on the Planck measurement uncertainties only. Not included in the error estimates are the statistical errors on the scaling relation, the intrinsic scatter in the relation, or systematic errors in data selection for the scaling relation fit.<br />
<br />
=== Selection function ===<br />
<br />
The selection function for the union, intersection and individual pipeline catalogues are contained in the FITS files:<br />
* {{PLASingleFile | fileType=cat | name=HFI_PCCS_SZ-selfunc-union-survey_R2.08.fits | link=HFI_PCCS_SZ-selfunc-union-survey_R2.08.fits }} (union catalogue, survey mask)<br />
* {{PLASingleFile | fileType=cat | name=HFI_PCCS_SZ-selfunc-union-cosmolog_R2.08.fits | link=HFI_PCCS_SZ-selfunc-union-cosmology_R2.08.fits }} (union catalogue, cosmology mask)<br />
* {{PLASingleFile | fileType=cat | name=HFI_PCCS_SZ-selfunc-intersec-survey_R2.08.fits | link=HFI_PCCS_SZ-selfunc-intersec-survey_R2.08.fits }} (intersection catalogue, survey mask)<br />
* {{PLASingleFile | fileType=cat | name=HFI_PCCS_SZ-selfunc-intersec-cosmolog_R2.08.fits | link=HFI_PCCS_SZ-selfunc-intersec-cosmolog_R2.08.fits }} (intersection catalogue, cosmology mask)<br />
* {{PLASingleFile | fileType=cat | name=HFI_PCCS_SZ-selfunc-MMF1-survey_R2.08.fits | link=HFI_PCCS_SZ-selfunc-MMF1-survey_R2.08.fits }} (MMF1 catalogue, survey mask)<br />
* {{PLASingleFile | fileType=cat | name=HFI_PCCS_SZ-selfunc-MMF1-cosmolog_R2.08.fits | link=HFI_PCCS_SZ-selfunc-MMF1-cosmolog_R2.08.fits }} (MMF1 catalogue, cosmology mask)<br />
* {{PLASingleFile | fileType=cat | name=HFI_PCCS_SZ-selfunc-MMF3-survey_R2.08.fits | link=HFI_PCCS_SZ-selfunc-MMF3-survey_R2.08.fits }} (MMF3 catalogue, survey mask)<br />
* {{PLASingleFile | fileType=cat | name=HFI_PCCS_SZ-selfunc-MMF3-cosmolog_R2.08.fits | link=HFI_PCCS_SZ-selfunc-MMF3-cosmolog_R2.08.fits }} (MMF3 catalogue, cosmology mask)<br />
* {{PLASingleFile | fileType=cat | name=HFI_PCCS_SZ-selfunc-PwS-survey_R2.08.fits | link=HFI_PCCS_SZ-selfunc-PwS-survey_R2.08.fits }} (PowellSnakes catalogue, survey mask)<br />
* {{PLASingleFile | fileType=cat | name=HFI_PCCS_SZ-selfunc-PwS-cosmolog_R2.08.fits | link=HFI_PCCS_SZ-selfunc-PwS-cosmolog_R2.08.fits }} (PowellSnakes catalogue, cosmology mask)<br />
<br />
Their structure is as follows:<br />
<br />
{| border="1" cellpadding="3" cellspacing="0" align="center" style="text-align:left" width=800px<br />
|+ '''FITS file structure'''<br />
|- bgcolor="ffdead" <br />
! colspan="4" | Extension 0: Primary header, no data<br />
|- bgcolor="ffdead" <br />
! FITS Keyword || Data Type || Units || Description<br />
|- <br />
|INSTRUME || String || || Instrument (HFI)<br />
|- <br />
| VERSION || String || || Version of catalogue<br />
|- <br />
| DATE || String || || Date file created: yyyy-mm-dd<br />
|- <br />
| ORIGIN || String || || Name of organization responsible for the data (HFI-DPC)<br />
|- <br />
| TELESCOP || String || || Telescope (PLANCK)<br />
|- <br />
| CREATOR || String || || Pipeline version<br />
|- <br />
| DATE-OBS || String || || Start time of the survey: yyyy-mm-dd<br />
|- <br />
| DATE-END || String || || End time of the survey: yyyy-mm-dd<br />
|- <br />
| PROCVER || String || || Data version<br />
|- <br />
| JOIN || String || || Join type (UNION, INTERSEC, MMF1, MMF3, PwS)<br />
|- <br />
| MASK || String || || Mask name (SURVEY, COSMOLOG)<br />
<br />
|- bgcolor="ffdead" <br />
! colspan="4" | Extension 1: BINTABLE, HEALPix map (see note 1)<br />
|- bgcolor="ffdead" <br />
! FITS keyword || Data Type || Value || Description<br />
|-<br />
|PIXTYPE || String || HEALPIX || HEALPix pixelation <br />
|-<br />
|ORDERING || String || RING || Pixel ordering<br />
|-<br />
|NSIDE || Int*4 || 2048 || HEALPix resolution parameter<br />
|-<br />
|NPIX ||Int*4 || 50331648 || Number of pixels<br />
|-<br />
|COORDSYS || String || G || Coordinate system<br />
<br />
|- bgcolor="ffdead" <br />
! colspan="4" | Extension 2: IMAGE, EXTNAME = SELFUNC (see note 2)<br />
|- bgcolor="ffdead" <br />
! Keyword || Data Type || Value || Description<br />
|- <br />
| NAXIS1 || Integer || 30 || Dimension 1<br />
|- <br />
| NAXIS2 || Integer || 32 || Dimension 2 <br />
|- <br />
| NAXIS3 || Integer || 12 || Dimension 3<br />
|- bgcolor="ffdead" <br />
! Keyword || Data Type || Value || Description<br />
|- <br />
| AXIS1 || String || CY500 || Name of axis 1<br />
|- <br />
| AXIS2 || String || T500 || Name of axis 2<br />
|- <br />
| AXIS3 || String || SNRCUT || Name of axis 3<br />
|- <br />
| UNITS || String || PERCENT || Units of selection function<br />
|- <br />
| COMPTYPE || String || DIFF || Type of selection function (differential)<br />
<br />
|- bgcolor="ffdead"<br />
! colspan="4" | Extension 3: IMAGE, EXTNAME = YGRID (see note 3)<br />
|- bgcolor="ffdead" <br />
! Keyword || Data Type || Value || Description<br />
|- <br />
| NAXIS1 || Integer || 30 || Dimension 1<br />
|- bgcolor="ffdead" <br />
! Keyword || Data Type || Value || Description<br />
|- <br />
| COL1 || String || CY500 || Grid values of Y<sub>500</sub><br />
<br />
|- bgcolor="ffdead"<br />
! colspan="4" | Extension 4: IMAGE, EXTNAME = TGRID (see note 4)<br />
|- bgcolor="ffdead" <br />
! Keyword || Data Type || Value || Description<br />
|- <br />
| NAXIS1 || Integer || 32 || Dimension 1<br />
|- bgcolor="ffdead" <br />
! Keyword || Data Type || Value || Description<br />
|- <br />
| COL1 || String || T500 || Grid values of &theta;<sub>500</sub><br />
<br />
|- bgcolor="ffdead"<br />
! colspan="4" | Extension 5: IMAGE, EXTNAME = SNR_THRESH (see note 5)<br />
|- bgcolor="ffdead" <br />
! Keyword || Data Type || Value || Description<br />
|- <br />
| NAXIS1 || Integer || 12 || Dimension 1<br />
|- bgcolor="ffdead" <br />
! Keyword || Data Type || Value || Description<br />
|- <br />
| COL1 || String || S/N || Grid values of S/N threshold<br />
<br />
|}<br />
<br />
'''Notes'''<br />
# Extension 1 contains a mask defining the survey region, given by an N<sub>side</sub> = 2048 ring-ordered HEALPix map in GALACTIC coordinates. Pixels in the survey region have the value 1.0 while pixels outside of the survey region have value 0.0.<br />
# Extension 2 contains a three-dimensional image containing the survey completeness probability distribution for various S/N thresholds. The information is stored in an image of size 30 &times; 32 &times; 12. The first dimension is Y<sub>500</sub>, the second dimension is &theta;<sub>500</sub> and the third dimension is the signal-to-noise threshold. The units are percent and lie in the range 0-100 and denote the detection probability of a cluster in the given (Y<sub>500</sub>, &theta;<sub>500</sub>) bin.<br />
# Extension 3 contains the Y<sub>500</sub> grid values for the completeness data cube in the second extension. It has length 30 and spans the range from 1.12480 &times; 10<sup>-4</sup> arcmin<sup>2</sup> to 7.20325 &times; 10<sup>-2</sup> arcmin<sup>2</sup> in logarithmic steps.<br />
# Extension 4 contains the θ<sub>500</sub> grid values for the completeness data cube in the second extension. It has length 32 and spans the range from 0.9416 arcmin to 35.31 arcmin in logarithmic steps.<br />
# Extension 5 contains the signal-to-noise threshold grid values for the completeness data cube in the second extension. It has length 12 and contains thresholds from 4.5 to 10.0 in steps of 0.5.<br />
<br />
==Planck Catalogue of Galactic Cold Clumps==<br />
<br />
The Planck Catalogue of Galactic Cold Clumps (PGCC) is a list of 13188 Galactic sources and 54 sources located in the Small and Large Magellanic Clouds. The sources have been identified in Planck data as sources colder than their environment. It has been buit using the 48 months Planck data at 857, 545, and 353 GHz combined with the 3 THz IRAS data, as it is described in {{PlanckPapers | planck2014-a37}}.<br />
<br />
The all-sky distribution of the PGCC sources is shown below on top of the 857 GHz emission shown in logarithmic scale between 10<sup>-2</sup> to 10<sup>2</sup> MJy/sr.<br />
[[File:PGCC_allsky.png|800px|thumb|center|All-sky distribution of the PGCC sources.]]<br />
<br />
Sources are divided into three categories based on the reliability of the flux density estimates in IRAS 3 THz and Planck 857, 545, and 353 GHz bands.<br />
* FLUX_QUALITY=1 : sources with flux density estimates S/N > 1 in all bands ;<br />
* FLUX_QUALITY=2 : sources with flux density estimates S/N > 1 only in 857, 545, and 353 GHz Planck bands, considered as very cold source candidates ;<br />
* FLUX_QUALITY=3 : sources without any reliable flux density estimates, listed as poor candidates.<br />
The all-sky distributions of the PGCC sources per FLUX_QUALITY category are shown below on top of the 857 GHz map in grey scale shown in logarithmic scale between 10<sup>-2</sup> to 10<sup>2</sup> MJy/sr.<br />
[[File:PGCC_allsky_FQ1.png|800px|thumb|center|All-sky distribution of the PGCC sources with FLUX_QUALITY=1.]]<br />
[[File:PGCC_allsky_FQ2.png|800px|thumb|center|All-sky distribution of the PGCC sources with FLUX_QUALITY=2.]]<br />
[[File:PGCC_allsky_FQ3.png|800px|thumb|center|All-sky distribution of the PGCC sources with FLUX_QUALITY=3.]]<br />
<br />
Distance estimates have been obtained on 5574 PGCC sources using seven different methods/technics, as described in {{PlanckPapers | planck2014-a37}}. A flag is raised to quantify the quality of the distance estimates, defined as follows:<br />
* DIST_QUALITY=0 : No distance estimate ;<br />
* DIST_QUALITY=1 : Single distance estimate ;<br />
* DIST_QUALITY=2 : Multiple distance estimates which are consistent within 1<math>\sigma</math> ;<br />
* DIST_QUALITY=3 : Multiple distance estimates which are not consistent within 1<math>\sigma</math> ;<br />
* DIST_QUALITY=4 : Single upper limits.<br />
The all-sky distribution of the sources with robust distance estimates is shown below.<br />
[[File:PGCC_allsky_DIST.png|800px|thumb|center|All-sky distribution of the 4655 PGCC sources for which a distance estimate with a DIST_QUALITY flag equal to 1 or 2 is available. The various types of distance estimates are defined as follows : kinematic (purple), optical extinction (blue), near-infrared extinction (green), molecular complex association (orange), and Herschel HKP-GCC (red). We also show the distribution of the 664 sources with an upper-limit estimate (DIST_QUALITY=4) provided by the near-infrared extinction method (light green). Molecular complexes are outlined with black contours.]]<br />
<br />
The catalogue is contained in the FITS file {{PLASingleFile | fileType=cat | name=HFI_PCCS_GCC_R2.02.fits | link=HFI_PCCS_GCC_R2.02.fits }}. <br />
It structure is as follows:<br />
<br />
{| border="1" cellpadding="3" cellspacing="0" align="center" style="text-align:left" width=1000px<br />
|+ '''FITS file structure'''<br />
|- bgcolor="ffdead" <br />
! colspan="4" | Identification<br />
|- bgcolor="ffdead" <br />
! FITS Keyword || Data Type || Units || Description<br />
|- <br />
|NAME || String || || Source Name<br />
|- <br />
|SNR || real*8 || || Maximum S/N over the 857, 545, and 353 GHz Planck cold residual maps<br />
|- <br />
|SNR_857 || real*8 || || S/N of the cold residual detection at 857 GHz<br />
|- <br />
|SNR_545 || real*8 || || S/N of the cold residual detection at 545 GHz<br />
|- <br />
|SNR_353 || real*8 || || S/N of the cold residual detection at 353 GHz<br />
|- bgcolor="ffdead" <br />
! colspan="4" | Source position<br />
|- bgcolor="ffdead" <br />
! FITS Keyword || Data Type || Units || Description<br />
|- <br />
|GLON || real*8 || deg || Galactic longitude based on morphology fitting<br />
|- <br />
|GLAT || real*8 || deg || Galactic latitude based on morphology fitting<br />
|- <br />
|RA || real*8 || deg || Right ascension (J2000) in degrees transformed from (GLON, GLAT)<br />
|- <br />
|DEC || real*8 || deg || Declination (J2000) in degrees transformed from (GLON, GLAT)<br />
|- bgcolor="ffdead" <br />
! colspan="4" | Morphology<br />
|- bgcolor="ffdead" <br />
! FITS Keyword || Data Type || Units || Description<br />
|- <br />
|GAU_MAJOR_AXIS || real*8 || arcmin || FWHM along the major axis of the elliptical Gaussian<br />
|- <br />
|GAU_MAJOR_AXIS_SIG || real*8 || arcmin || 1<math>\sigma</math> uncertainty on the FWHM along the major axis<br />
|- <br />
|GAU_MINOR_AXIS || real*8 || arcmin || FWHM along the minor axis of the elliptical Gaussian<br />
|- <br />
|GAU_MINOR_AXIS_SIG || real*8 || arcmin || 1<math>\sigma</math> uncertainty on the FWHM along the minor axis<br />
|- <br />
|GAU_POSITION_ANGLE || real*8 || rad || Position angle of the elliptical gaussian (see note 1) <br />
|- <br />
|GAU_POSITION_ANGLE_SIG || real*8 || rad || 1<math>\sigma</math> uncertainty on the position angle<br />
|- bgcolor="ffdead" <br />
! colspan="4" | Photometry<br />
|- bgcolor="ffdead" <br />
! FITS Keyword || Data Type || Units || Description<br />
|- <br />
|FLUX_3000_CLUMP || real*8 || Jy || Flux density of the clump at 3 THz<br />
|- <br />
|FLUX_3000_CLUMP_SIG || real*8 || Jy || 1<math>\sigma</math> uncertainty on the flux density of the clump at 3 THz<br />
|- <br />
|FLUX_857_CLUMP || real*8 || Jy || Flux density of the clump at 857 GHz<br />
|- <br />
|FLUX_857_CLUMP_SIG || real*8 || Jy || 1<math>\sigma</math> uncertainty on the flux density of the clump at 857 GHz<br />
|- <br />
|FLUX_545_CLUMP || real*8 || Jy || Flux density of the clump at 545 GHz<br />
|- <br />
|FLUX_545_CLUMP_SIG || real*8 || Jy || 1<math>\sigma</math> uncertainty on the flux density of the clump at 545 GHz<br />
|- <br />
|FLUX_353_CLUMP || real*8 || Jy || Flux density of the clump at 353 GHz<br />
|- <br />
|FLUX_353_CLUMP_SIG || real*8 || Jy || 1<math>\sigma</math> uncertainty on the flux density of the clump at 353 GHz<br />
|- <br />
|FLUX_3000_WBKG || real*8 || Jy || Flux density of the warm background at 3 THz (see note 2)<br />
|- <br />
|FLUX_3000_WBKG_SIG || real*8 || Jy || 1<math>\sigma</math> uncertainty on the flux density of warm background at 3 THz<br />
|- <br />
|FLUX_857_WBKG || real*8 || Jy || Flux density of the warm background at 857 GHz<br />
|- <br />
|FLUX_857_WBKG_SIG || real*8 || Jy || 1<math>\sigma</math> uncertainty on the flux density of the warm background at 857 GHz<br />
|- <br />
|FLUX_545_WBKG || real*8 || Jy || Flux density of the warm background at 545 GHz<br />
|- <br />
|FLUX_545_WBKG_SIG || real*8 || Jy || 1<math>\sigma</math> uncertainty on the flux density of the warm background at 545 GHz<br />
|- <br />
|FLUX_353_WBKG || real*8 || Jy || Flux density of the warm background at 353 GHz<br />
|- <br />
|FLUX_353_WBKG_SIG || real*8 || Jy || 1<math>\sigma</math> uncertainty on the flux density of the warm background at 353 GHz<br />
|- <br />
|FLUX_QUALITY || int*4 || 1-3 || Category of flux density reliability (see note 3)<br />
|- <br />
|FLUX_BLENDING || int*4 || 0/1 || 1 if blending issue with flux density estimate (see note 4)<br />
|- <br />
|FLUX_BLENDING_IDX || int*8 || || Catalogue index of the closest source responsible for blending<br />
|- <br />
|FLUX_BLENDING_ANG_DIST || real*8 || arcmin || Angular distance to the closest source responsible for blending<br />
|- <br />
|FLUX_BLENDING_BIAS_3000 || real*8 || % || Relative bias of the flux density at 3000 GHz due to blending<br />
|- <br />
|FLUX_BLENDING_BIAS_857 || real*8 || % || Relative bias of the flux density at 857 GHz due to blending<br />
|- <br />
|FLUX_BLENDING_BIAS_545 || real*8 || % || Relative bias of the flux density at 545 GHz due to blending<br />
|- <br />
|FLUX_BLENDING_BIAS_353 || real*8 || % || Relative bias of the flux density at 353 GHz due to blending<br />
|- bgcolor="ffdead" <br />
! colspan="4" | Distance<br />
|- bgcolor="ffdead" <br />
! FITS Keyword || Data Type || Units || Description<br />
|- <br />
|DIST_KINEMATIC || real*8 || kpc || Distance estimate [1] using kinematics<br />
|- <br />
|DIST_KINEMATIC_SIG || real*8 || kpc || 1<math>\sigma</math> uncertainty on the distance estimate [1] using kinematics<br />
|- <br />
|DIST_OPT_EXT_DR7 || real*8 || kpc || Distance estimate [2] using optical extinction on SDSS DR7<br />
|- <br />
|DIST_OPT_EXT_DR7_SIG || real*8 || kpc || 1<math>\sigma</math> uncertainty on the distance estimate [2] using optical extinction on SDSS DR7<br />
|- <br />
|DIST_OPT_EXT_DR9 || real*8 || kpc || Distance estimate [3] using optical extinction on SDSS DR9<br />
|- <br />
|DIST_OPT_EXT_DR9_SIG || real*8 || kpc || 1<math>\sigma</math> uncertainty on the distance estimate [3] using optical extinction on SDSS DR9<br />
|- <br />
|DIST_NIR_EXT_IRDC || real*8 || kpc || Distance estimate [4] using near-infrared extinction towards IRDCs<br />
|- <br />
|DIST_NIR_EXT_IRDC_SIG || real*8 || kpc || 1<math>\sigma</math> uncertainty on the distance estimate [4] using near-infrared extinction towards IRDCs<br />
|- <br />
|DIST_NIR_EXT || real*8 || kpc || Distance estimate [5] using near-infrared extinction<br />
|- <br />
|DIST_NIR_EXT_SIG || real*8 || kpc || 1<math>\sigma</math> uncertainty on the distance estimate [5] using near-infrared extinction<br />
|- <br />
|DIST_MOLECULAR_COMPLEX || real*8 || kpc || Distance estimate [6] using molecular complex association<br />
|- <br />
|DIST_MOLECULAR_COMPLEX_SIG || real*8 || kpc || 1<math>\sigma</math> uncertainty on the distance estimate [6] using molecular complex association<br />
|- <br />
|DIST_HKP_GCC || real*8 || kpc || Distance estimate [7] from the Herschel Key-Programme Galactic Cold Cores<br />
|- <br />
|DIST_HKP_GCC_SIG || real*8 || kpc || 1<math>\sigma</math> uncertainty on the distance estimate [7] from the Herschel Key-Programme Galactic Cold Cores<br />
|- <br />
|DIST_OPTION || int*4 || 0-7 || Option of the best distance estimate used in other physical properties<br />
|- <br />
|DIST_QUALITY || int*4 || 0-4 || Quality Flag of the consistency between distance estimates (see note 5)<br />
|- <br />
|DIST || real*8 || kpc || Best distance estimate used for further physical properties<br />
|- <br />
|DIST_SIG || real*8 || kpc || 1<math>\sigma</math> uncertainty on the best distance estimate <br />
|- bgcolor="ffdead" <br />
! colspan="4" | Temperature<br />
|- bgcolor="ffdead" <br />
! FITS Keyword || Data Type || Units || Description<br />
|- <br />
|TEMP_CLUMP || real*8 || K || Temperature of the clump with <math>\beta</math> as a free parameter<br />
|- <br />
|TEMP_CLUMP_SIG || real*8 || K || 1<math>\sigma</math> uncertainty on the clump temperature with <math>\beta</math> free <br />
|- <br />
|TEMP_CLUMP_LOW1 || real*8 || K || Lower 68% confidence limit of the clump temperature with <math>\beta</math> free <br />
|- <br />
|TEMP_CLUMP_UP1 || real*8 || K || Upper 68% confidence limit of the clump temperature with <math>\beta</math> free <br />
|- <br />
|BETA_CLUMP || real*8 || || Spectral index <math>\beta</math> of the clump<br />
|- <br />
|BETA_CLUMP_SIG || real*8 || || 1<math>\sigma</math> uncertainty (from MCMC) on the emissivity spectral index <math>\beta</math> of the clump<br />
|- <br />
|BETA_CLUMP_LOW1 || real*8 || || Lower 68% confidence limit of the emissivity spectral index <math>\beta</math> of the clump<br />
|- <br />
|BETA_CLUMP_UP1 || real*8 || || Upper 68% confidence limit of the emissivity spectral index <math>\beta</math> of the clump<br />
|- <br />
|TEMP_BETA2_CLUMP || real*8 || K || Temperature of the clump with <math>\beta</math> = 2<br />
|- <br />
|TEMP_BETA2_CLUMP_SIG || real*8 || K || 1<math>\sigma</math> uncertainty on the temperature of the clump with <math>\beta</math> = 2<br />
|- <br />
|TEMP_BETA2_CLUMP_LOW1 || real*8 || K || Lower 68% confidence limit of the clump temperature with <math>\beta</math> = 2<br />
|- <br />
|TEMP_BETA2_CLUMP_UP1 || real*8 || K || Upper 68% confidence limit of the clump temperature with <math>\beta</math> = 2<br />
|- <br />
|TEMP_WBKG || real*8 || K || Temperature of the warm background with <math>\beta</math> as a free parameter (see note 6)<br />
|- <br />
|TEMP_WBKG_SIG || real*8 || K || 1<math>\sigma</math> dispersion of the warm background temperature with <math>\beta</math> free <br />
|- <br />
|TEMP_WBKG_LOW1 || real*8 || K || Lower 68% confidence limit of the warm background temperature with <math>\beta</math> free <br />
|- <br />
|TEMP_WBKG_UP1 || real*8 || K || Upper 68% confidence limit of the warm background temperature with <math>\beta</math> free <br />
|- <br />
|BETA_WBKG || real*8 || || Spectral index <math>\beta</math> of the warm background (see note 6)<br />
|- <br />
|BETA_WBKG_SIG || real*8 || || 1<math>\sigma</math> uncertainty (from MCMC) of the emissivity spectral index <math>\beta</math> of the warm background<br />
|- <br />
|BETA_WBKG_LOW1 || real*8 || || Lower 68% confidence limit of the emissivity spectral index <math>\beta</math> of the warm background<br />
|- <br />
|BETA_WBKG_UP1 || real*8 || || Upper 68% confidence limit of the emissivity spectral index <math>\beta</math> of the warm background<br />
|- <br />
|TEMP_BETA2_WBKG || real*8 || K || Temperature of the warm background with <math>\beta</math> = 2<br />
|- <br />
|TEMP_BETA2_WBKG_SIG || real*8 || K || 1<math>\sigma</math> uncertainty on the temperature of the warm background with <math>\beta</math> = 2<br />
|- <br />
|TEMP_BETA2_WBKG_LOW1 || real*8 || K || Lower 68% confidence limit of the warm background temperature with <math>\beta</math> = 2<br />
|- <br />
|TEMP_BETA2_WBKG_UP1 || real*8 || K || Upper 68% confidence limit of the warm background temperature with <math>\beta</math> = 2<br />
|- bgcolor="ffdead" <br />
! colspan="4" | Physical properties<br />
|- bgcolor="ffdead" <br />
! FITS Keyword || Data Type || Units || Description<br />
|- <br />
|NH2 || real*8 || cm<sup>-2</sup> || Column density <math>N_{H_2}</math> of the clump<br />
|- <br />
|NH2_SIG || real*8 || cm<sup>-2</sup> || 1<math>\sigma</math> uncertainty on the column density<br />
|- <br />
|NH2_LOW[1,2,3] || real*8 || cm<sup>-2</sup> || Lower 68%, 95% and 99% confidence limit of the column density<br />
|- <br />
|NH2_UP[1,2,3] || real*8 || cm<sup>-2</sup> || Upper 68%, 95% and 99% confidence limit of the column density<br />
|- <br />
|MASS || real*8 || <math>M_{o}</math> || Mass estimate of the clump<br />
|- <br />
|MASS_SIG || real*8 || <math>M_{o}</math> || 1<math>\sigma</math> uncertainty on the mass estimate of the clump<br />
|- <br />
|MASS_LOW[1,2,3] || real*8 || <math>M_{o}</math> || Lower 68%, 95% and 99% confidence limit of the mass estimate<br />
|- <br />
|MASS_UP[1,2,3] || real*8 || <math>M_{0}</math> || Upper 68%, 95% and 99% confidence limit of the mass estimate<br />
|- <br />
|DENSITY || real*8 || cm<sup>-3</sup> || Mean density of the clump<br />
|- <br />
|DENSITY_SIG || real*8 || cm<sup>-3</sup> || 1<math>\sigma</math> uncertainty on the mean density estimate of the clump<br />
|- <br />
|DENSITY_LOW[1,2,3] || real*8 || cm<sup>-3</sup> || Lower 68%, 95% and 99% confidence limit of the mean density estimate<br />
|- <br />
|DENSITY_UP[1,2,3] || real*8 || cm<sup>-3</sup> || Upper 68%, 95% and 99% confidence limit of the mean density estimate<br />
|- <br />
|SIZE || real*8 || pc || Physical size of the clump <br />
|- <br />
|SIZE_SIG || real*8 || pc || 1<math>\sigma</math> uncertainty on the physical size estimate of the clump<br />
|- <br />
|SIZE_LOW[1,2,3] || real*8 || pc || Lower 68%, 95% and 99% confidence limit of the physical size estimate<br />
|- <br />
|SIZE_UP[1,2,3] || real*8 || pc || Upper 68%, 95% and 99% confidence limit of the physical size estimate<br />
|- <br />
|LUMINOSITY || real*8 || L<sub>o</sub> || Luminosity of the clump<br />
|- <br />
|LUMINOSITY_SIG || real*8 || L<sub>o</sub> || 1<math>\sigma</math> uncertainty on the luminosity estimate of the clump<br />
|- <br />
|LUMINOSITY_LOW[1,2,3] || real*8 || L<sub>o</sub> || Lower 68%, 95% and 99% confidence limit of the luminosity estimate<br />
|- <br />
|LUMINOSITY_UP[1,2,3] || real*8 || L<sub>o</sub> || Upper 68%, 95% and 99% confidence limit of the luminosity estimate<br />
|- bgcolor="ffdead" <br />
! colspan="4" | Flags<br />
|- bgcolor="ffdead" <br />
! FITS Keyword || Data Type || Units || Description<br />
|- <br />
|XFLAG_LMC || int*4 || 0/1 || 1 if part of the LMC<br />
|- <br />
|XFLAG_SMC || int*4 || 0/1 || 1 if part of the SMC<br />
|- <br />
|XFLAG_ECC || int*4 || 0/1 || 1 if present in the ECC<br />
|- <br />
|XFLAG_PCCS_857 || int*4 || 0/1 || 1 if present in the PCCS 857 GHz band<br />
|- <br />
|XFLAG_PCCS_545 || int*4 || 0/1 || 1 if present in the PCCS 545 GHz band<br />
|- <br />
|XFLAG_PCCS_353 || int*4 || 0/1 || 1 if present in the PCCS 353 GHz band<br />
|- <br />
|XFLAG_PCCS_217 || int*4 || 0/1 || 1 if present in the PCCS 217 GHz band<br />
|- <br />
|XFLAG_PCCS_143 || int*4 || 0/1 || 1 if present in the PCCS 143 GHz band<br />
|-<br />
|XFLAG_PCCS_100 || int*4 || 0/1 || 1 if present in the PCCS 100 GHz band<br />
|-<br />
|XFLAG_PCCS_70 || int*4 || 0/1 || 1 if present in the PCCS 70 GHz band<br />
|-<br />
|XFLAG_PCCS_44 || int*4 || 0/1 || 1 if present in the PCCS 44 GHz band<br />
|-<br />
|XFLAG_PCCS_30 || int*4 || 0/1 || 1 if present in the PCCS 30 GHz band<br />
|-<br />
|XFLAG_PSZ || int*4 || 0/1 || 1 if present in the PCCS PSZ<br />
|-<br />
|XFLAG_PHZ || int*4 || 0/1 || 1 if present in the PCCS HZ<br />
|-<br />
|XFLAG_HKP_GCC || int*4 || 0/1 || 1 if present in the Herschel HKP-GCC<br />
<br />
|}<br />
<br />
<br />
Notes:<br />
* 1: The position angle of the 2D ellipse is defined as the angle between the axis parallele to the Galactic plane and the major axis, counted clockwise.<br />
* 2: The warm bakcground flux densities are computed using the same solid angle as for the clumps flux densities, but on the warm conponent map.<br />
* 3: See text above for a full description of the FLUX_QUALITY flag, for which 1 is best.<br />
* 4: This relative bias due to blending provides a rough estimate of the factor that should be applied on the clumpds flux densities to get a corrected estimate. It has been obtained on a very simple modelling of clumps morphology and the local environment. It has therefore to be taken very carefully.<br />
* 5: See text above for a full description of the DIST_QUALITY flag.<br />
* 6: Temperature and spectral index of the warm background are based on the warm background flux density estimates obtained on the same solid angle used for clumps<br />
<br />
==References==<br />
<References /> <br />
<br />
[[Category:Mission products|005]]</div>
Xdupac
https://wiki.cosmos.esa.int/planckpla2015/index.php?title=CMB_spectrum_%26_Likelihood_Code&diff=11459
CMB spectrum & Likelihood Code
2015-05-06T09:30:54Z
<p>Xdupac: /* File names and Meta data */</p>
<hr />
<div>{{DISPLAYTITLE:2015 CMB spectra and likelihood code}}<br />
<br />
==2015 CMB spectra==<br />
<br />
<br />
===General description===<br />
====TT====<br />
The Planck best-fit CMB temperature power spectrum, shown in the figure below, covers the wide range of multipoles <math> \ell </math> = 2-2508. Over the multipole range <math> \ell </math> = 2–29, the power spectrum is derived from the ''Commander'': component separation algorithm applied to the combination of Planck 2015 temperature data between 30 and 857 GHz, the 9-year WMAP sky maps, and the 408 MHz Haslam et al. (1982) survey, including 93% of the sky {{PlanckPapers|planck2014-a12}} . The asymmetric error bars associated to this spectrum are the 68% confidence limits and include the uncertainties due to foreground subtraction.<br />
<br />
For multipoles equal or greater than <math>\ell=30</math>, instead, the spectrum is derived from the ''Plik'' likelihood {{PlanckPapers|planck2014-a13}} by optimally combining the spectra in the frequency range 100-217 GHz, and correcting them for unresolved foregrounds using the best-fit foreground solution from a Planck TT+lowP <math>\Lambda</math>CDM run. Associated 1-sigma errors include beam uncertainties. Both ''Commander'' and ''Plik'' are described in more details in the sections below.<br />
<br />
[[File: A15_TT.png|thumb|center|700px|'''The Planck 2015 TT power spectrum. Logarithmic x-scale up to <math>\ell = 30 </math> , linear at higher <math>\ell</math>. The red line is the Planck best-fit primordial power spectrum (cf Planck TT+lowP in Table 3 of Planck-2015-A15[3]). Residuals with respect to this model are shown in the lower panel. The error bars show <math>\pm 1\sigma</math> uncertainties.''']]<br />
<br />
====TE and EE====<br />
The Planck best-fit CMB polarization and temperature-polarization cross-correlation power spectra, shown in the figure below, cover the multipole range <math> \ell </math> = 30-1996. The data points relative to the multipole range <math> \ell </math> = 2-29 will be released at a later time.<br />
Analogously to the TT case, the <math> \ell\ge 30 </math> spectrum is derived from the ''Plik'' likelihood {{PlanckPapers|planck2014-a13}} by optimally combining the spectra in the frequency range 100-217 GHz, and correcting them for unresolved foregrounds using the best-fit foreground solution from a Planck TT,TE,EE+lowP <math>\Lambda</math>CDM run. <br />
<br />
{|style="margin: 0 auto;"<br />
|[[File: A15_EE.png|thumb|center|500px|'''The Planck 2015 EE power spectrum. The red line is the Planck best-fit primordial power spectrum (cf Planck TT+lowP in Table 3 of Planck-2015-A15). Residuals with respect to this model are shown in the lower panel. The error bars show <math>\pm 1\sigma</math> uncertainties. The green lines in the lower panels show the best-fit temperature-to-polarization leakage model of Eqs. (11a) and (11b) in Planck-2015-A15.''']]<br />
|[[File: A15_TE.png|thumb|center|500px|'''The Planck 2015 TE power spectrum. The red line is the Planck best-fit primordial power spectrum (cf Planck TT+lowP in Table 3 of Planck-2015-A15). Residuals with respect to this model are shown in the lower panel. The error bars show <math>\pm 1\sigma</math> uncertainties. The green lines in the lower panels show the best-fit temperature-to-polarization leakage model of Eqs. (11a) and (11b) in Planck-2015-A15.''']]<br />
|}<br />
<br />
===Production process===<br />
The <math>\ell</math> < 30 part of the Planck TT power spectrum is derived from the Commander approach, which implements Bayesian component separation in pixel space, fitting a parametric model to the data by sampling the posterior distribution for the model parameters {{PlanckPapers|planck2014-a12}}. The power spectrum at any multipole <math>\ell</math> is given as the maximum probability point for the posterior <math>C_\ell</math> distribution, marginalized over the other multipoles, and the error bars are 68% confidence level; see {{PlanckPapers|planck2014-a12}}. <br />
<br />
The <math>\ell \ge 30</math> part of the TT, TE and EE power spectra have been derived by the Plik likelihood, a code that implements a pseudo-Cl based technique, extensively described in Sec. 2 and the Appendix of {{PlanckPapers|planck2013-p08}} and {{PlanckPapers|planck2014-a13}}. Frequency spectra are computed as cross-spectra between half-mission maps. Mask and multipole range choices for each frequency spectrum are summarized in Section 3.3 of {{PlanckPapers|planck2014-a15}} and in {{PlanckPapers|planck2014-a13}}. The final power spectrum is an optimal combination of the 100, 143, 143x217 and 217 GHz spectra, corrected for the best-fit unresolved foregrounds and inter-frequency calibration factors, as derived from the full likelihood analysis (for TT we use the best-fit solutions for the nuisance parameters from the Planck+TT+lowP data combination, while for TE and EE we use the best fit from Planck+TT+lowP, cf Table 3 of {{PlanckPapers|planck2014-a15}}). A thorough description of the models of unresolved foregrounds is given in {{PlanckPapers|planck2014-a13}}. The spectrum covariance matrix accounts for cosmic variance and noise contributions, together with beam uncertainties. The <math>\ell \ge 30</math> CMB TT spectrum and associated covariance matrix are available in two formats:<br />
#Unbinned. TT: 2479 bandpowers (<math>\ell=30-2508</math>); TE or EE: 1697 bandpowers (<math>\ell=30-1996</math>).<br />
#Binned, in bins of <math> \Delta\ell=30 </math>. TT: 83 bandpowers. TE or EE: 66 bandpowers. We bin the <math> C_\ell </math> power spectrum with a weight proportional to <math> \ell (\ell+1) </math>, so that the <math> C_{\ell_b} </math> binned bandpower centered in <math> \ell_b </math> is: <math> \\ C_{\ell_b}=\Sigma_{\ell \in b} w_{\ell_b\ell} C_\ell \quad \text{with} \quad w_{\ell_b\ell}=\frac{\ell (\ell+1)}{\Sigma_{\ell \in b} \ell (\ell+1)}. \\</math> Equivalently, using the matrix formalism, we can construct the binning matrix B as: <math>\\ B_{\ell_b \ell}=w_{\ell_b\ell} \\ </math> where B is a <math> n_b\times n_\ell</math> matrix, with <math>n_b=83</math> the number of bins and <math>n_\ell=2479</math> the number of unbinned multipoles. Thus: <math> \\ \vec{C}_\mathrm{binned}=B \, \vec{C} \\ \mathrm{cov_\mathrm{binned}}= B\, \mathrm{cov}\, B^T \\ \ell_b=B\, \ell \\ </math> Here, <math> \vec{C}_{binned}\, (\vec{C}) </math> is the vector containing all the binned (unbinned) <math>C_\ell</math> bandpowers, <math>\mathrm{cov} </math> is the covariance matrix and <math>\ell_b</math> is the weighted average multipole in each bin. Note that following this definition, <math>\ell_b</math> can be a non-integer. The binned <math>D_{\ell_B}</math> power spectrum is then calculated as: <math> \\ D_{\ell_b}=\frac{\ell_b (\ell_b+1)}{2\pi} C_{\ell_b} </math>.<br />
<br />
===Inputs===<br />
<br />
; Low-l spectrum (<math>\ell < 30</math>):<br />
* Planck 30 and 44 GHz frequency maps<br />
* Planck 70 to 857 GHz detector and detector set maps<br />
* 9-year WMAP temperature sky maps between 23 and 94 GHz<br />
* 408 MHz survey by Haslam et al. (1982) <br />
* Commander <math>\chi^2</math> based LM93 confidence mask {{PlanckPapers|planck2014-a12}}<br />
<br />
; High-l spectrum (<math>30 \le \ell \le 2508</math>): <br />
<br />
* 100, 143, 143x217 and 217 GHz spectra and their covariance matrix (Sec. 3.3 {{PlanckPapers|planck2014-a15}})<br />
* best-fit foreground templates and inter-frequency calibration factors (Table 3 of {{PlanckPapers|planck2014-a15}})<br />
* Beam transfer function uncertainties {{PlanckPapers|planck2014-a08}}<br />
=== File names and Meta data ===<br />
<br />
The CMB spectrum and its covariance matrix are distributed in a single FITS file named <br />
<!--- * ''{{PLASingleFile | fileType=cosmo | name=COM_PowerSpect_CMB_R2.00.fits | link=COM_PowerSpect_CMB_R1.10.fits}}'' ---><br />
* ''COM_PowerSpect_CMB_R2.nn.fits''<br />
which contains 7 ''BINTABLE'' extensions<br />
<br />
; 1. TT low-ell, unbinned (TTLOLUNB)<br />
: with the low ell part of the spectrum, not binned, and for l=2-29. The table columns are<br />
# ''ELL'' (integer): multipole number<br />
# ''D_ELL'' (float): <math>D_ell</math> as described above<br />
# ''ERRUP'' (float): the upward uncertainty<br />
# ''ERRDOWN'' (float): the downward uncertainty<br />
<br />
; 2. TT high-ell, binned (TTHILBIN)<br />
: with the high-ell part of the spectrum, binned into 83 bins covering <math>\langle l \rangle = 47-2499\ </math> in bins of width <math>l=30</math> (with the exception of the last bin that is smaller). The table columns are as follows:<br />
# ''ELL'' (float): mean multipole number of bin<br />
# ''L_MIN'' (integer): lowest multipole of bin<br />
# ''L_MAX'' (integer): highest multipole of bin<br />
# ''D_ELL'' (float): <math>D_\ell</math> as described above<br />
# ''ERR'' (float): the uncertainty<br />
<br />
; 3. TT high-ell unbinned (TTHILUNB) <br />
: with the high-ell part of the spectrum, unbinned, in 2979 bins covering <math>\langle l \rangle = 30-2508\ </math>. The table columns are as follows:<br />
# ''ELL'' (integer): multipole <br />
# ''D_ELL'' (float): <math>D_\ell</math> as described above<br />
# ''ERR'' (float): the uncertainty<br />
<br />
; 4. TE high-ell, binned (TEHILBIN) <br />
: with the high-ell part of the spectrum, binned into 83 bins covering <math>\langle l \rangle = 47-1988\ </math> in bins of width <math>l=30</math> (with the exception of the last bin that is smaller). The table columns are as follows:<br />
# ''ELL'' (float): mean multipole number of bin<br />
# ''L_MIN'' (integer): lowest multipole of bin<br />
# ''L_MAX'' (integer): highest multipole of bin<br />
# ''D_ELL'' (float): <math>D_\ell</math> as described above<br />
# ''ERR'' (float): the uncertainty<br />
<br />
; 5. TE high-ell, unbinned (TEHILUNB) <br />
: with the high-ell part of the spectrum, unbinned, in 2979 bins covering <math>\langle l \rangle = 30-1996\ </math>. The table columns are as follows:<br />
# ''ELL'' (integer): multipole <br />
# ''D_ELL'' (float): <math>D_\ell</math> as described above<br />
# ''ERR'' (float): the uncertainty<br />
<br />
; 6. EE high-ell, binned (EEHILBIN) <br />
: with the high-ell part of the spectrum, binned into 83 bins covering <math>\langle l \rangle = 47-1988\ </math> in bins of width <math>l=30</math> (with the exception of the last bin that is smaller). The table columns are as follows:<br />
# ''ELL'' (float): mean multipole number of bin<br />
# ''L_MIN'' (integer): lowest multipole of bin<br />
# ''L_MAX'' (integer): highest multipole of bin<br />
# ''D_ELL'' (float): <math>D_\ell</math> as described above<br />
# ''ERR'' (float): the uncertainty<br />
<br />
; 7. EE high-ell, unbinned (EEHILUNB) <br />
: with the high-ell part of the spectrum, unbinned, in 2979 bins covering <math>\langle l \rangle = 30-1996\ </math>. The table columns are as follows:<br />
# ''ELL'' (integer): multipole <br />
# ''D_ELL'' (float): <math>D_\ell</math> as described above<br />
# ''ERR'' (float): the uncertainty<br />
<br />
Note that R2.00 of these files contained a small error in that the ''effective'' <math>\ell</math> of the bin in the binned data was truncated to an integer. While the <math>\ell</math> values of the unbinned (full) data are indeed integer, the ''effective'' <math>\ell</math> of the binned data is a weighted average of the <math>\ell</math>'s used in the bin and it should be a real number. This is corrected in R2.01.<br />
<br />
The spectra give <math>D_\ell = \ell(\ell+1)C_\ell / 2\pi </math> in units of <math>\mu\, K^2</math>. The covariance matrices of the spectra will be released at a later time.<br />
<br />
The CMB spectra are also given in seven simple text files, corresponding to each of the FITS file BINTABLE extensions described above.<br />
<br />
==Likelihood==<br />
The likelihood code will released in March-April 2015 with an accompanying paper and an Explanatory Supplement update. <br />
<!-- <br />
===Likelihood===<br />
<span style="color:red"> ALL OF THE FOLLOWING IN THE LIKELIHOOD SECTION IS OLD. </span><br />
The likelihood code (and the data that comes with it) used to compute the likelihood of a model that predicts the CMB power spectra, lensing power spectrum, together with some foreground and some instrumental parameters. The data files are built primarily from the Planck mission results, but include also some results from the WMAP-9 data release. The data files are written in a specific format that can only be read by the code. The code consists in a c/f90 library, along with some optional tools in python. The code is used to read the data files, and given model power spectra and nuisance parameters it computes the log likelihood of that model. <br />
<br />
Detailed description of the installation and usage of the likelihood code and data is provided in the package. The package includes five data files: four for the CMB likelihoods and one for the lensing likelihood. All of the likelihoods delivered are described in detail in the {{PlanckPapers|planck2013-p08|1|Power spectrum & Likelihood Paper}} (for the CMB based likelihood) and in the {{PlanckPapers|planck2013-p12|1|Lensing Paper}} (for the lensing likelihood) .<br />
<br />
The CMB full likelihood has been divided into four parts to allow using selectively different ranges of multipoles. It also reflects the fact that the mathematical approximations used for those different parts are very different, as is the underlying data. In detail, we distribute<br />
* one low-<math>\ell</math> temperature only likelihood (commander), <br />
* one low-<math>\ell</math> temperature and polarisation likelihood (lowlike), and <br />
* one higl-<math>\ell</math> likelihood CAMspec. <br />
<br />
The ''Commander'' likelihood covers the multipoles 2 to 49. It uses a semi-analytic method to sample the low-<math>\ell</math> temperature likelihood on an intermediate product of one of the component separated maps. The samples are used along with an analytical approximation of the likelihood posterior to perform the likelihood computation in the code. See {{PlanckPapers|planck2013-p08}} section 8.1 for more details.<br />
<br />
The ''lowlike'' likelihood covers the multipoles 2 to 32 for temperature and polarization data. Since Planck is not releasing polarisation data at this time, the polarization map from WMAP9 is used instead. A temperature map is needed to perform the computation nevertheless, and we use here the same commander map. The likelihood is computed using a map-based approximation at low resolution and a master one at intermediate resolution, as in WMAP. The likelihood code actually calls a very slightly modified version of the WMAP9 code. This piece of the likelihood essentially provides a prior on the optical depth and has almost no other impact on cosmological parameter estimation. As such it could be replaced by a simple prior, and a user can decide to do so, which is one of the motivation to leave the three pieces of the CMB likelihood as different data packages; see {{PlanckPapers|planck2013-p08}} section 8.3 for more details. Note that the version of the WMAP code used here (code version v1.0) does not perform any test on the positive definiteness of the TT, TE, EE covariance matrices, and will return a null log likelihood in the unphysical cases where the absolute value of TE is too large. This will be corrected in a later version.<br />
<br />
The ''CAMspec'' likelihood covers the multipoles 50 to 2500 for temperature only. The likelihood is computed using a quadratic approximation, including mode to mode correlations that have been precomputed on a fiducial model. The likelihood uses data from the 100, 143 and 217 GHz channels. To do so it models the foreground at each frequency using the model described in the likelihood paper. Uncertainties on the relative calibration and on the beam transfer functions are included either as parametric models, or marginalized and integrated in the covariance matrix. Detailed description of the different nuisance parameters is given below. Priors are included in the likelihood on the CIB spectral index, relative calibration factors and beam error eigenmodes. See {{PlanckPapers|planck2013-p08}} section 2.1 for more details.<br />
<br />
The ''act/spt'' likelihood covers the multipoles 1500 to 10000 for temperature. It is described in{{BibCite|dun2013}}{{BibCite|Keis2011}}{{BibCite|Reic2012}}. It uses the code and data that can be retrieved from the [http://lambda.gsfc.nasa.gov/ Lambda archive] for [http://lambda.gsfc.nasa.gov/product/act/act_prod_table.cfm ACT] and [http://lambda.gsfc.nasa.gov/product/spt/spt_prod_table.cfm SPT]. It has been slightly modified to use a thermal and kinetic SZ model that matches the one used in CAMspec. As stated in{{BibCite|dun2013}}, the dust parameters a_ge and a_gs must be explored with the following priors: a_ge = 0.8 ± 0.2 and a_gs = 0.4 ± 0.2. Those priors are not included in the log likelihood computed by the code.<br />
<br />
The ''lensing'' likelihood covers the multipoles 40 to 400 using the result of the [[Specially_processed_maps | lensing reconstruction]]. It uses a quadratic approximation for the likelihood, with a covariance matrix including the marginalized contribution of the beam transfer function uncertainties, the diffuse point source correction uncertainties and the cosmological model uncertainty affecting the first order non-gaussian bias (N1). The correlation between temperature and lensing is not taken into account. Cosmological uncertainty effects on the normalization are dealt with using a first order renormalization procedure. This means that the code will need both the TT and $\phi\phi$ power spectrum up to <math>\ell</math> = 2048 to correctly perform the integrals needed for the renormalization. Nevertheless, the code will only produce an estimate based on the data between <math>\ell</math> = 40 to 400. See {{PlanckPapers|planck2013-p12}} section 6.1 for more details.<br />
</span><br />
<span style="color:red">OUTSTANDING: description of likelihood masks </span><br />
==Production process==<br />
<br />
===Likelihood===<br />
<span style="color:red"> ALL OF THE FOLLOWING IN THE LIKELIHOOD SECTION IS OLD. </span><br />
The code is based on some basic routines from the libpmc library in the [http://arxiv.org/abs/1101.0950 cosmoPMC] code. It also uses some code from the [http://lambda.gsfc.nasa.gov/product/map/dr5/likelihood_get.cfm WMAP9 likelihood] for the lowlike likelihood and{{BibCite|dun2013}}{{BibCite|Keis2011}}{{BibCite|Reic2012}} for the act/spt one. The rest of the code has been specifically written for the Planck data. Each likelihood file has been processed using a different and dedicated pipeline as described in the likelihood paper {{PlanckPapers|planck2013-p08}} (section 2 and 8) and in the lensing paper {{PlanckPapers|planck2013-p12}} (section 6.1). We refer the reader to those papers for full details. The data are then encapsulated into the specific file format.<br />
<br />
Each dataset comes with its own self check. Whenever the code is used to read a data file, a computation will be done against an included test spectrum/nuisance parameter, and the log-likelihood will be displayed along with the expected result. Difference of the order of 10<math>^{-6}</math> or less are expected depending of the architecture.<br />
<br />
==Inputs==<br />
<br />
===Likelihood===<br />
<br />
; ''commander'' :<br />
* all Planck channels maps<br />
* compact source catalogs<br />
* common masks<br />
* beam transfer functions for all channels<br />
<br />
; ''lowlike'' :<br />
* WMAP9 likelihood data<br />
* Low-<math>\ell</math> Commander map<br />
<br />
; ''CAMspec'' :<br />
* 100, 143 and 217 GHz detector and detsets maps<br />
* 857GHz channel map<br />
* compact source catalog<br />
* common masks (0,1 & 3)<br />
* beam transfer function and error eigenmodes and covariance for 100, 143 and 217 GHz detectors & detsets<br />
* theoretical templates for the tSZ and kSZ contributions<br />
* color corrections for the CIB emission for the 143 and 217GHz detectors and detsets<br />
* fiducial CMB model (bootstrapped from WMAP7 best fit spectrum) estimated noise contribution from the half-ring maps for 100, 143 and 217 GHz<br />
<br />
; ''lensing'' :<br />
* the lensing map<br />
* beam error eigenmodes and covariance for the 143 and 217GHz channel maps<br />
* fiducial CMB model (from Planck cosmological parameter best fit)<br />
<br />
; ''act/spt'' :<br />
* data and code from [http://lambda.gsfc.nasa.gov/product/act/act_fulllikelihood_get.cfm here]<br />
* the tSZ andkSZ template are changed to match those of CAMspec<br />
<br />
== File names and Meta data ==<br />
<br />
===Likelihood===<br />
<span style="color:red"> ALL OF THE FOLLOWING IN THE LIKELIHOOD SECTION IS OLD. </span><br />
<br />
'''Likelihood source code'''<br />
<br />
The source code is in the file<br />
: {{PLASingleFile |fileType=cosmo|name=COM_Code_Likelihood-v1.0_R1.10.tar.gz|link=COM_Code_Likelihood-v1.0_R1.10.tar.gz}} (C, f90 and python likelihood library and tools)<br />
<br />
'''Likelihood data packages'''<br />
<br />
The {{PLALikelihood|type=Data|link=data packages}} are<br />
: ''{{PLASingleFile | fileType=cosmo | name=COM_Data_Likelihood-commander_R1.10.tar.gz | link=COM_Data_Likelihood-commander_R1.10.tar.gz}}'' (low-ell TT likelihood)<br />
: ''{{PLASingleFile | fileType=cosmo | name=COM_Data_Likelihood-lowlike_R1.10.tar.gz | link=COM_Data_Likelihood-lowlike_R1.10.tar.gz}}'' (low-ell TE,EE,BB likelihood)<br />
: ''{{PLASingleFile | fileType=cosmo | name=COM_Data_Likelihood-CAMspec_R1.10.tar.gz | link=COM_Data_Likelihood-CAMspec_R1.10.tar.gz}}'' (high-ell TT likelihood)<br />
: ''{{PLASingleFile | fileType=cosmo | name=COM_Data_Likelihood-actspt_R1.10.tar | link=COM_Data_Likelihood-actspt_R1.10.tar.gz}}'' (high-ell TT likelihood)<br />
: ''{{PLASingleFile | fileType=cosmo | name=COM_Data_Likelihood-lensing_R1.10.tar.gz | link=COM_Data_Likelihood-lensing_R1.10.tar.gz}}'' (lensing likelihood)<br />
<br />
Untar and unzip all files to recover the code and likelihood data. Each package comes with a README file; follow the instructions inclosed to<br />
build the code and use it. To compute the CMB likelihood one has to sum the log likelihood of each of the commander_v4.1_lm49.clik, lowlike_v222.clik and CAMspec_v6.2TN_2013_02_26.clik, actspt_2013_01.clik. To compute the CMB+lensing likelihood, one has to sum the log likelihood of all 5 files.<br />
<br />
The CMB and lensing likelihood format are different. The CMB files have the termination .clik, the lensing one .clik_lensing. The lensing data being simpler (due to the less detailled modeling permitted by the lower signal-noise), the file is a simple ascii file containing all the data along with comments describing it, and linking the different quantities to the lensing paper. The CMB file format is more complex and must accommodate different forms of data (maps, power spectrum, distribution samples, covariance matrices...). It consists of a tree structure containing the data. At each level of the tree structure a given directory can contain array data (in the form of FITS files or ascii files for strings) and scalar data (joined in a single ascii file "_mdb"). Those files are not user modifiable and do not contain interesting meta data for the user. Tools to manipulate those files are included in the code package as optional python tools. They are documented in the code package.<br />
<br />
'''Likelihood masks'''<br />
<br />
The masks used in the Likelihood paper {{PlanckPapers|planck2013-p08}} are found in<br />
{{PLASingleFile|fileType=map|name=COM_Mask_Likelihood_2048_R1.10.fits|link=COM_Mask_Likelihood_2048_R1.10.fits}}<br />
<br />
which contains ten masks which are written into a single ''BINTABLE'' extension of 10 columns by 50331648 rows (the number of Healpix pixels in an Nside = 2048 map). The structure is as follows, where the column names are the names of the masks: <br />
<br />
{| border="1" cellpadding="3" cellspacing="0" align="center" style="text-align:left" width=800px<br />
|+ '''Likelihodd masks file data structure'''<br />
|- bgcolor="ffdead" <br />
!colspan="4" | 1. EXTNAME = 'MSK-LIKE' : Data columns<br />
|- bgcolor="ffdead" <br />
! Column Name || Data Type || Units || Description<br />
|-<br />
|CL31 || Real*4 || none || mask<br />
|-<br />
|CL39 || Real*4 || none || mask<br />
|-<br />
|CL49 || Real*4 || none || mask<br />
|-<br />
|G22 || Real*4 || none || mask <br />
|-<br />
|G35 || Real*4 || none || mask<br />
|-<br />
|G45 || Real*4 || none || mask<br />
|-<br />
|G56 || Real*4 || none || mask<br />
|-<br />
|G65 || Real*4 || none || mask<br />
|-<br />
|PS96 || Real*4 || none || mask<br />
|-<br />
|PSA82 || Real*4 || none || mask<br />
|-<br />
|- bgcolor="ffdead" <br />
! Keyword || Data Type || Value || Description<br />
|-<br />
|PIXTYPE || string || HEALPIX ||<br />
|-<br />
|COORDSYS || string || GALACTIC ||Coordinate system <br />
|-<br />
|ORDERING || string || NESTED || Healpix ordering<br />
|-<br />
|NSIDE || Int || 2048 || Healpix Nside <br />
|-<br />
|FIRSTPIX || Int*4 || 0 || First pixel number<br />
|-<br />
|LASTPIX || Int*4 || 50331647 || Last pixel number, for LFI and HFI, respectively<br />
<br />
|}<br />
--><br />
<br />
== References ==<br />
<References /><br />
<br />
<br />
<br />
[[Category:Mission products|008]]</div>
Xdupac
https://wiki.cosmos.esa.int/planckpla2015/index.php?title=CMB_spectrum_%26_Likelihood_Code&diff=11457
CMB spectrum & Likelihood Code
2015-04-15T15:09:42Z
<p>Xdupac: </p>
<hr />
<div>{{DISPLAYTITLE:2015 CMB spectra and likelihood code}}<br />
<br />
==2015 CMB spectra==<br />
<br />
<br />
===General description===<br />
====TT====<br />
The Planck best-fit CMB temperature power spectrum, shown in the figure below, covers the wide range of multipoles <math> \ell </math> = 2-2508. Over the multipole range <math> \ell </math> = 2–29, the power spectrum is derived from the ''Commander'': component separation algorithm applied to the combination of Planck 2015 temperature data between 30 and 857 GHz, the 9-year WMAP sky maps, and the 408 MHz Haslam et al. (1982) survey, including 93% of the sky {{PlanckPapers|planck2014-a12}} . The asymmetric error bars associated to this spectrum are the 68% confidence limits and include the uncertainties due to foreground subtraction.<br />
<br />
For multipoles equal or greater than <math>\ell=30</math>, instead, the spectrum is derived from the ''Plik'' likelihood {{PlanckPapers|planck2014-a13}} by optimally combining the spectra in the frequency range 100-217 GHz, and correcting them for unresolved foregrounds using the best-fit foreground solution from a Planck TT+lowP <math>\Lambda</math>CDM run. Associated 1-sigma errors include beam uncertainties. Both ''Commander'' and ''Plik'' are described in more details in the sections below.<br />
<br />
[[File: A15_TT.png|thumb|center|700px|'''The Planck 2015 TT power spectrum. Logarithmic x-scale up to <math>\ell = 30 </math> , linear at higher <math>\ell</math>. The red line is the Planck best-fit primordial power spectrum (cf Planck TT+lowP in Table 3 of Planck-2015-A15[3]). Residuals with respect to this model are shown in the lower panel. The error bars show <math>\pm 1\sigma</math> uncertainties.''']]<br />
<br />
====TE and EE====<br />
The Planck best-fit CMB polarization and temperature-polarization cross-correlation power spectra, shown in the figure below, cover the multipole range <math> \ell </math> = 30-1996. The data points relative to the multipole range <math> \ell </math> = 2-29 will be released at a later time.<br />
Analogously to the TT case, the <math> \ell\ge 30 </math> spectrum is derived from the ''Plik'' likelihood {{PlanckPapers|planck2014-a13}} by optimally combining the spectra in the frequency range 100-217 GHz, and correcting them for unresolved foregrounds using the best-fit foreground solution from a Planck TT,TE,EE+lowP <math>\Lambda</math>CDM run. <br />
<br />
{|style="margin: 0 auto;"<br />
|[[File: A15_EE.png|thumb|center|500px|'''The Planck 2015 EE power spectrum. The red line is the Planck best-fit primordial power spectrum (cf Planck TT+lowP in Table 3 of Planck-2015-A15). Residuals with respect to this model are shown in the lower panel. The error bars show <math>\pm 1\sigma</math> uncertainties. The green lines in the lower panels show the best-fit temperature-to-polarization leakage model of Eqs. (11a) and (11b) in Planck-2015-A15.''']]<br />
|[[File: A15_TE.png|thumb|center|500px|'''The Planck 2015 TE power spectrum. The red line is the Planck best-fit primordial power spectrum (cf Planck TT+lowP in Table 3 of Planck-2015-A15). Residuals with respect to this model are shown in the lower panel. The error bars show <math>\pm 1\sigma</math> uncertainties. The green lines in the lower panels show the best-fit temperature-to-polarization leakage model of Eqs. (11a) and (11b) in Planck-2015-A15.''']]<br />
|}<br />
<br />
===Production process===<br />
The <math>\ell</math> < 30 part of the Planck TT power spectrum is derived from the Commander approach, which implements Bayesian component separation in pixel space, fitting a parametric model to the data by sampling the posterior distribution for the model parameters {{PlanckPapers|planck2014-a12}}. The power spectrum at any multipole <math>\ell</math> is given as the maximum probability point for the posterior <math>C_\ell</math> distribution, marginalized over the other multipoles, and the error bars are 68% confidence level; see {{PlanckPapers|planck2014-a12}}. <br />
<br />
The <math>\ell \ge 30</math> part of the TT, TE and EE power spectra have been derived by the Plik likelihood, a code that implements a pseudo-Cl based technique, extensively described in Sec. 2 and the Appendix of {{PlanckPapers|planck2013-p08}} and {{PlanckPapers|planck2014-a13}}. Frequency spectra are computed as cross-spectra between half-mission maps. Mask and multipole range choices for each frequency spectrum are summarized in Section 3.3 of {{PlanckPapers|planck2014-a15}} and in {{PlanckPapers|planck2014-a13}}. The final power spectrum is an optimal combination of the 100, 143, 143x217 and 217 GHz spectra, corrected for the best-fit unresolved foregrounds and inter-frequency calibration factors, as derived from the full likelihood analysis (for TT we use the best-fit solutions for the nuisance parameters from the Planck+TT+lowP data combination, while for TE and EE we use the best fit from Planck+TT+lowP, cf Table 3 of {{PlanckPapers|planck2014-a15}}). A thorough description of the models of unresolved foregrounds is given in {{PlanckPapers|planck2014-a13}}. The spectrum covariance matrix accounts for cosmic variance and noise contributions, together with beam uncertainties. The <math>\ell \ge 30</math> CMB TT spectrum and associated covariance matrix are available in two formats:<br />
#Unbinned. TT: 2479 bandpowers (<math>\ell=30-2508</math>); TE or EE: 1697 bandpowers (<math>\ell=30-1996</math>).<br />
#Binned, in bins of <math> \Delta\ell=30 </math>. TT: 83 bandpowers. TE or EE: 66 bandpowers. We bin the <math> C_\ell </math> power spectrum with a weight proportional to <math> \ell (\ell+1) </math>, so that the <math> C_{\ell_b} </math> binned bandpower centered in <math> \ell_b </math> is: <math> \\ C_{\ell_b}=\Sigma_{\ell \in b} w_{\ell_b\ell} C_\ell \quad \text{with} \quad w_{\ell_b\ell}=\frac{\ell (\ell+1)}{\Sigma_{\ell \in b} \ell (\ell+1)}. \\</math> Equivalently, using the matrix formalism, we can construct the binning matrix B as: <math>\\ B_{\ell_b \ell}=w_{\ell_b\ell} \\ </math> where B is a <math> n_b\times n_\ell</math> matrix, with <math>n_b=83</math> the number of bins and <math>n_\ell=2479</math> the number of unbinned multipoles. Thus: <math> \\ \vec{C}_\mathrm{binned}=B \, \vec{C} \\ \mathrm{cov_\mathrm{binned}}= B\, \mathrm{cov}\, B^T \\ \ell_b=B\, \ell \\ </math> Here, <math> \vec{C}_{binned}\, (\vec{C}) </math> is the vector containing all the binned (unbinned) <math>C_\ell</math> bandpowers, <math>\mathrm{cov} </math> is the covariance matrix and <math>\ell_b</math> is the weighted average multipole in each bin. Note that following this definition, <math>\ell_b</math> can be a non-integer. The binned <math>D_{\ell_B}</math> power spectrum is then calculated as: <math> \\ D_{\ell_b}=\frac{\ell_b (\ell_b+1)}{2\pi} C_{\ell_b} </math>.<br />
<br />
===Inputs===<br />
<br />
; Low-l spectrum (<math>\ell < 30</math>):<br />
* Planck 30 and 44 GHz frequency maps<br />
* Planck 70 to 857 GHz detector and detector set maps<br />
* 9-year WMAP temperature sky maps between 23 and 94 GHz<br />
* 408 MHz survey by Haslam et al. (1982) <br />
* Commander <math>\chi^2</math> based LM93 confidence mask {{PlanckPapers|planck2014-a12}}<br />
<br />
; High-l spectrum (<math>30 \le \ell \le 2508</math>): <br />
<br />
* 100, 143, 143x217 and 217 GHz spectra and their covariance matrix (Sec. 3.3 {{PlanckPapers|planck2014-a15}})<br />
* best-fit foreground templates and inter-frequency calibration factors (Table 3 of {{PlanckPapers|planck2014-a15}})<br />
* Beam transfer function uncertainties {{PlanckPapers|planck2014-a08}}<br />
=== File names and Meta data ===<br />
<br />
The CMB spectrum and its covariance matrix are distributed in a single FITS file named <br />
<!--- * ''{{PLASingleFile | fileType=cosmo | name=COM_PowerSpect_CMB_R2.00.fits | link=COM_PowerSpect_CMB_R1.10.fits}}'' ---><br />
* ''COM_PowerSpect_CMB_R2.nn.fits''<br />
which contains 7 ''BINTABLE'' extensions<br />
<br />
; 1. TT low-ell, unbinned (TTLOLUNB)<br />
: with the low ell part of the spectrum, not binned, and for l=2-29. The table columns are<br />
# ''ELL'' (integer): multipole number<br />
# ''D_ELL'' (float): <math>D_ell</math> as described above<br />
# ''ERRUP'' (float): the upward uncertainty<br />
# ''ERRDOWN'' (float): the downward uncertainty<br />
<br />
; 2. TT high-ell, binned (TTHILBIN)<br />
: with the high-ell part of the spectrum, binned into 83 bins covering <math>\langle l \rangle = 47-2499\ </math> in bins of width <math>l=30</math> (with the exception of the last bin that is smaller). The table columns are as follows:<br />
# ''ELL'' (float): mean multipole number of bin<br />
# ''L_MIN'' (integer): lowest multipole of bin<br />
# ''L_MAX'' (integer): highest multipole of bin<br />
# ''D_ELL'' (float): <math>D_\ell</math> as described above<br />
# ''ERR'' (float): the uncertainty<br />
<br />
; 3. TT high-ell unbinned (TTHILUNB) <br />
: with the high-ell part of the spectrum, unbinned, in 2979 bins covering <math>\langle l \rangle = 30-2508\ </math>. The table columns are as follows:<br />
# ''ELL'' (integer): multipole <br />
# ''D_ELL'' (float): <math>D_\ell</math> as described above<br />
# ''ERR'' (float): the uncertainty<br />
<br />
; 4. TE high-ell, binned (TEHILBIN) <br />
: with the high-ell part of the spectrum, binned into 83 bins covering <math>\langle l \rangle = 47-1988\ </math> in bins of width <math>l=30</math> (with the exception of the last bin that is smaller). The table columns are as follows:<br />
# ''ELL'' (float): mean multipole number of bin<br />
# ''L_MIN'' (integer): lowest multipole of bin<br />
# ''L_MAX'' (integer): highest multipole of bin<br />
# ''D_ELL'' (float): <math>D_\ell</math> as described above<br />
# ''ERR'' (float): the uncertainty<br />
<br />
; 5. TE high-ell, unbinned (TEHILUNB) <br />
: with the high-ell part of the spectrum, unbinned, in 2979 bins covering <math>\langle l \rangle = 30-1996\ </math>. The table columns are as follows:<br />
# ''ELL'' (integer): multipole <br />
# ''D_ELL'' (float): <math>D_\ell</math> as described above<br />
# ''ERR'' (float): the uncertainty<br />
<br />
; 6. EE high-ell, binned (EEHILBIN) <br />
: with the high-ell part of the spectrum, binned into 83 bins covering <math>\langle l \rangle = 47-1988\ </math> in bins of width <math>l=30</math> (with the exception of the last bin that is smaller). The table columns are as follows:<br />
# ''ELL'' (float): mean multipole number of bin<br />
# ''L_MIN'' (integer): lowest multipole of bin<br />
# ''L_MAX'' (integer): highest multipole of bin<br />
# ''D_ELL'' (float): <math>D_\ell</math> as described above<br />
# ''ERR'' (float): the uncertainty<br />
<br />
; 7. EE high-ell, unbinned (EEHILUNB) <br />
: with the high-ell part of the spectrum, unbinned, in 2979 bins covering <math>\langle l \rangle = 30-1996\ </math>. The table columns are as follows:<br />
# ''ELL'' (integer): multipole <br />
# ''D_ELL'' (float): <math>D_\ell</math> as described above<br />
# ''ERR'' (float): the uncertainty<br />
<br />
Note that R2.00 of these files contained a small error in that the ''effective'' <math>\ell</math> of the bin in the binned data was truncated to an integer. While the <math>\ell</math> values of the unbinned (full) data are indeed integer, the ''effective'' <math>\ell</math> of the binned data is a weighted average of the <math>\ell</math>'s used in the bin and it should be a real number. This is corrected in R2.01.<br />
<br />
The spectra give <math>D_\ell = \ell(\ell+1)C_\ell / 2\pi </math> in units of <math>\mu\, K^2</math>. The covariance matrices of the spectra will be released at a later time.<br />
<!-- <br />
<br />
The CMB spectrum is also given in a simple text comma-separated file:<br />
* ''{{PLASingleFile | fileType=cosmo | name=COM_PowerSpect_CMB_R1.10.txt |link=COM_PowerSpect_CMB_R1.10.txt}}''<br />
<br />
--><br />
<br />
==Likelihood==<br />
The likelihood code will released in March-April 2015 with an accompanying paper and an Explanatory Supplement update. <br />
<!-- <br />
===Likelihood===<br />
<span style="color:red"> ALL OF THE FOLLOWING IN THE LIKELIHOOD SECTION IS OLD. </span><br />
The likelihood code (and the data that comes with it) used to compute the likelihood of a model that predicts the CMB power spectra, lensing power spectrum, together with some foreground and some instrumental parameters. The data files are built primarily from the Planck mission results, but include also some results from the WMAP-9 data release. The data files are written in a specific format that can only be read by the code. The code consists in a c/f90 library, along with some optional tools in python. The code is used to read the data files, and given model power spectra and nuisance parameters it computes the log likelihood of that model. <br />
<br />
Detailed description of the installation and usage of the likelihood code and data is provided in the package. The package includes five data files: four for the CMB likelihoods and one for the lensing likelihood. All of the likelihoods delivered are described in detail in the {{PlanckPapers|planck2013-p08|1|Power spectrum & Likelihood Paper}} (for the CMB based likelihood) and in the {{PlanckPapers|planck2013-p12|1|Lensing Paper}} (for the lensing likelihood) .<br />
<br />
The CMB full likelihood has been divided into four parts to allow using selectively different ranges of multipoles. It also reflects the fact that the mathematical approximations used for those different parts are very different, as is the underlying data. In detail, we distribute<br />
* one low-<math>\ell</math> temperature only likelihood (commander), <br />
* one low-<math>\ell</math> temperature and polarisation likelihood (lowlike), and <br />
* one higl-<math>\ell</math> likelihood CAMspec. <br />
<br />
The ''Commander'' likelihood covers the multipoles 2 to 49. It uses a semi-analytic method to sample the low-<math>\ell</math> temperature likelihood on an intermediate product of one of the component separated maps. The samples are used along with an analytical approximation of the likelihood posterior to perform the likelihood computation in the code. See {{PlanckPapers|planck2013-p08}} section 8.1 for more details.<br />
<br />
The ''lowlike'' likelihood covers the multipoles 2 to 32 for temperature and polarization data. Since Planck is not releasing polarisation data at this time, the polarization map from WMAP9 is used instead. A temperature map is needed to perform the computation nevertheless, and we use here the same commander map. The likelihood is computed using a map-based approximation at low resolution and a master one at intermediate resolution, as in WMAP. The likelihood code actually calls a very slightly modified version of the WMAP9 code. This piece of the likelihood essentially provides a prior on the optical depth and has almost no other impact on cosmological parameter estimation. As such it could be replaced by a simple prior, and a user can decide to do so, which is one of the motivation to leave the three pieces of the CMB likelihood as different data packages; see {{PlanckPapers|planck2013-p08}} section 8.3 for more details. Note that the version of the WMAP code used here (code version v1.0) does not perform any test on the positive definiteness of the TT, TE, EE covariance matrices, and will return a null log likelihood in the unphysical cases where the absolute value of TE is too large. This will be corrected in a later version.<br />
<br />
The ''CAMspec'' likelihood covers the multipoles 50 to 2500 for temperature only. The likelihood is computed using a quadratic approximation, including mode to mode correlations that have been precomputed on a fiducial model. The likelihood uses data from the 100, 143 and 217 GHz channels. To do so it models the foreground at each frequency using the model described in the likelihood paper. Uncertainties on the relative calibration and on the beam transfer functions are included either as parametric models, or marginalized and integrated in the covariance matrix. Detailed description of the different nuisance parameters is given below. Priors are included in the likelihood on the CIB spectral index, relative calibration factors and beam error eigenmodes. See {{PlanckPapers|planck2013-p08}} section 2.1 for more details.<br />
<br />
The ''act/spt'' likelihood covers the multipoles 1500 to 10000 for temperature. It is described in{{BibCite|dun2013}}{{BibCite|Keis2011}}{{BibCite|Reic2012}}. It uses the code and data that can be retrieved from the [http://lambda.gsfc.nasa.gov/ Lambda archive] for [http://lambda.gsfc.nasa.gov/product/act/act_prod_table.cfm ACT] and [http://lambda.gsfc.nasa.gov/product/spt/spt_prod_table.cfm SPT]. It has been slightly modified to use a thermal and kinetic SZ model that matches the one used in CAMspec. As stated in{{BibCite|dun2013}}, the dust parameters a_ge and a_gs must be explored with the following priors: a_ge = 0.8 ± 0.2 and a_gs = 0.4 ± 0.2. Those priors are not included in the log likelihood computed by the code.<br />
<br />
The ''lensing'' likelihood covers the multipoles 40 to 400 using the result of the [[Specially_processed_maps | lensing reconstruction]]. It uses a quadratic approximation for the likelihood, with a covariance matrix including the marginalized contribution of the beam transfer function uncertainties, the diffuse point source correction uncertainties and the cosmological model uncertainty affecting the first order non-gaussian bias (N1). The correlation between temperature and lensing is not taken into account. Cosmological uncertainty effects on the normalization are dealt with using a first order renormalization procedure. This means that the code will need both the TT and $\phi\phi$ power spectrum up to <math>\ell</math> = 2048 to correctly perform the integrals needed for the renormalization. Nevertheless, the code will only produce an estimate based on the data between <math>\ell</math> = 40 to 400. See {{PlanckPapers|planck2013-p12}} section 6.1 for more details.<br />
</span><br />
<span style="color:red">OUTSTANDING: description of likelihood masks </span><br />
==Production process==<br />
<br />
===Likelihood===<br />
<span style="color:red"> ALL OF THE FOLLOWING IN THE LIKELIHOOD SECTION IS OLD. </span><br />
The code is based on some basic routines from the libpmc library in the [http://arxiv.org/abs/1101.0950 cosmoPMC] code. It also uses some code from the [http://lambda.gsfc.nasa.gov/product/map/dr5/likelihood_get.cfm WMAP9 likelihood] for the lowlike likelihood and{{BibCite|dun2013}}{{BibCite|Keis2011}}{{BibCite|Reic2012}} for the act/spt one. The rest of the code has been specifically written for the Planck data. Each likelihood file has been processed using a different and dedicated pipeline as described in the likelihood paper {{PlanckPapers|planck2013-p08}} (section 2 and 8) and in the lensing paper {{PlanckPapers|planck2013-p12}} (section 6.1). We refer the reader to those papers for full details. The data are then encapsulated into the specific file format.<br />
<br />
Each dataset comes with its own self check. Whenever the code is used to read a data file, a computation will be done against an included test spectrum/nuisance parameter, and the log-likelihood will be displayed along with the expected result. Difference of the order of 10<math>^{-6}</math> or less are expected depending of the architecture.<br />
<br />
==Inputs==<br />
<br />
===Likelihood===<br />
<br />
; ''commander'' :<br />
* all Planck channels maps<br />
* compact source catalogs<br />
* common masks<br />
* beam transfer functions for all channels<br />
<br />
; ''lowlike'' :<br />
* WMAP9 likelihood data<br />
* Low-<math>\ell</math> Commander map<br />
<br />
; ''CAMspec'' :<br />
* 100, 143 and 217 GHz detector and detsets maps<br />
* 857GHz channel map<br />
* compact source catalog<br />
* common masks (0,1 & 3)<br />
* beam transfer function and error eigenmodes and covariance for 100, 143 and 217 GHz detectors & detsets<br />
* theoretical templates for the tSZ and kSZ contributions<br />
* color corrections for the CIB emission for the 143 and 217GHz detectors and detsets<br />
* fiducial CMB model (bootstrapped from WMAP7 best fit spectrum) estimated noise contribution from the half-ring maps for 100, 143 and 217 GHz<br />
<br />
; ''lensing'' :<br />
* the lensing map<br />
* beam error eigenmodes and covariance for the 143 and 217GHz channel maps<br />
* fiducial CMB model (from Planck cosmological parameter best fit)<br />
<br />
; ''act/spt'' :<br />
* data and code from [http://lambda.gsfc.nasa.gov/product/act/act_fulllikelihood_get.cfm here]<br />
* the tSZ andkSZ template are changed to match those of CAMspec<br />
<br />
== File names and Meta data ==<br />
<br />
===Likelihood===<br />
<span style="color:red"> ALL OF THE FOLLOWING IN THE LIKELIHOOD SECTION IS OLD. </span><br />
<br />
'''Likelihood source code'''<br />
<br />
The source code is in the file<br />
: {{PLASingleFile |fileType=cosmo|name=COM_Code_Likelihood-v1.0_R1.10.tar.gz|link=COM_Code_Likelihood-v1.0_R1.10.tar.gz}} (C, f90 and python likelihood library and tools)<br />
<br />
'''Likelihood data packages'''<br />
<br />
The {{PLALikelihood|type=Data|link=data packages}} are<br />
: ''{{PLASingleFile | fileType=cosmo | name=COM_Data_Likelihood-commander_R1.10.tar.gz | link=COM_Data_Likelihood-commander_R1.10.tar.gz}}'' (low-ell TT likelihood)<br />
: ''{{PLASingleFile | fileType=cosmo | name=COM_Data_Likelihood-lowlike_R1.10.tar.gz | link=COM_Data_Likelihood-lowlike_R1.10.tar.gz}}'' (low-ell TE,EE,BB likelihood)<br />
: ''{{PLASingleFile | fileType=cosmo | name=COM_Data_Likelihood-CAMspec_R1.10.tar.gz | link=COM_Data_Likelihood-CAMspec_R1.10.tar.gz}}'' (high-ell TT likelihood)<br />
: ''{{PLASingleFile | fileType=cosmo | name=COM_Data_Likelihood-actspt_R1.10.tar | link=COM_Data_Likelihood-actspt_R1.10.tar.gz}}'' (high-ell TT likelihood)<br />
: ''{{PLASingleFile | fileType=cosmo | name=COM_Data_Likelihood-lensing_R1.10.tar.gz | link=COM_Data_Likelihood-lensing_R1.10.tar.gz}}'' (lensing likelihood)<br />
<br />
Untar and unzip all files to recover the code and likelihood data. Each package comes with a README file; follow the instructions inclosed to<br />
build the code and use it. To compute the CMB likelihood one has to sum the log likelihood of each of the commander_v4.1_lm49.clik, lowlike_v222.clik and CAMspec_v6.2TN_2013_02_26.clik, actspt_2013_01.clik. To compute the CMB+lensing likelihood, one has to sum the log likelihood of all 5 files.<br />
<br />
The CMB and lensing likelihood format are different. The CMB files have the termination .clik, the lensing one .clik_lensing. The lensing data being simpler (due to the less detailled modeling permitted by the lower signal-noise), the file is a simple ascii file containing all the data along with comments describing it, and linking the different quantities to the lensing paper. The CMB file format is more complex and must accommodate different forms of data (maps, power spectrum, distribution samples, covariance matrices...). It consists of a tree structure containing the data. At each level of the tree structure a given directory can contain array data (in the form of FITS files or ascii files for strings) and scalar data (joined in a single ascii file "_mdb"). Those files are not user modifiable and do not contain interesting meta data for the user. Tools to manipulate those files are included in the code package as optional python tools. They are documented in the code package.<br />
<br />
'''Likelihood masks'''<br />
<br />
The masks used in the Likelihood paper {{PlanckPapers|planck2013-p08}} are found in<br />
{{PLASingleFile|fileType=map|name=COM_Mask_Likelihood_2048_R1.10.fits|link=COM_Mask_Likelihood_2048_R1.10.fits}}<br />
<br />
which contains ten masks which are written into a single ''BINTABLE'' extension of 10 columns by 50331648 rows (the number of Healpix pixels in an Nside = 2048 map). The structure is as follows, where the column names are the names of the masks: <br />
<br />
{| border="1" cellpadding="3" cellspacing="0" align="center" style="text-align:left" width=800px<br />
|+ '''Likelihodd masks file data structure'''<br />
|- bgcolor="ffdead" <br />
!colspan="4" | 1. EXTNAME = 'MSK-LIKE' : Data columns<br />
|- bgcolor="ffdead" <br />
! Column Name || Data Type || Units || Description<br />
|-<br />
|CL31 || Real*4 || none || mask<br />
|-<br />
|CL39 || Real*4 || none || mask<br />
|-<br />
|CL49 || Real*4 || none || mask<br />
|-<br />
|G22 || Real*4 || none || mask <br />
|-<br />
|G35 || Real*4 || none || mask<br />
|-<br />
|G45 || Real*4 || none || mask<br />
|-<br />
|G56 || Real*4 || none || mask<br />
|-<br />
|G65 || Real*4 || none || mask<br />
|-<br />
|PS96 || Real*4 || none || mask<br />
|-<br />
|PSA82 || Real*4 || none || mask<br />
|-<br />
|- bgcolor="ffdead" <br />
! Keyword || Data Type || Value || Description<br />
|-<br />
|PIXTYPE || string || HEALPIX ||<br />
|-<br />
|COORDSYS || string || GALACTIC ||Coordinate system <br />
|-<br />
|ORDERING || string || NESTED || Healpix ordering<br />
|-<br />
|NSIDE || Int || 2048 || Healpix Nside <br />
|-<br />
|FIRSTPIX || Int*4 || 0 || First pixel number<br />
|-<br />
|LASTPIX || Int*4 || 50331647 || Last pixel number, for LFI and HFI, respectively<br />
<br />
|}<br />
--><br />
<br />
== References ==<br />
<References /><br />
<br />
<br />
<br />
[[Category:Mission products|008]]</div>
Xdupac
https://wiki.cosmos.esa.int/planckpla2015/index.php?title=Scanning_Beams&diff=11456
Scanning Beams
2015-04-15T14:33:04Z
<p>Xdupac: </p>
<hr />
<div>{{DISPLAYTITLE:2015 Scanning Beams}}<br />
<br />
== LFI beams ==<br />
<br />
We released maps of the Stokes parameters of the band-averaged [[Beams LFI#Polarized_Scanning_Beams_and_Focal_Plane_calibration|scanning beams]]. The averages are performed using the [[The_RIMO#LFI_2|RIMO]] bandpass, assuming a flat spectrum of the incoming radiation. The Stokes parameters maps contain the complete information about the field intensity and polarization properties. Main Beam, Intermediate Beam, and Sidelobes are released separately.<br />
<br />
More information on LFI beams can be found at {{PlanckPapers|planck2014-a05}} and on HFI beams at {{PlanckPapers|planck2014-a08}}<br />
<br />
===File Names===<br />
<br />
The file names are of the form:<br />
<br />
''LFI_ScanBeam-{mb,ib,sl}_{fff}-{rrr}_R2.{nn}.stokes''<br />
<br />
where<br />
* ''fff'' denotes the frequency<br />
* ''mb'' denotes the Main Beams<br />
* ''ib'' denotes the Intermediate Beam <br />
* ''sl'' denotes the Sidelobes<br />
* ''rrr'' denotes the radiometer<br />
* ''R2.nn'' is the version.<br />
<br />
<br />
At the present time, HFI is not releasing the Scanning Beams.<br />
<br />
===FITS file structure===<br />
The FITS files contain a primary extension with no data and a minimal header, and one BINTABLE extension with data and with a description of the data in the header keywords. <br />
The BINTABLE extension consist in four columns, each containing the array of one Stokes parameter. <br />
The columns are called:<br />
* ''Beamdata'' , containing <math>I</math><br />
* ''BeamdataQ'', containing <math>Q</math><br />
* ''BeamdataU'', containing <math>U</math><br />
* ''BeamdataV'', containing <math>V</math>.<br />
<br />
Main Beam, Intermediate Beams and Sidelobes are saved with a different data format: <br />
<br />
* Main Beams are projected on the tangent plane to the sphere, and sampled on a grid. The grid include an angular region expressed by the keyword ''angularCut'', and its dimensions are given by the keywords ''Nx'' and ''Ny'', representing the number of columns and rows. Each column of the BINDATA extension contains the sequence of the <math>Nx \times Ny</math> samples of the map in row major order. The keywords ''Xcentre'' and ''Ycentre'' express the coordinates of the beam maximum (i.e. where the sphere intersect the tangent plane).<br />
<br />
{| border="1" cellpadding="3" cellspacing="0" align="center" style="text-align:left" width=800px<br />
|+ '''Main Beam file structure''' <br />
<br />
|- bgcolor="ffdead" <br />
! Column Name || Data Type || Units || Description || Comment<br />
|-<br />
|BEAMDATA || Real*4 || none || Stokes parameter I || <br />
|-<br />
|BEAMDATAQ || Real*4 || none || Stokes parameter Q ||<br />
|-<br />
|BEAMDATAU || Real*4 || none || Stokes parameter U ||<br />
|-<br />
|BEAMDATAV || Real*4 || none || Stokes parameter V ||<br />
<br />
|- bgcolor="ffdead" <br />
<br />
! Keyword || Data Type || Value || Description || Comment<br />
|-<br />
|Nx || Int || 601 || X axis samples number || X axis aligned with the direction of the S arm<br />
|-<br />
|Ny || Int || 601 || Y axis samples number || Y axis aligned with the direction of the M arm<br />
|-<br />
|Xcentre || Int || 301 || X coordinate of the beam centre ||<br />
|-<br />
|Ycentre || Int || 301 || Y coordinate of the beam centre || <br />
|-<br />
|Xdelta || Float || || X step in radians || <br />
|-<br />
|Ydelta || Float || || Y step in radians || <br />
|}<br />
<br />
<br />
<br />
<br />
* Intermediate Beams and Sidelobes are sampled on the sphere. The resolution in <math>\theta</math> and <math>\phi</math> is given by the keywords "Ntheta" and "Nphi". The columns of the BINDATA extension contain the sequence of Nphi Stokes parameters for each <math>\theta</math>.<br />
<br />
{| border="1" cellpadding="3" cellspacing="0" align="center" style="text-align:left" width=800px<br />
|+ '''Intermediate Beam and Sidelobes file structure''' <br />
<br />
|- bgcolor="ffdead"<br />
! Column Name || Data Type || Units || Description ||Comment<br />
|-<br />
|BEAMDATA || Real*4 || none || Stokes parameter I || <br />
|-<br />
|BEAMDATAQ || Real*4 || none || Stokes parameter Q ||<br />
|-<br />
|BEAMDATAU || Real*4 || none || Stokes parameter U ||<br />
|-<br />
|BEAMDATAV || Real*4 || none || Stokes parameter V ||<br />
<br />
|- bgcolor="ffdead" <br />
<br />
! Keyword || Data Type || Value || Description || Comment<br />
|-<br />
|Ntheta || Int || || <math>\theta</math> samples number || colatitude<br />
|-<br />
|Nphi || Int || || <math>\phi</math> samples number || longitude<br />
|-<br />
|Mintheta || Float || || Minimum value of <math>\theta</math> ||<br />
|-<br />
|Maxtheta || Float || || Maximum value of <math>\theta</math> ||<br />
|-<br />
|angularCut || Float || || Angular cut [deg] ||<br />
<br />
|}<br />
<br />
== HFI Beams ==<br />
<br />
The HFI scanning beams are a combination of observations of Saturn, for the central parts, and Jupiter, for the wings, as described in the [[Beams | Beams]] section of this document, and in Section 4.1 of {{PlanckPapers | planck2014-a08}} on ''Hybrid beams''. Saturn data are used where they are signal-dominated; when the SNR of Saturn drops to < 9, Jupiter data are used, after binning them azimuthally. Beyond that, i.e., below the noise floor of the Jupiter data, and out to 100 arcmin, a power law (~θ<sup> -3</sup>) is used, where the exponent is derived from GRASP physical optics models. The figure below, taken from the [[Beams#Key_Changes | Beams]] section of this document, shows graphically the different portions of the beam model.<br />
<br />
<br />
[[Image:HybridBeamDiagram.png|thumb|500px|center| Scanning beam map for detector 143-6 showing a rough diagram of the regions that are handled with a different<br />
data selection or binning.]]<br />
<br />
<br />
The beams are provided in FITS files named <br />
* ''HFI_ScanBeam_{det-name}_R2.nn.fits'', <br />
where ''det-name'' is of the form ''100-1a'', and ''nn'' is the version number. Each file contains a single ''IMAGE'' extension. The image is 6001x6001 pixels of size 2x2 arcsec<sup>2</sup> (given in the ''DELTAX'' and ''DELTAY'' keywords), centred on pixel 3001,3001, and normalised to 1 at the maximum, where ''X'' and ''Y'' and in the Dxx reference system.<br />
<br />
== References ==<br />
<References /></div>
Xdupac
https://wiki.cosmos.esa.int/planckpla2015/index.php?title=Scanning_Beams&diff=11455
Scanning Beams
2015-04-15T14:30:52Z
<p>Xdupac: </p>
<hr />
<div>{{DISPLAYTITLE:2015 Scanning Beams}}<br />
<br />
== LFI beams ==<br />
<br />
We released maps of the Stokes parameters of the band-averaged [[Beams LFI#Polarized_Scanning_Beams_and_Focal_Plane_calibration|scanning beams]]. The averages are performed using the [[The_RIMO#LFI_2|RIMO]] bandpass, assuming a flat spectrum of the incoming radiation. The Stokes parameters maps contain the complete information about the field intensity and polarization properties. Main Beam, Intermediate Beam, and Sidelobes are released separately.<br />
<br />
More information on LFI beams can be found at {{PlanckPapers|planck2014-a05}} and on HFI beams at {{PlanckPapers|planck2014-a08}}<br />
<br />
===File Names===<br />
<br />
The file names are of the form:<br />
<br />
''LFI_ScanBeam-{mb,ib,sl}_{fff}-{rrr}_R2.{nn}.stokes''<br />
<br />
where<br />
* ''fff'' denotes the frequency<br />
* ''mb'' denotes the Main Beams<br />
* ''ib'' denotes the Intermediate Beam <br />
* ''sl'' denotes the Sidelobes<br />
* ''rrr'' denotes the radiometer<br />
* ''R2.nn'' is the version.<br />
<br />
<br />
At the present time, HFI is not releasing the Scanning Beams.<br />
<br />
===FITS file structure===<br />
The FITS files contain a primary extension with no data and a minimal header, and one BINTABLE extension with data and with a description of the data in the header keywords. <br />
The BINTABLE extension consist in four columns, each containing the array of one Stokes parameter. <br />
The columns are called:<br />
* ''Beamdata'' , containing <math>I</math><br />
* ''BeamdataQ'', containing <math>Q</math><br />
* ''BeamdataU'', containing <math>U</math><br />
* ''BeamdataV'', containing <math>V</math>.<br />
<br />
Main Beam, Intermediate Beams and Sidelobes are saved with a different data format: <br />
<br />
* Main Beams are projected on the tangent plane to the sphere, and sampled on a grid. The grid include an angular region expressed by the keyword ''angularCut'', and its dimensions are given by the keywords ''Nx'' and ''Ny'', representing the number of columns and rows. Each column of the BINDATA extension contains the sequence of the <math>Nx \times Ny</math> samples of the map in row major order. The keywords ''Xcentre'' and ''Ycentre'' express the coordinates of the beam maximum (i.e. where the sphere intersect the tangent plane).<br />
<br />
{| border="1" cellpadding="3" cellspacing="0" align="center" style="text-align:left" width=800px<br />
|+ '''Main Beam file structure''' <br />
<br />
|- bgcolor="ffdead" <br />
! Column Name || Data Type || Units || Description || Comment<br />
|-<br />
|BEAMDATA || Real*4 || none || Stokes parameter I || <br />
|-<br />
|BEAMDATAQ || Real*4 || none || Stokes parameter Q ||<br />
|-<br />
|BEAMDATAU || Real*4 || none || Stokes parameter U ||<br />
|-<br />
|BEAMDATAV || Real*4 || none || Stokes parameter V ||<br />
<br />
|- bgcolor="ffdead" <br />
<br />
! Keyword || Data Type || Value || Description || Comment<br />
|-<br />
|Nx || Int || 601 || X axis samples number || X axis aligned with the direction of the S arm<br />
|-<br />
|Ny || Int || 601 || Y axis samples number || Y axis aligned with the direction of the M arm<br />
|-<br />
|Xcentre || Int || 301 || X coordinate of the beam centre ||<br />
|-<br />
|Ycentre || Int || 301 || Y coordinate of the beam centre || <br />
|-<br />
|Xdelta || Float || || X step in radians || <br />
|-<br />
|Ydelta || Float || || Y step in radians || <br />
|}<br />
<br />
<br />
<br />
<br />
* Intermediate Beams and Sidelobes are sampled on the sphere. The resolution in <math>\theta</math> and <math>\phi</math> is given by the keywords "Ntheta" and "Nphi". The columns of the BINDATA extension contain the sequence of Nphi Stokes parameters for each <math>\theta</math>.<br />
<br />
{| border="1" cellpadding="3" cellspacing="0" align="center" style="text-align:left" width=800px<br />
|+ '''Intermediate Beam and Sidelobes file structure''' <br />
<br />
|- bgcolor="ffdead"<br />
! Column Name || Data Type || Units || Description ||Comment<br />
|-<br />
|BEAMDATA || Real*4 || none || Stokes parameter I || <br />
|-<br />
|BEAMDATAQ || Real*4 || none || Stokes parameter Q ||<br />
|-<br />
|BEAMDATAU || Real*4 || none || Stokes parameter U ||<br />
|-<br />
|BEAMDATAV || Real*4 || none || Stokes parameter V ||<br />
<br />
|- bgcolor="ffdead" <br />
<br />
! Keyword || Data Type || Value || Description || Comment<br />
|-<br />
|Ntheta || Int || || <math>\theta</math> samples number || colatitude<br />
|-<br />
|Nphi || Int || || <math>\phi</math> samples number || longitude<br />
|-<br />
|Mintheta || Float || || Minimum value of <math>\theta</math> ||<br />
|-<br />
|Maxtheta || Float || || Maximum value of <math>\theta</math> ||<br />
|-<br />
|angularCut || Float || || Angular cut [deg] ||<br />
<br />
|}<br />
<br />
== HFI Beams ==<br />
<br />
The HFI scanning beams are a combination of observations of Saturn, for the central parts, and Jupiter, for the wings, as described in the [[Beams | Beams]] section of this document, and in Section 4.1 of {{PlanckPapers | planck2014-a08}} on ''Hybrid beams''. Saturn data are used where they are signal-dominated; when the SNR of Saturn drops to < 9, Jupiter data are used, after binning them azimuthally. Beyond that, i.e., below the noise floor of the Jupiter data, and out to 100 arcmin, a power law (~θ<sup> -3</sup>) is used, where the exponent is derived from GRASP physical optics models. The figure below, taken from the [[Beams#Key_Changes | Beams]] section of this document, shows graphically the different portions of the beam model.<br />
<br />
<br />
[[Image:HybridBeamDiagram.png|thumb|500px|center| Scanning beam map for detector 143-6 showing a rough diagram of the regions that are handled with a different<br />
data selection or binning.]]<br />
<br />
<br />
The beams are provided in FITS files named <br />
* ''HFI_ScanBeam_{det-name}_R2.nn.fits'', <br />
where ''det-name'' is of the form ''100-1a'', and ''nn'' is the version number. Each file contains a single ''IMAGE'' extension. The image is 6001x6001 pixels of size 2x2 arcsec<sup>2</sup> (given in the ''DELTAX'' and ''DELTAY'' keywords), centred on pixel 3001,3001, and normalised to 1 at the maximum, where ''X'' and ''Y'' and in the Dxx reference system.</div>
Xdupac
https://wiki.cosmos.esa.int/planckpla2015/index.php?title=Scanning_Beams&diff=11454
Scanning Beams
2015-04-15T14:30:15Z
<p>Xdupac: </p>
<hr />
<div>{{DISPLAYTITLE:2015 Scanning Beams}}<br />
<br />
== LFI beams ==<br />
<br />
We released maps of the Stokes parameters of the band-averaged [[Beams LFI#Polarized_Scanning_Beams_and_Focal_Plane_calibration|scanning beams]]. The averages are performed using the [[The_RIMO#LFI_2|RIMO]] bandpass, assuming a flat spectrum of the incoming radiation. The Stokes parameters maps contain the complete information about the field intensity and polarization properties. Main Beam, Intermediate Beam, and Sidelobes are released separately.<br />
<br />
More information on LFI beams can be found at {{PlanckPapers|planck2014-a05}} and on HFI beams at {{PlanckPapers|planck2014-a08}}<br />
<br />
===File Names===<br />
<br />
The file names are of the form:<br />
<br />
''LFI_ScanBeam-{mb,ib,sl}_{fff}-{rrr}_R2.{nn}.stokes''<br />
<br />
where<br />
* ''fff'' denotes the frequency<br />
* ''mb'' denotes the Main Beams<br />
* ''ib'' denotes the Intermediate Beam <br />
* ''sl'' denotes the Sidelobes<br />
* ''rrr'' denotes the radiometer<br />
* ''R2.nn'' is the version.<br />
<br />
<br />
At the present time, HFI is not releasing the Scanning Beams.<br />
<br />
===FITS file structure===<br />
The FITS files contain a primary extension with no data and a minimal header, and one BINTABLE extension with data and with a description of the data in the header keywords. <br />
The BINTABLE extension consist in four columns, each containing the array of one Stokes parameter. <br />
The columns are called:<br />
* ''Beamdata'' , containing <math>I</math><br />
* ''BeamdataQ'', containing <math>Q</math><br />
* ''BeamdataU'', containing <math>U</math><br />
* ''BeamdataV'', containing <math>V</math>.<br />
<br />
Main Beam, Intermediate Beams and Sidelobes are saved with a different data format: <br />
<br />
* Main Beams are projected on the tangent plane to the sphere, and sampled on a grid. The grid include an angular region expressed by the keyword ''angularCut'', and its dimensions are given by the keywords ''Nx'' and ''Ny'', representing the number of columns and rows. Each column of the BINDATA extension contains the sequence of the <math>Nx \times Ny</math> samples of the map in row major order. The keywords ''Xcentre'' and ''Ycentre'' express the coordinates of the beam maximum (i.e. where the sphere intersect the tangent plane).<br />
<br />
{| border="1" cellpadding="3" cellspacing="0" align="center" style="text-align:left" width=800px<br />
|+ '''Main Beam file structure''' <br />
<br />
|- bgcolor="ffdead" <br />
! Column Name || Data Type || Units || Description || Comment<br />
|-<br />
|BEAMDATA || Real*4 || none || Stokes parameter I || <br />
|-<br />
|BEAMDATAQ || Real*4 || none || Stokes parameter Q ||<br />
|-<br />
|BEAMDATAU || Real*4 || none || Stokes parameter U ||<br />
|-<br />
|BEAMDATAV || Real*4 || none || Stokes parameter V ||<br />
<br />
|- bgcolor="ffdead" <br />
<br />
! Keyword || Data Type || Value || Description || Comment<br />
|-<br />
|Nx || Int || 601 || X axis samples number || X axis aligned with the direction of the S arm<br />
|-<br />
|Ny || Int || 601 || Y axis samples number || Y axis aligned with the direction of the M arm<br />
|-<br />
|Xcentre || Int || 301 || X coordinate of the beam centre ||<br />
|-<br />
|Ycentre || Int || 301 || Y coordinate of the beam centre || <br />
|-<br />
|Xdelta || Float || || X step in radians || <br />
|-<br />
|Ydelta || Float || || Y step in radians || <br />
|}<br />
<br />
<br />
<br />
<br />
* Intermediate Beams and Sidelobes are sampled on the sphere. The resolution in <math>\theta</math> and <math>\phi</math> is given by the keywords "Ntheta" and "Nphi". The columns of the BINDATA extension contain the sequence of Nphi Stokes parameters for each <math>\theta</math>.<br />
<br />
{| border="1" cellpadding="3" cellspacing="0" align="center" style="text-align:left" width=800px<br />
|+ '''Intermediate Beam and Sidelobes file structure''' <br />
<br />
|- bgcolor="ffdead"<br />
! Column Name || Data Type || Units || Description ||Comment<br />
|-<br />
|BEAMDATA || Real*4 || none || Stokes parameter I || <br />
|-<br />
|BEAMDATAQ || Real*4 || none || Stokes parameter Q ||<br />
|-<br />
|BEAMDATAU || Real*4 || none || Stokes parameter U ||<br />
|-<br />
|BEAMDATAV || Real*4 || none || Stokes parameter V ||<br />
<br />
|- bgcolor="ffdead" <br />
<br />
! Keyword || Data Type || Value || Description || Comment<br />
|-<br />
|Ntheta || Int || || <math>\theta</math> samples number || colatitude<br />
|-<br />
|Nphi || Int || || <math>\phi</math> samples number || longitude<br />
|-<br />
|Mintheta || Float || || Minimum value of <math>\theta</math> ||<br />
|-<br />
|Maxtheta || Float || || Maximum value of <math>\theta</math> ||<br />
|-<br />
|angularCut || Float || || Angular cut [deg] ||<br />
<br />
== HFI Beams ==<br />
<br />
The HFI scanning beams are a combination of observations of Saturn, for the central parts, and Jupiter, for the wings, as described in the [[Beams | Beams]] section of this document, and in Section 4.1 of {{PlanckPapers | planck2014-a08}} on ''Hybrid beams''. Saturn data are used where they are signal-dominated; when the SNR of Saturn drops to < 9, Jupiter data are used, after binning them azimuthally. Beyond that, i.e., below the noise floor of the Jupiter data, and out to 100 arcmin, a power law (~θ<sup> -3</sup>) is used, where the exponent is derived from GRASP physical optics models. The figure below, taken from the [[Beams#Key_Changes | Beams]] section of this document, shows graphically the different portions of the beam model.<br />
<br />
<br />
[[Image:HybridBeamDiagram.png|thumb|500px|center| Scanning beam map for detector 143-6 showing a rough diagram of the regions that are handled with a different<br />
data selection or binning.]]<br />
<br />
<br />
The beams are provided in FITS files named <br />
* ''HFI_ScanBeam_{det-name}_R2.nn.fits'', <br />
where ''det-name'' is of the form ''100-1a'', and ''nn'' is the version number. Each file contains a single ''IMAGE'' extension. The image is 6001x6001 pixels of size 2x2 arcsec<sup>2</sup> (given in the ''DELTAX'' and ''DELTAY'' keywords), centred on pixel 3001,3001, and normalised to 1 at the maximum, where ''X'' and ''Y'' and in the Dxx reference system.<br />
<br />
<br />
|}</div>
Xdupac
https://wiki.cosmos.esa.int/planckpla2015/index.php?title=Scanning_Beams&diff=11453
Scanning Beams
2015-04-15T14:28:46Z
<p>Xdupac: </p>
<hr />
<div>{{DISPLAYTITLE:2015 Scanning Beams}}<br />
<br />
== LFI beams ==<br />
<br />
We released maps of the Stokes parameters of the band-averaged [[Beams LFI#Polarized_Scanning_Beams_and_Focal_Plane_calibration|scanning beams]]. The averages are performed using the [[The_RIMO#LFI_2|RIMO]] bandpass, assuming a flat spectrum of the incoming radiation. The Stokes parameters maps contain the complete information about the field intensity and polarization properties. Main Beam, Intermediate Beam, and Sidelobes are released separately.<br />
<br />
More information on LFI beams can be found at {{PlanckPapers|planck2014-a05}} and on HFI beams at {{PlanckPapers|planck2014-a08}}<br />
<br />
===File Names===<br />
<br />
The file names are of the form:<br />
<br />
''LFI_ScanBeam-{mb,ib,sl}_{fff}-{rrr}_R2.{nn}.stokes''<br />
<br />
where<br />
* ''fff'' denotes the frequency<br />
* ''mb'' denotes the Main Beams<br />
* ''ib'' denotes the Intermediate Beam <br />
* ''sl'' denotes the Sidelobes<br />
* ''rrr'' denotes the radiometer<br />
* ''R2.nn'' is the version.<br />
<br />
<br />
At the present time, HFI is not releasing the Scanning Beams.<br />
<br />
===FITS file structure===<br />
The FITS files contain a primary extension with no data and a minimal header, and one BINTABLE extension with data and with a description of the data in the header keywords. <br />
The BINTABLE extension consist in four columns, each containing the array of one Stokes parameter. <br />
The columns are called:<br />
* ''Beamdata'' , containing <math>I</math><br />
* ''BeamdataQ'', containing <math>Q</math><br />
* ''BeamdataU'', containing <math>U</math><br />
* ''BeamdataV'', containing <math>V</math>.<br />
<br />
Main Beam, Intermediate Beams and Sidelobes are saved with a different data format: <br />
<br />
* Main Beams are projected on the tangent plane to the sphere, and sampled on a grid. The grid include an angular region expressed by the keyword ''angularCut'', and its dimensions are given by the keywords ''Nx'' and ''Ny'', representing the number of columns and rows. Each column of the BINDATA extension contains the sequence of the <math>Nx \times Ny</math> samples of the map in row major order. The keywords ''Xcentre'' and ''Ycentre'' express the coordinates of the beam maximum (i.e. where the sphere intersect the tangent plane).<br />
<br />
{| border="1" cellpadding="3" cellspacing="0" align="center" style="text-align:left" width=800px<br />
|+ '''Main Beam file structure''' <br />
<br />
|- bgcolor="ffdead" <br />
! Column Name || Data Type || Units || Description || Comment<br />
|-<br />
|BEAMDATA || Real*4 || none || Stokes parameter I || <br />
|-<br />
|BEAMDATAQ || Real*4 || none || Stokes parameter Q ||<br />
|-<br />
|BEAMDATAU || Real*4 || none || Stokes parameter U ||<br />
|-<br />
|BEAMDATAV || Real*4 || none || Stokes parameter V ||<br />
<br />
|- bgcolor="ffdead" <br />
<br />
! Keyword || Data Type || Value || Description || Comment<br />
|-<br />
|Nx || Int || 601 || X axis samples number || X axis aligned with the direction of the S arm<br />
|-<br />
|Ny || Int || 601 || Y axis samples number || Y axis aligned with the direction of the M arm<br />
|-<br />
|Xcentre || Int || 301 || X coordinate of the beam centre ||<br />
|-<br />
|Ycentre || Int || 301 || Y coordinate of the beam centre || <br />
|-<br />
|Xdelta || Float || || X step in radians || <br />
|-<br />
|Ydelta || Float || || Y step in radians || <br />
|}<br />
<br />
<br />
<br />
<br />
* Intermediate Beams and Sidelobes are sampled on the sphere. The resolution in <math>\theta</math> and <math>\phi</math> is given by the keywords "Ntheta" and "Nphi". The columns of the BINDATA extension contain the sequence of Nphi Stokes parameters for each <math>\theta</math>.<br />
<br />
{| border="1" cellpadding="3" cellspacing="0" align="center" style="text-align:left" width=800px<br />
|+ '''Intermediate Beam and Sidelobes file structure''' <br />
<br />
|- bgcolor="ffdead"<br />
! Column Name || Data Type || Units || Description ||Comment<br />
|-<br />
|BEAMDATA || Real*4 || none || Stokes parameter I || <br />
|-<br />
|BEAMDATAQ || Real*4 || none || Stokes parameter Q ||<br />
|-<br />
|BEAMDATAU || Real*4 || none || Stokes parameter U ||<br />
|-<br />
|BEAMDATAV || Real*4 || none || Stokes parameter V ||<br />
<br />
|- bgcolor="ffdead" <br />
<br />
! Keyword || Data Type || Value || Description || Comment<br />
|-<br />
|Ntheta || Int || || <math>\theta</math> samples number || colatitude<br />
|-<br />
|Nphi || Int || || <math>\phi</math> samples number || longitude<br />
|-<br />
|Mintheta || Float || || Minimum value of <math>\theta</math> ||<br />
|-<br />
|Maxtheta || Float || || Maximum value of <math>\theta</math> ||<br />
|-<br />
|angularCut || Float || || Angular cut [deg] ||<br />
<br />
|}</div>
Xdupac
https://wiki.cosmos.esa.int/planckpla2015/index.php?title=Scanning_Beams&diff=11452
Scanning Beams
2015-04-15T14:28:09Z
<p>Xdupac: </p>
<hr />
<div>{{DISPLAYTITLE:2015 Scanning Beams}}<br />
<br />
== LFI beams ==<br />
<br />
We released maps of the Stokes parameters of the band-averaged [[Beams LFI#Polarized_Scanning_Beams_and_Focal_Plane_calibration|scanning beams]]. The averages are performed using the [[The_RIMO#LFI_2|RIMO]] bandpass, assuming a flat spectrum of the incoming radiation. The Stokes parameters maps contain the complete information about the field intensity and polarization properties. Main Beam, Intermediate Beam, and Sidelobes are released separately.<br />
<br />
More information on LFI beams can be found at {{PlanckPapers|planck2014-a05}} and on HFI beams at {{PlanckPapers|planck2014-a08}}<br />
<br />
==File Names==<br />
<br />
The file names are of the form:<br />
<br />
''LFI_ScanBeam-{mb,ib,sl}_{fff}-{rrr}_R2.{nn}.stokes''<br />
<br />
where<br />
* ''fff'' denotes the frequency<br />
* ''mb'' denotes the Main Beams<br />
* ''ib'' denotes the Intermediate Beam <br />
* ''sl'' denotes the Sidelobes<br />
* ''rrr'' denotes the radiometer<br />
* ''R2.nn'' is the version.<br />
<br />
<br />
At the present time, HFI is not releasing the Scanning Beams.<br />
<br />
==FITS file structure==<br />
The FITS files contain a primary extension with no data and a minimal header, and one BINTABLE extension with data and with a description of the data in the header keywords. <br />
The BINTABLE extension consist in four columns, each containing the array of one Stokes parameter. <br />
The columns are called:<br />
* ''Beamdata'' , containing <math>I</math><br />
* ''BeamdataQ'', containing <math>Q</math><br />
* ''BeamdataU'', containing <math>U</math><br />
* ''BeamdataV'', containing <math>V</math>.<br />
<br />
Main Beam, Intermediate Beams and Sidelobes are saved with a different data format: <br />
<br />
* Main Beams are projected on the tangent plane to the sphere, and sampled on a grid. The grid include an angular region expressed by the keyword ''angularCut'', and its dimensions are given by the keywords ''Nx'' and ''Ny'', representing the number of columns and rows. Each column of the BINDATA extension contains the sequence of the <math>Nx \times Ny</math> samples of the map in row major order. The keywords ''Xcentre'' and ''Ycentre'' express the coordinates of the beam maximum (i.e. where the sphere intersect the tangent plane).<br />
<br />
{| border="1" cellpadding="3" cellspacing="0" align="center" style="text-align:left" width=800px<br />
|+ '''Main Beam file structure''' <br />
<br />
|- bgcolor="ffdead" <br />
! Column Name || Data Type || Units || Description || Comment<br />
|-<br />
|BEAMDATA || Real*4 || none || Stokes parameter I || <br />
|-<br />
|BEAMDATAQ || Real*4 || none || Stokes parameter Q ||<br />
|-<br />
|BEAMDATAU || Real*4 || none || Stokes parameter U ||<br />
|-<br />
|BEAMDATAV || Real*4 || none || Stokes parameter V ||<br />
<br />
|- bgcolor="ffdead" <br />
<br />
! Keyword || Data Type || Value || Description || Comment<br />
|-<br />
|Nx || Int || 601 || X axis samples number || X axis aligned with the direction of the S arm<br />
|-<br />
|Ny || Int || 601 || Y axis samples number || Y axis aligned with the direction of the M arm<br />
|-<br />
|Xcentre || Int || 301 || X coordinate of the beam centre ||<br />
|-<br />
|Ycentre || Int || 301 || Y coordinate of the beam centre || <br />
|-<br />
|Xdelta || Float || || X step in radians || <br />
|-<br />
|Ydelta || Float || || Y step in radians || <br />
|}<br />
<br />
<br />
<br />
<br />
* Intermediate Beams and Sidelobes are sampled on the sphere. The resolution in <math>\theta</math> and <math>\phi</math> is given by the keywords "Ntheta" and "Nphi". The columns of the BINDATA extension contain the sequence of Nphi Stokes parameters for each <math>\theta</math>.<br />
<br />
{| border="1" cellpadding="3" cellspacing="0" align="center" style="text-align:left" width=800px<br />
|+ '''Intermediate Beam and Sidelobes file structure''' <br />
<br />
|- bgcolor="ffdead"<br />
! Column Name || Data Type || Units || Description ||Comment<br />
|-<br />
|BEAMDATA || Real*4 || none || Stokes parameter I || <br />
|-<br />
|BEAMDATAQ || Real*4 || none || Stokes parameter Q ||<br />
|-<br />
|BEAMDATAU || Real*4 || none || Stokes parameter U ||<br />
|-<br />
|BEAMDATAV || Real*4 || none || Stokes parameter V ||<br />
<br />
|- bgcolor="ffdead" <br />
<br />
! Keyword || Data Type || Value || Description || Comment<br />
|-<br />
|Ntheta || Int || || <math>\theta</math> samples number || colatitude<br />
|-<br />
|Nphi || Int || || <math>\phi</math> samples number || longitude<br />
|-<br />
|Mintheta || Float || || Minimum value of <math>\theta</math> ||<br />
|-<br />
|Maxtheta || Float || || Maximum value of <math>\theta</math> ||<br />
|-<br />
|angularCut || Float || || Angular cut [deg] ||<br />
<br />
|}</div>
Xdupac
https://wiki.cosmos.esa.int/planckpla2015/index.php?title=Cosmological_Parameters&diff=11451
Cosmological Parameters
2015-04-15T11:38:29Z
<p>Xdupac: A. Lewis correction (removed .corr description)</p>
<hr />
<div>{{DISPLAYTITLE: 2015 Cosmological parameters and MC chains}}<br />
== Description ==<br />
<br />
The 2015 cosmological parameter results explore a variety of cosmological models with combinations of Planck and other data. We provide results from MCMC exploration chains, as well as best fits, and sets of parameter tables. Definitions, conventions and reference are contained in {{PlanckPapers|planck2013-p11}} {{PlanckPapers|planck2014-a15||Planck-2015-A15}}.<br />
<br />
==Production process==<br />
<br />
Parameter chains are produced using CosmoMC, a sampling package available [http://cosmologist.info/cosmomc here]. This includes the sample analysis package (and GUI) GetDist, and the scripts for managing, analysing, and plotting results from the full grid or runs. Chain products provided here have had burn in removed. Some results with additional data are produced by importance sampling.<br />
<br />
Note that the baseline model includes one massive neutrino (0.06eV). Grid outputs include WMAP 9 results for consistent assumptions.<br />
<br />
== Caveats and known issues ==<br />
<br />
# Confidence intervals are derived from the MCMC samples, and assume the input likelihoods are exactly correct, so there is no quantification for systematic errors other than via the covariance, foreground and beam error models assumed in the likelihood codes. <br />
# Non-linear lensing modelling uses Halofit; for some extended models and CMB lensing only analyses, tails of the chains may be away from the domain of validity.<br />
# The CAMB version used for most results is Dec 2014; the Jan 2015 version is used for lensing-only models with neutrinos, and only differs in the neutrino corrections to the Halofit model.<br />
# There is evidence of temperature-polarization leakage that may affect results including high-L polarization; hence use caution in the interpretation of results including polarization<br />
# Alternative CamSpec likelihood results in the tables are generated using a slightly older CosmoMC version, with fewer derived parameters and a slightly different BBN predictions for the helium abundance.<br />
<br />
== Related products ==<br />
<br />
Results of the baseline parameter exploration runs should be reproducible using CosmoMC with the Planck 2015 likelihood codes (when available).<br />
<br />
== Parameter Tables ==<br />
<br />
These list parameter constraints for each considered model and data combination separately. For the baseline likelihood see<br />
<br />
* PDF tables with 68% limits [[Media:baseline_params_table_2015_limit68.pdf]]<br />
* PDF tables with 95% limits [[Media:baseline_params_table_2015_limit95.pdf]]<br />
<br />
There are also larger files including alternative CamSpec and DetSet likelihood results, along with shifts in parameters compared to baseline in units of the baseline error:<br />
<br />
* PDF tables with 68% limits [[Media:params_table_2015_limit68.pdf]]<br />
* PDF tables with 95% limits [[Media:params_table_2015_limit95.pdf]]<br />
<br />
<br />
Data combination tags used to label results are as follows (see {{PlanckPapers|planck2013-p11}} for full description and references):<br />
<br />
<br />
{| class="wikitable" align="center" style="text-align:left" border="1" cellpadding="3" cellspacing="0" width=800px<br />
|+ <br />
|- bgcolor="ffdead" <br />
! Tag|| Data<br />
|-<br />
| '''plikHM''' || baseline high-L Planck power spectra (plik cross half-mission, 30 <= l <= 2508)<br />
|-<br />
| '''plikDS''' || high-L Planck power spectra (plik cross detsets, 30 <= l <= 2508)<br />
|-<br />
| '''CamSpecHM''' || high-L Planck power spectra (CamSpec cross half-mission, 30 <= l <= 2500)<br />
|-<br />
| '''CamSpecDS''' || high-L Planck power spectra (CamSpec cross detsets, 30 <= l <= 2500)<br />
|-<br />
| '''lowl''' || low-L: Planck temperature only (2 <= l <= 29)<br />
|-<br />
| '''lowTEB''' || low-L temperature and LFI polarization (2 <= l <= 29)<br />
|-<br />
| '''lowEB''' || low-L LFI polarization only (2 <= l <= 29)<br />
|-<br />
| '''WMAPTEB''' || low-L temperature, and LFI+WMAP polarization (2 <= l <= 29)<br />
|-<br />
| '''lensing''' || Planck lensing power spectrum reconstruction<br />
|-<br />
| '''lensingonly''' || Planck lensing power spectrum reconstruction only; T,E fixed to best-fit spectrum + priors<br />
|-<br />
| '''BKP''' || The Bicep-Keck-Planck fiducial B mode likelihood<br />
|-<br />
| '''zre6p5''' || A hard prior z_re > 6.5<br />
|-<br />
| '''tau07''' || A Gaussian prior on the optical depth, tau = 0.07 +- 0.02<br />
|-<br />
| '''reion''' || A hard prior z_re > 6.5, combined with Gaussian prior z_re = 7 +- 1<br />
|-<br />
| '''BAO''' || Baryon oscillation data from DR11LOWZ, DR11CMASS, MGS and 6DF<br />
|-<br />
| '''JLA''' || Supernova data from the SDSS-II/SNLS3 Joint Light-curve Analysis<br />
|-<br />
| '''H070p6''' || Hubble parameter constraint, H_0 = 70.6 +- 3.3<br />
|-<br />
| '''theta''' || theta_MC fixed to 1.0408<br />
|-<br />
| '''WLonlyHeymans''' || Conservative cut of the CFHTLenS weak lensing data + priors<br />
|-<br />
| '''WMAP''' || The full WMAP (temperature and polarization) 9 year data <br />
|}<br />
<br />
The high-L Planck likelihoods have TT, TE, EE variants from each spectrum alone, plus the TTTEEE joint constraint.<br />
<br />
<br />
Tags used to identify the model parameters that are varied are described in [[Media:parameter_tag_definitions_2015.pdf]]. <br />
<br />
== Parameter Chains ==<br />
<br />
We provide the full chains and getdist outputs for our parameter results. The entire grid of results is available from as a 3.7GB compressed file:<br />
<!--- * {{PLASingleFile|fileType=cosmo|name= COM_CosmoParams_R2.00.tar.gz|link=Full Grid Download}} ----><br />
* ''COM_CosmoParams_R2.nn.tar.gz''<br />
Where ''nn'' is the most recent update. You can also download the Bicep2/Keck/Planck (BKP) joint constraints for +r models, and smaller files containing key results in the base model only: <br />
<!---* {{PLASingleFile|fileType=cosmo|name=COM_CosmoParams_base_plikHM_TT_lowTEB_R2.00.tar.gz|link=Baseline LCDM chains with plikHM_TT_lowTEB}}<br />
* {{PLASingleFile|fileType=cosmo|name=COM_CosmoParams_base_plikHM_TT_lowTEB_R2.00.tar.gz|link=Baseline LCDM chains with all plikHM combinations}}<br />
* {{PLASingleFile|fileType=cosmo|name=COM_CosmoParams_base_lensonly_R2.00.tar.gz|link=CMB lensing only in LCDM}} ---><br />
* ''COM_CosmoParams_base_plikHM_TT_lowTEB_R2.nn.tar.gz''<br />
* ''COM_CosmoParams_base_plikHM_R2.nn.tar.gz''<br />
* ''COM_CosmoParams_base_lensonly_R2.nn.tar.gz''<br />
* ''COM_CosmoParams_base_r_plikHM_BKP_R2.nn.tar.gz''<br />
<br />
The download contains a hierarchy of directories, with each separate chain in a separate directory. The structure for the directories is<br />
<br />
: '' base_AAA_BBB/XXX_YYY_.../''<br />
<br />
where AAA and BBB are any additional parameters that are varied in addition to the six parameters of the baseline model. XXX, YYY, etc encode the data combinations used. These follow the naming conventions described above under Parameter Tables. Each directory contains the main chains, 4-8 text files with one chain in each, and various other files all with names of the form<br />
<br />
: ''base_AAA_BBB_XXX_YYY.ext''<br />
<br />
where ''ext'' describes the type of file, and the possible values or ''ext'' are<br />
<br />
<br />
{| class="wikitable" align="center" style="text-align:left" border="1" cellpadding="3" cellspacing="0" width=800px<br />
|+ <br />
|- bgcolor="ffdead" <br />
! Extension || Data<br />
|-<br />
| '''.txt''' || parameter chain file with burn in removed<br />
|-<br />
| '''.paramnames''' || File that describes the parameters included in the chains<br />
|-<br />
| '''.inputparams''' || Input parameters used when generating the chain<br />
|-<br />
| '''.minimum''' || Best-fit parameter values, -log likelihoods and chi-square<br />
|-<br />
| '''.minimum.theory_cl''' || The best-fit temperature and polarization power spectra and lensing potential (see below)<br />
|-<br />
| '''.minimum.plik_foregrounds''' || The best-fit foreground model (additive component) for each data power spectrum used<br />
|-<br />
| '''.minimum.inputparams''' || Input parameters used when generating the best fit<br />
|-<br />
| '''.ranges''' || prior ranges assumed for each parameter<br />
|}<br />
<br />
<br />
In addition each directory contains any importance sampled outputs with additional data. These have names of the form<br />
<br />
: ''base_AAA_BBB_XXX_YYY_post_ZZZ.ext''<br />
<br />
where ZZZ is the data likelihood that is added by importance sampling. Finally, each directory contains a ''dist'' subdirectory, containing results of chain analysis. File names follow the above conventions, with the following extensions<br />
<br />
<br />
{| class="wikitable" align="center" style="text-align:left" border="1" cellpadding="3" cellspacing="0" width=800px<br />
|+ <br />
|- bgcolor="ffdead" <br />
! Extension || Data<br />
|-<br />
| '''.margestats''' || mean, variance and 68, 95 and 99% limits for each parameter (see below)<br />
|-<br />
| '''.likestats''' || parameters of best-fitting sample in the chain (generally different from the .minmum global best-fit)<br />
|-<br />
| '''.covmat''' || Covariance matrix for the MCMC parameters<br />
|-<br />
| '''.converge''' || A summary of various convergence diagnostics<br />
|}<br />
<br />
<br />
Python scripts for reading in chains and calculating new derived parameter constraints are available as part of CosmoMC, see the readme for details [http://cosmologist.info/cosmomc/readme_planck.html]. The config directory in the download includes information about the grid configuration used by the plotting and grid scripts.<br />
<br />
== File formats ==<br />
<br />
The file formats are standard Jan 2015 CosmoMC outputs. CosmoMC includes python scripts for generating tables, 1D, 2D and 3D plots using the provided data, as well as a GUI for conveniently making plots from grid downloads. The formats are summarised here:<br />
<br />
; Chain files<br />
: Each chain file is ASCII and contains one sample on each line. Each line is of the format<br />
<br />
: '' weight like param1 param2 param3 …''<br />
<br />
: Here ''weight'' is the importance weight or multiplicity count, and ''like'' is the total -log Likelihood. ''param1'',''param2'', etc are the parameter values for the sample, where the numbering is defined by the position in the accompanying .paramnames files.<br />
<br />
: Note that burn in has been removed from the cosmomc outputs, so full chains provided can be used for analysis. Importance sampled results (with ''_post'') in the name have been thinned by a factor of 10 compared to the original chains, so the files are smaller, but this does not significantly affect the effective number of samples. Note that due to the way MCMC works, the samples in the chain outputs are not independent, but it is safe to use all the samples for estimating posterior averages.<br />
<br />
;.margestats files<br />
: Each row contains the marginalized constraint on individual parameters. The format is fairly self explanatory given the text description in the file, with each line of the form<br />
<br />
: '' parameter mean sddev lower1 upper1 limit1 lower2 upper2 limit2 lower3 upper3 limit3''<br />
<br />
: where sddev is the standard deviation, and the limits are 1: 68%, 2: 95%, 3: 99%. The limit tags specify whether a given limit is one tail, two tail or none (if no constraint within the assumed prior boundary). <br />
<br />
;.minimum.theory_cl files<br />
: They contain the best-fit theoretical power spectra (without foregrounds) for each model. The columns are: <math>l</math>, <math>D^{TT}_l</math>, <math>D^{TE}_l</math>, <math>D^{EE}_l</math>, <math>D^{BB}_l</math>, and <math>D^{dd}_l</math>, were <math>D_l \equiv l(l+1) C_l / (2\pi)</math> in <math>\mu{\rm K}^2</math>. Also <math>D^{dd}_l= [l(l+1)]^2 C^{\phi\phi}_l/(2\pi)</math> is the power spectrum of the lensing deflection angle, where <math>C^{\phi\phi}_l</math> is the lensing potential power spectrum. Note that the lensing spectrum may not be accurate at L > 400 due to the maximum wavenumber and non-linear correction accuracy settings.<br />
<br />
<br />
== References ==<br />
<br />
<br />
<References /><br />
<br />
<br />
<br />
<br />
<br />
[[Category:Mission products|009]]</div>
Xdupac
https://wiki.cosmos.esa.int/planckpla2015/index.php?title=CMB_spectrum_%26_Likelihood_Code&diff=11450
CMB spectrum & Likelihood Code
2015-04-13T11:34:58Z
<p>Xdupac: /* File names and Meta data */</p>
<hr />
<div>{{DISPLAYTITLE:2015 CMB spectra and likelihood code}}<br />
<br />
==2015 CMB spectra==<br />
<br />
<br />
===General description===<br />
====TT====<br />
The Planck best-fit CMB temperature power spectrum, shown in the figure below, covers the wide range of multipoles <math> \ell </math> = 2-2508. Over the multipole range <math> \ell </math> = 2–29, the power spectrum is derived from the ''Commander'': component separation algorithm applied to the combination of Planck 2015 temperature data between 30 and 857 GHz, the 9-year WMAP sky maps, and the 408 MHz Haslam et al. (1982) survey, including 93% of the sky {{PlanckPapers|planck2014-a12}} . The asymmetric error bars associated to this spectrum are the 68% confidence limits and include the uncertainties due to foreground subtraction.<br />
<br />
For multipoles equal or greater than <math>\ell=30</math>, instead, the spectrum is derived from the ''Plik'' likelihood {{PlanckPapers|planck2014-a13}} by optimally combining the spectra in the frequency range 100-217 GHz, and correcting them for unresolved foregrounds using the best-fit foreground solution from a Planck TT+lowP <math>\Lambda</math>CDM run. Associated 1-sigma errors include beam uncertainties. Both ''Commander'' and ''Plik'' are described in more details in the sections below.<br />
<br />
[[File: A15_TT.png|thumb|center|700px|'''The Planck 2015 TT power spectrum. Logarithmic x-scale up to <math>\ell = 30 </math> , linear at higher <math>\ell</math>. The red line is the Planck best-fit primordial power spectrum (cf Planck TT+lowP in Table 3 of Planck-2015-A15[3]). Residuals with respect to this model are shown in the lower panel. The error bars show <math>\pm 1\sigma</math> uncertainties.''']]<br />
<br />
====TE and EE====<br />
The Planck best-fit CMB polarization and temperature-polarization cross-correlation power spectra, shown in the figure below, cover the multipole range <math> \ell </math> = 30-1996. The data points relative to the multipole range <math> \ell </math> = 2-29 will be released in a second moment.<br />
Analogously to the TT case, the <math> \ell\ge 30 </math> spectrum is derived from the ''Plik'' likelihood {{PlanckPapers|planck2014-a13}} by optimally combining the spectra in the frequency range 100-217 GHz, and correcting them for unresolved foregrounds using the best-fit foreground solution from a Planck TT,TE,EE+lowP <math>\Lambda</math>CDM run. <br />
<br />
{|style="margin: 0 auto;"<br />
|[[File: A15_EE.png|thumb|center|500px|'''The Planck 2015 EE power spectrum. The red line is the Planck best-fit primordial power spectrum (cf Planck TT+lowP in Table 3 of Planck-2015-A15). Residuals with respect to this model are shown in the lower panel. The error bars show <math>\pm 1\sigma</math> uncertainties. The green lines in the lower panels show the best-fit temperature-to-polarization leakage model of Eqs. (11a) and (11b) in Planck-2015-A15.''']]<br />
|[[File: A15_TE.png|thumb|center|500px|'''The Planck 2015 TE power spectrum. The red line is the Planck best-fit primordial power spectrum (cf Planck TT+lowP in Table 3 of Planck-2015-A15). Residuals with respect to this model are shown in the lower panel. The error bars show <math>\pm 1\sigma</math> uncertainties. The green lines in the lower panels show the best-fit temperature-to-polarization leakage model of Eqs. (11a) and (11b) in Planck-2015-A15.''']]<br />
|}<br />
<br />
===Production process===<br />
The <math>\ell</math> < 30 part of the Planck TT power spectrum is derived from the Commander approach, which implements Bayesian component separation in pixel space, fitting a parametric model to the data by sampling the posterior distribution for the model parameters {{PlanckPapers|planck2014-a12}}. The power spectrum at any multipole <math>\ell</math> is given as the maximum probability point for the posterior <math>C_\ell</math> distribution, marginalized over the other multipoles, and the error bars are 68% confidence level; see {{PlanckPapers|planck2014-a12}}. <br />
<br />
The <math>\ell \ge 30</math> part of the TT, TE and EE power spectra have been derived by the Plik likelihood, a code that implements a pseudo-Cl based technique, extensively described in Sec. 2 and the Appendix of {{PlanckPapers|planck2013-p08}} and {{PlanckPapers|planck2014-a13}}. Frequency spectra are computed as cross-spectra between half-mission maps. Mask and multipole range choices for each frequency spectrum are summarized in Section 3.3 of {{PlanckPapers|planck2014-a15}} and in {{PlanckPapers|planck2014-a13}}. The final power spectrum is an optimal combination of the 100, 143, 143x217 and 217 GHz spectra, corrected for the best-fit unresolved foregrounds and inter-frequency calibration factors, as derived from the full likelihood analysis (for TT we use the best-fit solutions for the nuisance parameters from the Planck+TT+lowP data combination, while for TE and EE we use the best fit from Planck+TT+lowP, cf Table 3 of {{PlanckPapers|planck2014-a15}}). A thorough description of the models of unresolved foregrounds is given in {{PlanckPapers|planck2014-a13}}. The spectrum covariance matrix accounts for cosmic variance and noise contributions, together with beam uncertainties. The <math>\ell \ge 30</math> CMB TT spectrum and associated covariance matrix are available in two formats:<br />
#Unbinned. TT: 2479 bandpowers (<math>\ell=30-2508</math>); TE or EE: 1697 bandpowers (<math>\ell=30-1996</math>).<br />
#Binned, in bins of <math> \Delta\ell=30 </math>. TT: 83 bandpowers. TE or EE: 66 bandpowers. We bin the <math> C_\ell </math> power spectrum with a weight proportional to <math> \ell (\ell+1) </math>, so that the <math> C_{\ell_b} </math> binned bandpower centered in <math> \ell_b </math> is: <math> \\ C_{\ell_b}=\Sigma_{\ell \in b} w_{\ell_b\ell} C_\ell \quad \text{with} \quad w_{\ell_b\ell}=\frac{\ell (\ell+1)}{\Sigma_{\ell \in b} \ell (\ell+1)}. \\</math> Equivalently, using the matrix formalism, we can construct the binning matrix B as: <math>\\ B_{\ell_b \ell}=w_{\ell_b\ell} \\ </math> where B is a <math> n_b\times n_\ell</math> matrix, with <math>n_b=83</math> the number of bins and <math>n_\ell=2479</math> the number of unbinned multipoles. Thus: <math> \\ \vec{C}_\mathrm{binned}=B \, \vec{C} \\ \mathrm{cov_\mathrm{binned}}= B\, \mathrm{cov}\, B^T \\ \ell_b=B\, \ell \\ </math> Here, <math> \vec{C}_{binned}\, (\vec{C}) </math> is the vector containing all the binned (unbinned) <math>C_\ell</math> bandpowers, <math>\mathrm{cov} </math> is the covariance matrix and <math>\ell_b</math> is the weighted average multipole in each bin. Note that following this definition, <math>\ell_b</math> can be a non-integer. The binned <math>D_{\ell_B}</math> power spectrum is then calculated as: <math> \\ D_{\ell_b}=\frac{\ell_b (\ell_b+1)}{2\pi} C_{\ell_b} </math>.<br />
<br />
===Inputs===<br />
<br />
; Low-l spectrum (<math>\ell < 30</math>):<br />
* Planck 30 and 44 GHz frequency maps<br />
* Planck 70 to 857 GHz detector and detector set maps<br />
* 9-year WMAP temperature sky maps between 23 and 94 GHz<br />
* 408 MHz survey by Haslam et al. (1982) <br />
* Commander <math>\chi^2</math> based LM93 confidence mask {{PlanckPapers|planck2014-a12}}<br />
<br />
; High-l spectrum (<math>30 \le \ell \le 2508</math>): <br />
<br />
* 100, 143, 143x217 and 217 GHz spectra and their covariance matrix (Sec. 3.3 {{PlanckPapers|planck2014-a15}})<br />
* best-fit foreground templates and inter-frequency calibration factors (Table 3 of {{PlanckPapers|planck2014-a15}})<br />
* Beam transfer function uncertainties {{PlanckPapers|planck2014-a08}}<br />
=== File names and Meta data ===<br />
<br />
The CMB spectrum and its covariance matrix are distributed in a single FITS file named <br />
<!--- * ''{{PLASingleFile | fileType=cosmo | name=COM_PowerSpect_CMB_R2.00.fits | link=COM_PowerSpect_CMB_R1.10.fits}}'' ---><br />
* ''COM_PowerSpect_CMB_R2.nn.fits''<br />
which contains 7 ''BINTABLE'' extensions<br />
<br />
; 1. TT low-ell, unbinned (TTLOLUNB)<br />
: with the low ell part of the spectrum, not binned, and for l=2-29. The table columns are<br />
# ''ELL'' (integer): multipole number<br />
# ''D_ELL'' (float): <math>D_ell</math> as described above<br />
# ''ERRUP'' (float): the upward uncertainty<br />
# ''ERRDOWN'' (float): the downward uncertainty<br />
<br />
; 2. TT high-ell, binned (TTHILBIN)<br />
: with the high-ell part of the spectrum, binned into 83 bins covering <math>\langle l \rangle = 47-2499\ </math> in bins of width <math>l=30</math> (with the exception of the last bin that is smaller). The table columns are as follows:<br />
# ''ELL'' (integer): mean multipole number of bin<br />
# ''L_MIN'' (integer): lowest multipole of bin<br />
# ''L_MAX'' (integer): highest multipole of bin<br />
# ''D_ELL'' (float): <math>D_\ell</math> as described above<br />
# ''ERR'' (float): the uncertainty<br />
<br />
; 3. TT high-ell unbinned (TTHILUNB) <br />
: with the high-ell part of the spectrum, unbinned, in 2979 bins covering <math>\langle l \rangle = 30-2508\ </math>. The table columns are as follows:<br />
# ''ELL'' (integer): multipole <br />
# ''D_ELL'' (float): <math>D_\ell</math> as described above<br />
# ''ERR'' (float): the uncertainty<br />
<br />
; 4. TE high-ell, binned (TEHILBIN) <br />
: with the high-ell part of the spectrum, binned into 83 bins covering <math>\langle l \rangle = 47-1988\ </math> in bins of width <math>l=30</math> (with the exception of the last bin that is smaller). The table columns are as follows:<br />
# ''ELL'' (integer): mean multipole number of bin<br />
# ''L_MIN'' (integer): lowest multipole of bin<br />
# ''L_MAX'' (integer): highest multipole of bin<br />
# ''D_ELL'' (float): <math>D_\ell</math> as described above<br />
# ''ERR'' (float): the uncertainty<br />
<br />
; 5. TE high-ell, unbinned (TEHILUNB) <br />
: with the high-ell part of the spectrum, unbinned, in 2979 bins covering <math>\langle l \rangle = 30-1996\ </math>. The table columns are as follows:<br />
# ''ELL'' (integer): multipole <br />
# ''D_ELL'' (float): <math>D_\ell</math> as described above<br />
# ''ERR'' (float): the uncertainty<br />
<br />
; 6. EE high-ell, binned (EEHILBIN) <br />
: with the high-ell part of the spectrum, binned into 83 bins covering <math>\langle l \rangle = 47-1988\ </math> in bins of width <math>l=30</math> (with the exception of the last bin that is smaller). The table columns are as follows:<br />
# ''ELL'' (integer): mean multipole number of bin<br />
# ''L_MIN'' (integer): lowest multipole of bin<br />
# ''L_MAX'' (integer): highest multipole of bin<br />
# ''D_ELL'' (float): <math>D_\ell</math> as described above<br />
# ''ERR'' (float): the uncertainty<br />
<br />
; 7. EE high-ell, unbinned (EEHILUNB) <br />
: with the high-ell part of the spectrum, unbinned, in 2979 bins covering <math>\langle l \rangle = 30-1996\ </math>. The table columns are as follows:<br />
# ''ELL'' (integer): multipole <br />
# ''D_ELL'' (float): <math>D_\ell</math> as described above<br />
# ''ERR'' (float): the uncertainty<br />
<br />
<br />
The spectra give <math>D_\ell = \ell(\ell+1)C_\ell / 2\pi </math> in units of <math>\mu\, K^2</math>. The covariance matrices of the spectra will be released in a second moment.<br />
<!-- <br />
<br />
The CMB spectrum is also given in a simple text comma-separated file:<br />
* ''{{PLASingleFile | fileType=cosmo | name=COM_PowerSpect_CMB_R1.10.txt |link=COM_PowerSpect_CMB_R1.10.txt}}''<br />
<br />
--><br />
<br />
==Likelihood==<br />
The likelihood code will released in March-April 2015 with an accompanying paper and an Explanatory Supplement update. <br />
<!-- <br />
===Likelihood===<br />
<span style="color:red"> ALL OF THE FOLLOWING IN THE LIKELIHOOD SECTION IS OLD. </span><br />
The likelihood code (and the data that comes with it) used to compute the likelihood of a model that predicts the CMB power spectra, lensing power spectrum, together with some foreground and some instrumental parameters. The data files are built primarily from the Planck mission results, but include also some results from the WMAP-9 data release. The data files are written in a specific format that can only be read by the code. The code consists in a c/f90 library, along with some optional tools in python. The code is used to read the data files, and given model power spectra and nuisance parameters it computes the log likelihood of that model. <br />
<br />
Detailed description of the installation and usage of the likelihood code and data is provided in the package. The package includes five data files: four for the CMB likelihoods and one for the lensing likelihood. All of the likelihoods delivered are described in detail in the {{PlanckPapers|planck2013-p08|1|Power spectrum & Likelihood Paper}} (for the CMB based likelihood) and in the {{PlanckPapers|planck2013-p12|1|Lensing Paper}} (for the lensing likelihood) .<br />
<br />
The CMB full likelihood has been divided into four parts to allow using selectively different ranges of multipoles. It also reflects the fact that the mathematical approximations used for those different parts are very different, as is the underlying data. In detail, we distribute<br />
* one low-<math>\ell</math> temperature only likelihood (commander), <br />
* one low-<math>\ell</math> temperature and polarisation likelihood (lowlike), and <br />
* one higl-<math>\ell</math> likelihood CAMspec. <br />
<br />
The ''Commander'' likelihood covers the multipoles 2 to 49. It uses a semi-analytic method to sample the low-<math>\ell</math> temperature likelihood on an intermediate product of one of the component separated maps. The samples are used along with an analytical approximation of the likelihood posterior to perform the likelihood computation in the code. See {{PlanckPapers|planck2013-p08}} section 8.1 for more details.<br />
<br />
The ''lowlike'' likelihood covers the multipoles 2 to 32 for temperature and polarization data. Since Planck is not releasing polarisation data at this time, the polarization map from WMAP9 is used instead. A temperature map is needed to perform the computation nevertheless, and we use here the same commander map. The likelihood is computed using a map-based approximation at low resolution and a master one at intermediate resolution, as in WMAP. The likelihood code actually calls a very slightly modified version of the WMAP9 code. This piece of the likelihood essentially provides a prior on the optical depth and has almost no other impact on cosmological parameter estimation. As such it could be replaced by a simple prior, and a user can decide to do so, which is one of the motivation to leave the three pieces of the CMB likelihood as different data packages; see {{PlanckPapers|planck2013-p08}} section 8.3 for more details. Note that the version of the WMAP code used here (code version v1.0) does not perform any test on the positive definiteness of the TT, TE, EE covariance matrices, and will return a null log likelihood in the unphysical cases where the absolute value of TE is too large. This will be corrected in a later version.<br />
<br />
The ''CAMspec'' likelihood covers the multipoles 50 to 2500 for temperature only. The likelihood is computed using a quadratic approximation, including mode to mode correlations that have been precomputed on a fiducial model. The likelihood uses data from the 100, 143 and 217 GHz channels. To do so it models the foreground at each frequency using the model described in the likelihood paper. Uncertainties on the relative calibration and on the beam transfer functions are included either as parametric models, or marginalized and integrated in the covariance matrix. Detailed description of the different nuisance parameters is given below. Priors are included in the likelihood on the CIB spectral index, relative calibration factors and beam error eigenmodes. See {{PlanckPapers|planck2013-p08}} section 2.1 for more details.<br />
<br />
The ''act/spt'' likelihood covers the multipoles 1500 to 10000 for temperature. It is described in{{BibCite|dun2013}}{{BibCite|Keis2011}}{{BibCite|Reic2012}}. It uses the code and data that can be retrieved from the [http://lambda.gsfc.nasa.gov/ Lambda archive] for [http://lambda.gsfc.nasa.gov/product/act/act_prod_table.cfm ACT] and [http://lambda.gsfc.nasa.gov/product/spt/spt_prod_table.cfm SPT]. It has been slightly modified to use a thermal and kinetic SZ model that matches the one used in CAMspec. As stated in{{BibCite|dun2013}}, the dust parameters a_ge and a_gs must be explored with the following priors: a_ge = 0.8 ± 0.2 and a_gs = 0.4 ± 0.2. Those priors are not included in the log likelihood computed by the code.<br />
<br />
The ''lensing'' likelihood covers the multipoles 40 to 400 using the result of the [[Specially_processed_maps | lensing reconstruction]]. It uses a quadratic approximation for the likelihood, with a covariance matrix including the marginalized contribution of the beam transfer function uncertainties, the diffuse point source correction uncertainties and the cosmological model uncertainty affecting the first order non-gaussian bias (N1). The correlation between temperature and lensing is not taken into account. Cosmological uncertainty effects on the normalization are dealt with using a first order renormalization procedure. This means that the code will need both the TT and $\phi\phi$ power spectrum up to <math>\ell</math> = 2048 to correctly perform the integrals needed for the renormalization. Nevertheless, the code will only produce an estimate based on the data between <math>\ell</math> = 40 to 400. See {{PlanckPapers|planck2013-p12}} section 6.1 for more details.<br />
</span><br />
<span style="color:red">OUTSTANDING: description of likelihood masks </span><br />
==Production process==<br />
<br />
===Likelihood===<br />
<span style="color:red"> ALL OF THE FOLLOWING IN THE LIKELIHOOD SECTION IS OLD. </span><br />
The code is based on some basic routines from the libpmc library in the [http://arxiv.org/abs/1101.0950 cosmoPMC] code. It also uses some code from the [http://lambda.gsfc.nasa.gov/product/map/dr5/likelihood_get.cfm WMAP9 likelihood] for the lowlike likelihood and{{BibCite|dun2013}}{{BibCite|Keis2011}}{{BibCite|Reic2012}} for the act/spt one. The rest of the code has been specifically written for the Planck data. Each likelihood file has been processed using a different and dedicated pipeline as described in the likelihood paper {{PlanckPapers|planck2013-p08}} (section 2 and 8) and in the lensing paper {{PlanckPapers|planck2013-p12}} (section 6.1). We refer the reader to those papers for full details. The data are then encapsulated into the specific file format.<br />
<br />
Each dataset comes with its own self check. Whenever the code is used to read a data file, a computation will be done against an included test spectrum/nuisance parameter, and the log-likelihood will be displayed along with the expected result. Difference of the order of 10<math>^{-6}</math> or less are expected depending of the architecture.<br />
<br />
==Inputs==<br />
<br />
===Likelihood===<br />
<br />
; ''commander'' :<br />
* all Planck channels maps<br />
* compact source catalogs<br />
* common masks<br />
* beam transfer functions for all channels<br />
<br />
; ''lowlike'' :<br />
* WMAP9 likelihood data<br />
* Low-<math>\ell</math> Commander map<br />
<br />
; ''CAMspec'' :<br />
* 100, 143 and 217 GHz detector and detsets maps<br />
* 857GHz channel map<br />
* compact source catalog<br />
* common masks (0,1 & 3)<br />
* beam transfer function and error eigenmodes and covariance for 100, 143 and 217 GHz detectors & detsets<br />
* theoretical templates for the tSZ and kSZ contributions<br />
* color corrections for the CIB emission for the 143 and 217GHz detectors and detsets<br />
* fiducial CMB model (bootstrapped from WMAP7 best fit spectrum) estimated noise contribution from the half-ring maps for 100, 143 and 217 GHz<br />
<br />
; ''lensing'' :<br />
* the lensing map<br />
* beam error eigenmodes and covariance for the 143 and 217GHz channel maps<br />
* fiducial CMB model (from Planck cosmological parameter best fit)<br />
<br />
; ''act/spt'' :<br />
* data and code from [http://lambda.gsfc.nasa.gov/product/act/act_fulllikelihood_get.cfm here]<br />
* the tSZ andkSZ template are changed to match those of CAMspec<br />
<br />
== File names and Meta data ==<br />
<br />
===Likelihood===<br />
<span style="color:red"> ALL OF THE FOLLOWING IN THE LIKELIHOOD SECTION IS OLD. </span><br />
<br />
'''Likelihood source code'''<br />
<br />
The source code is in the file<br />
: {{PLASingleFile |fileType=cosmo|name=COM_Code_Likelihood-v1.0_R1.10.tar.gz|link=COM_Code_Likelihood-v1.0_R1.10.tar.gz}} (C, f90 and python likelihood library and tools)<br />
<br />
'''Likelihood data packages'''<br />
<br />
The {{PLALikelihood|type=Data|link=data packages}} are<br />
: ''{{PLASingleFile | fileType=cosmo | name=COM_Data_Likelihood-commander_R1.10.tar.gz | link=COM_Data_Likelihood-commander_R1.10.tar.gz}}'' (low-ell TT likelihood)<br />
: ''{{PLASingleFile | fileType=cosmo | name=COM_Data_Likelihood-lowlike_R1.10.tar.gz | link=COM_Data_Likelihood-lowlike_R1.10.tar.gz}}'' (low-ell TE,EE,BB likelihood)<br />
: ''{{PLASingleFile | fileType=cosmo | name=COM_Data_Likelihood-CAMspec_R1.10.tar.gz | link=COM_Data_Likelihood-CAMspec_R1.10.tar.gz}}'' (high-ell TT likelihood)<br />
: ''{{PLASingleFile | fileType=cosmo | name=COM_Data_Likelihood-actspt_R1.10.tar | link=COM_Data_Likelihood-actspt_R1.10.tar.gz}}'' (high-ell TT likelihood)<br />
: ''{{PLASingleFile | fileType=cosmo | name=COM_Data_Likelihood-lensing_R1.10.tar.gz | link=COM_Data_Likelihood-lensing_R1.10.tar.gz}}'' (lensing likelihood)<br />
<br />
Untar and unzip all files to recover the code and likelihood data. Each package comes with a README file; follow the instructions inclosed to<br />
build the code and use it. To compute the CMB likelihood one has to sum the log likelihood of each of the commander_v4.1_lm49.clik, lowlike_v222.clik and CAMspec_v6.2TN_2013_02_26.clik, actspt_2013_01.clik. To compute the CMB+lensing likelihood, one has to sum the log likelihood of all 5 files.<br />
<br />
The CMB and lensing likelihood format are different. The CMB files have the termination .clik, the lensing one .clik_lensing. The lensing data being simpler (due to the less detailled modeling permitted by the lower signal-noise), the file is a simple ascii file containing all the data along with comments describing it, and linking the different quantities to the lensing paper. The CMB file format is more complex and must accommodate different forms of data (maps, power spectrum, distribution samples, covariance matrices...). It consists of a tree structure containing the data. At each level of the tree structure a given directory can contain array data (in the form of FITS files or ascii files for strings) and scalar data (joined in a single ascii file "_mdb"). Those files are not user modifiable and do not contain interesting meta data for the user. Tools to manipulate those files are included in the code package as optional python tools. They are documented in the code package.<br />
<br />
'''Likelihood masks'''<br />
<br />
The masks used in the Likelihood paper {{PlanckPapers|planck2013-p08}} are found in<br />
{{PLASingleFile|fileType=map|name=COM_Mask_Likelihood_2048_R1.10.fits|link=COM_Mask_Likelihood_2048_R1.10.fits}}<br />
<br />
which contains ten masks which are written into a single ''BINTABLE'' extension of 10 columns by 50331648 rows (the number of Healpix pixels in an Nside = 2048 map). The structure is as follows, where the column names are the names of the masks: <br />
<br />
{| border="1" cellpadding="3" cellspacing="0" align="center" style="text-align:left" width=800px<br />
|+ '''Likelihodd masks file data structure'''<br />
|- bgcolor="ffdead" <br />
!colspan="4" | 1. EXTNAME = 'MSK-LIKE' : Data columns<br />
|- bgcolor="ffdead" <br />
! Column Name || Data Type || Units || Description<br />
|-<br />
|CL31 || Real*4 || none || mask<br />
|-<br />
|CL39 || Real*4 || none || mask<br />
|-<br />
|CL49 || Real*4 || none || mask<br />
|-<br />
|G22 || Real*4 || none || mask <br />
|-<br />
|G35 || Real*4 || none || mask<br />
|-<br />
|G45 || Real*4 || none || mask<br />
|-<br />
|G56 || Real*4 || none || mask<br />
|-<br />
|G65 || Real*4 || none || mask<br />
|-<br />
|PS96 || Real*4 || none || mask<br />
|-<br />
|PSA82 || Real*4 || none || mask<br />
|-<br />
|- bgcolor="ffdead" <br />
! Keyword || Data Type || Value || Description<br />
|-<br />
|PIXTYPE || string || HEALPIX ||<br />
|-<br />
|COORDSYS || string || GALACTIC ||Coordinate system <br />
|-<br />
|ORDERING || string || NESTED || Healpix ordering<br />
|-<br />
|NSIDE || Int || 2048 || Healpix Nside <br />
|-<br />
|FIRSTPIX || Int*4 || 0 || First pixel number<br />
|-<br />
|LASTPIX || Int*4 || 50331647 || Last pixel number, for LFI and HFI, respectively<br />
<br />
|}<br />
--><br />
<br />
== References ==<br />
<References /><br />
<br />
<br />
<br />
[[Category:Mission products|008]]</div>
Xdupac
https://wiki.cosmos.esa.int/planckpla2015/index.php?title=CMB_spectrum_%26_Likelihood_Code&diff=11444
CMB spectrum & Likelihood Code
2015-02-09T09:53:58Z
<p>Xdupac: /* TE and EE */</p>
<hr />
<div>{{DISPLAYTITLE:2015 CMB spectra and likelihood code}}<br />
<br />
==2015 CMB spectra==<br />
<br />
<br />
===General description===<br />
====TT====<br />
The Planck best-fit CMB temperature power spectrum, shown in the figure below, covers the wide range of multipoles <math> \ell </math> = 2-2508. Over the multipole range <math> \ell </math> = 2–29, the power spectrum is derived from the ''Commander'': component separation algorithm applied to the combination of Planck 2015 temperature data between 30 and 857 GHz, the 9-year WMAP sky maps, and the 408 MHz Haslam et al. (1982) survey, including 93% of the sky {{PlanckPapers|planck2014-a12}} . The asymmetric error bars associated to this spectrum are the 68% confidence limits and include the uncertainties due to foreground subtraction.<br />
<br />
For multipoles equal or greater than <math>\ell=30</math>, instead, the spectrum is derived from the ''Plik'' likelihood {{PlanckPapers|planck2014-a13}} by optimally combining the spectra in the frequency range 100-217 GHz, and correcting them for unresolved foregrounds using the best-fit foreground solution from a Planck TT+lowP <math>\Lambda</math>CDM run. Associated 1-sigma errors include beam uncertainties. Both ''Commander'' and ''Plik'' are described in more details in the sections below.<br />
<br />
[[File: A15_TT.png|thumb|center|700px|'''The Planck 2015 TT power spectrum. Logarithmic x-scale up to <math>\ell = 30 </math> , linear at higher <math>\ell</math>. The red line is the Planck best-fit primordial power spectrum (cf Planck TT+lowP in Table 3 of Planck-2015-A15[3]). Residuals with respect to this model are shown in the lower panel. The error bars show <math>\pm 1\sigma</math> uncertainties.''']]<br />
<br />
====TE and EE====<br />
The Planck best-fit CMB polarization and temperature-polarization cross-correlation power spectra, shown in the figure below, cover the multipole range <math> \ell </math> = 30-1996. The data points relative to the multipole range <math> \ell </math> = 2-29 will be released in a second moment.<br />
Analogously to the TT case, the <math> \ell\ge 30 </math> spectrum is derived from the ''Plik'' likelihood {{PlanckPapers|planck2014-a13}} by optimally combining the spectra in the frequency range 100-217 GHz, and correcting them for unresolved foregrounds using the best-fit foreground solution from a Planck TT,TE,EE+lowP <math>\Lambda</math>CDM run. <br />
<br />
{|style="margin: 0 auto;"<br />
|[[File: A15_EE.png|thumb|center|500px|'''The Planck 2015 EE power spectrum. The red line is the Planck best-fit primordial power spectrum (cf Planck TT+lowP in Table 3 of Planck-2015-A15). Residuals with respect to this model are shown in the lower panel. The error bars show <math>\pm 1\sigma</math> uncertainties. The green lines in the lower panels show the best-fit temperature-to-polarization leakage model of Eqs. (11a) and (11b) in Planck-2015-A15.''']]<br />
|[[File: A15_TE.png|thumb|center|500px|'''The Planck 2015 TE power spectrum. The red line is the Planck best-fit primordial power spectrum (cf Planck TT+lowP in Table 3 of Planck-2015-A15). Residuals with respect to this model are shown in the lower panel. The error bars show <math>\pm 1\sigma</math> uncertainties. The green lines in the lower panels show the best-fit temperature-to-polarization leakage model of Eqs. (11a) and (11b) in Planck-2015-A15.''']]<br />
|}<br />
<br />
===Production process===<br />
The <math>\ell</math> < 30 part of the Planck TT power spectrum is derived from the Commander approach, which implements Bayesian component separation in pixel space, fitting a parametric model to the data by sampling the posterior distribution for the model parameters {{PlanckPapers|planck2014-a12}}. The power spectrum at any multipole <math>\ell</math> is given as the maximum probability point for the posterior <math>C_\ell</math> distribution, marginalized over the other multipoles, and the error bars are 68% confidence level; see {{PlanckPapers|planck2014-a12}}. <br />
<br />
The <math>\ell \ge 30</math> part of the TT, TE and EE power spectra have been derived by the Plik likelihood, a code that implements a pseudo-Cl based technique, extensively described in Sec. 2 and the Appendix of {{PlanckPapers|planck2013-p08}} and {{PlanckPapers|planck2014-a13}}. Frequency spectra are computed as cross-spectra between half-mission maps. Mask and multipole range choices for each frequency spectrum are summarized in Section 3.3 of {{PlanckPapers|planck2014-a15}} and in {{PlanckPapers|planck2014-a13}}. The final power spectrum is an optimal combination of the 100, 143, 143x217 and 217 GHz spectra, corrected for the best-fit unresolved foregrounds and inter-frequency calibration factors, as derived from the full likelihood analysis (for TT we use the best-fit solutions for the nuisance parameters from the Planck+TT+lowP data combination, while for TE and EE we use the best fit from Planck+TT+lowP, cf Table 3 of {{PlanckPapers|planck2014-a15}}). A thorough description of the models of unresolved foregrounds is given in {{PlanckPapers|planck2014-a13}}. The spectrum covariance matrix accounts for cosmic variance and noise contributions, together with beam uncertainties. The <math>\ell \ge 30</math> CMB TT spectrum and associated covariance matrix are available in two formats:<br />
#Unbinned. TT: 2479 bandpowers (<math>\ell=30-2508</math>); TE or EE: 1697 bandpowers (<math>\ell=30-1996</math>).<br />
#Binned, in bins of <math> \Delta\ell=30 </math>. TT: 83 bandpowers. TE or EE: 66 bandpowers. We bin the <math> C_\ell </math> power spectrum with a weight proportional to <math> \ell (\ell+1) </math>, so that the <math> C_{\ell_b} </math> binned bandpower centered in <math> \ell_b </math> is: <math> \\ C_{\ell_b}=\Sigma_{\ell \in b} w_{\ell_b\ell} C_\ell \quad \text{with} \quad w_{\ell_b\ell}=\frac{\ell (\ell+1)}{\Sigma_{\ell \in b} \ell (\ell+1)}. \\</math> Equivalently, using the matrix formalism, we can construct the binning matrix B as: <math>\\ B_{\ell_b \ell}=w_{\ell_b\ell} \\ </math> where B is a <math> n_b\times n_\ell</math> matrix, with <math>n_b=83</math> the number of bins and <math>n_\ell=2479</math> the number of unbinned multipoles. Thus: <math> \\ \vec{C}_\mathrm{binned}=B \, \vec{C} \\ \mathrm{cov_\mathrm{binned}}= B\, \mathrm{cov}\, B^T \\ \ell_b=B\, \ell \\ </math> Here, <math> \vec{C}_{binned}\, (\vec{C}) </math> is the vector containing all the binned (unbinned) <math>C_\ell</math> bandpowers, <math>\mathrm{cov} </math> is the covariance matrix and <math>\ell_b</math> is the weighted average multipole in each bin. Note that following this definition, <math>\ell_b</math> can be a non-integer. The binned <math>D_{\ell_B}</math> power spectrum is then calculated as: <math> \\ D_{\ell_b}=\frac{\ell_b (\ell_b+1)}{2\pi} C_{\ell_b} </math>.<br />
<br />
===Inputs===<br />
<br />
; Low-l spectrum (<math>\ell < 30</math>):<br />
* Planck 30 and 44 GHz frequency maps<br />
* Planck 70 to 857 GHz detector and detector set maps<br />
* 9-year WMAP temperature sky maps between 23 and 94 GHz<br />
* 408 MHz survey by Haslam et al. (1982) <br />
* Commander <math>\chi^2</math> based LM93 confidence mask {{PlanckPapers|planck2014-a12}}<br />
<br />
; High-l spectrum (<math>30 \le \ell \le 2508</math>): <br />
<br />
* 100, 143, 143x217 and 217 GHz spectra and their covariance matrix (Sec. 3.3 {{PlanckPapers|planck2014-a15}})<br />
* best-fit foreground templates and inter-frequency calibration factors (Table 3 of {{PlanckPapers|planck2014-a15}})<br />
* Beam transfer function uncertainties {{PlanckPapers|planck2014-a08}}<br />
=== File names and Meta data ===<br />
<br />
The CMB spectrum and its covariance matrix are distributed in a single FITS file named <br />
<!--- * ''{{PLASingleFile | fileType=cosmo | name=COM_PowerSpect_CMB_R2.00.fits | link=COM_PowerSpect_CMB_R1.10.fits}}'' ---><br />
* ''COM_PowerSpect_CMB_R2.nn.fits''<br />
which contains 7 ''BINTABLE'' extensions<br />
<br />
; 1. TT low-ell, unbinned (TTLOLUNB)<br />
: with the low ell part of the spectrum, not binned, and for l=2-29. The table columns are<br />
# ''ELL'' (integer): multipole number<br />
# ''D_ELL'' (float): <math>D_ell</math> as described above<br />
# ''ERRUP'' (float): the upward uncertainty<br />
# ''ERRDOWN'' (float): the downward uncertainty<br />
<br />
; 2. TT high-ell, binned (TTHILBIN)<br />
: with the high-ell part of the spectrum, binned into 83 bins covering <math>\langle l \rangle = 47-2499\ </math> in bins of width <math>l=30</math> (with the exception of the last bin that is smaller). The table columns are as follows:<br />
# ''ELL'' (integer): mean multipole number of bin<br />
# ''L_MIN'' (integer): lowest multipole of bin<br />
# ''L_MAX'' (integer): highest multipole of bin<br />
# ''D_ELL'' (float): <math>D_\ell</math> as described above<br />
# ''ERR'' (float): the uncertainty<br />
<br />
; 3. TT high-ell unbinned (TTHILUNB) <br />
: with the high-ell part of the spectrum, unbinned, in 2979 bins covering <math>\langle l \rangle = 30-2508\ </math>. The table columns are as follows:<br />
# ''ELL'' (integer): multipole <br />
# ''D_ELL'' (float): <math>D_\ell</math> as described above<br />
# ''ERR'' (float): the uncertainty<br />
<br />
; 4. TE high-ell, binned (TEHILBIN) <br />
: with the high-ell part of the spectrum, binned into 83 bins covering <math>\langle l \rangle = 47-1988\ </math> in bins of width <math>l=30</math> (with the exception of the last bin that is smaller). The table columns are as follows:<br />
# ''ELL'' (integer): mean multipole number of bin<br />
# ''L_MIN'' (integer): lowest multipole of bin<br />
# ''L_MAX'' (integer): highest multipole of bin<br />
# ''D_ELL'' (float): <math>D_\ell</math> as described above<br />
# ''ERR'' (float): the uncertainty<br />
<br />
; 5. TE high-ell, unbinned (TEHILUNB) <br />
: with the high-ell part of the spectrum, unbinned, in 2979 bins covering <math>\langle l \rangle = 30-1996\ </math>. The table columns are as follows:<br />
# ''ELL'' (integer): multipole <br />
# ''D_ELL'' (float): <math>D_\ell</math> as described above<br />
# ''ERR'' (float): the uncertainty<br />
<br />
; 6. EE high-ell, binned (EELOLBIN) <br />
: with the high-ell part of the spectrum, binned into 83 bins covering <math>\langle l \rangle = 47-1988\ </math> in bins of width <math>l=30</math> (with the exception of the last bin that is smaller). The table columns are as follows:<br />
# ''ELL'' (integer): mean multipole number of bin<br />
# ''L_MIN'' (integer): lowest multipole of bin<br />
# ''L_MAX'' (integer): highest multipole of bin<br />
# ''D_ELL'' (float): <math>D_\ell</math> as described above<br />
# ''ERR'' (float): the uncertainty<br />
<br />
; 7. EE high-ell, unbinned (EEHILUNB) <br />
: with the high-ell part of the spectrum, unbinned, in 2979 bins covering <math>\langle l \rangle = 30-1996\ </math>. The table columns are as follows:<br />
# ''ELL'' (integer): multipole <br />
# ''D_ELL'' (float): <math>D_\ell</math> as described above<br />
# ''ERR'' (float): the uncertainty<br />
<br />
<br />
The spectra give <math>D_\ell = \ell(\ell+1)C_\ell / 2\pi </math> in units of <math>\mu\, K^2</math>. The covariance matrices of the spectra will be released in a second moment.<br />
<!-- <br />
<br />
The CMB spectrum is also given in a simple text comma-separated file:<br />
* ''{{PLASingleFile | fileType=cosmo | name=COM_PowerSpect_CMB_R1.10.txt |link=COM_PowerSpect_CMB_R1.10.txt}}''<br />
<br />
--><br />
<br />
==Likelihood==<br />
The likelihood code will released in March-April 2015 with an accompanying paper and an Explanatory Supplement update. <br />
<!-- <br />
===Likelihood===<br />
<span style="color:red"> ALL OF THE FOLLOWING IN THE LIKELIHOOD SECTION IS OLD. </span><br />
The likelihood code (and the data that comes with it) used to compute the likelihood of a model that predicts the CMB power spectra, lensing power spectrum, together with some foreground and some instrumental parameters. The data files are built primarily from the Planck mission results, but include also some results from the WMAP-9 data release. The data files are written in a specific format that can only be read by the code. The code consists in a c/f90 library, along with some optional tools in python. The code is used to read the data files, and given model power spectra and nuisance parameters it computes the log likelihood of that model. <br />
<br />
Detailed description of the installation and usage of the likelihood code and data is provided in the package. The package includes five data files: four for the CMB likelihoods and one for the lensing likelihood. All of the likelihoods delivered are described in detail in the {{PlanckPapers|planck2013-p08|1|Power spectrum & Likelihood Paper}} (for the CMB based likelihood) and in the {{PlanckPapers|planck2013-p12|1|Lensing Paper}} (for the lensing likelihood) .<br />
<br />
The CMB full likelihood has been divided into four parts to allow using selectively different ranges of multipoles. It also reflects the fact that the mathematical approximations used for those different parts are very different, as is the underlying data. In detail, we distribute<br />
* one low-<math>\ell</math> temperature only likelihood (commander), <br />
* one low-<math>\ell</math> temperature and polarisation likelihood (lowlike), and <br />
* one higl-<math>\ell</math> likelihood CAMspec. <br />
<br />
The ''Commander'' likelihood covers the multipoles 2 to 49. It uses a semi-analytic method to sample the low-<math>\ell</math> temperature likelihood on an intermediate product of one of the component separated maps. The samples are used along with an analytical approximation of the likelihood posterior to perform the likelihood computation in the code. See {{PlanckPapers|planck2013-p08}} section 8.1 for more details.<br />
<br />
The ''lowlike'' likelihood covers the multipoles 2 to 32 for temperature and polarization data. Since Planck is not releasing polarisation data at this time, the polarization map from WMAP9 is used instead. A temperature map is needed to perform the computation nevertheless, and we use here the same commander map. The likelihood is computed using a map-based approximation at low resolution and a master one at intermediate resolution, as in WMAP. The likelihood code actually calls a very slightly modified version of the WMAP9 code. This piece of the likelihood essentially provides a prior on the optical depth and has almost no other impact on cosmological parameter estimation. As such it could be replaced by a simple prior, and a user can decide to do so, which is one of the motivation to leave the three pieces of the CMB likelihood as different data packages; see {{PlanckPapers|planck2013-p08}} section 8.3 for more details. Note that the version of the WMAP code used here (code version v1.0) does not perform any test on the positive definiteness of the TT, TE, EE covariance matrices, and will return a null log likelihood in the unphysical cases where the absolute value of TE is too large. This will be corrected in a later version.<br />
<br />
The ''CAMspec'' likelihood covers the multipoles 50 to 2500 for temperature only. The likelihood is computed using a quadratic approximation, including mode to mode correlations that have been precomputed on a fiducial model. The likelihood uses data from the 100, 143 and 217 GHz channels. To do so it models the foreground at each frequency using the model described in the likelihood paper. Uncertainties on the relative calibration and on the beam transfer functions are included either as parametric models, or marginalized and integrated in the covariance matrix. Detailed description of the different nuisance parameters is given below. Priors are included in the likelihood on the CIB spectral index, relative calibration factors and beam error eigenmodes. See {{PlanckPapers|planck2013-p08}} section 2.1 for more details.<br />
<br />
The ''act/spt'' likelihood covers the multipoles 1500 to 10000 for temperature. It is described in{{BibCite|dun2013}}{{BibCite|Keis2011}}{{BibCite|Reic2012}}. It uses the code and data that can be retrieved from the [http://lambda.gsfc.nasa.gov/ Lambda archive] for [http://lambda.gsfc.nasa.gov/product/act/act_prod_table.cfm ACT] and [http://lambda.gsfc.nasa.gov/product/spt/spt_prod_table.cfm SPT]. It has been slightly modified to use a thermal and kinetic SZ model that matches the one used in CAMspec. As stated in{{BibCite|dun2013}}, the dust parameters a_ge and a_gs must be explored with the following priors: a_ge = 0.8 ± 0.2 and a_gs = 0.4 ± 0.2. Those priors are not included in the log likelihood computed by the code.<br />
<br />
The ''lensing'' likelihood covers the multipoles 40 to 400 using the result of the [[Specially_processed_maps | lensing reconstruction]]. It uses a quadratic approximation for the likelihood, with a covariance matrix including the marginalized contribution of the beam transfer function uncertainties, the diffuse point source correction uncertainties and the cosmological model uncertainty affecting the first order non-gaussian bias (N1). The correlation between temperature and lensing is not taken into account. Cosmological uncertainty effects on the normalization are dealt with using a first order renormalization procedure. This means that the code will need both the TT and $\phi\phi$ power spectrum up to <math>\ell</math> = 2048 to correctly perform the integrals needed for the renormalization. Nevertheless, the code will only produce an estimate based on the data between <math>\ell</math> = 40 to 400. See {{PlanckPapers|planck2013-p12}} section 6.1 for more details.<br />
</span><br />
<span style="color:red">OUTSTANDING: description of likelihood masks </span><br />
==Production process==<br />
<br />
===Likelihood===<br />
<span style="color:red"> ALL OF THE FOLLOWING IN THE LIKELIHOOD SECTION IS OLD. </span><br />
The code is based on some basic routines from the libpmc library in the [http://arxiv.org/abs/1101.0950 cosmoPMC] code. It also uses some code from the [http://lambda.gsfc.nasa.gov/product/map/dr5/likelihood_get.cfm WMAP9 likelihood] for the lowlike likelihood and{{BibCite|dun2013}}{{BibCite|Keis2011}}{{BibCite|Reic2012}} for the act/spt one. The rest of the code has been specifically written for the Planck data. Each likelihood file has been processed using a different and dedicated pipeline as described in the likelihood paper {{PlanckPapers|planck2013-p08}} (section 2 and 8) and in the lensing paper {{PlanckPapers|planck2013-p12}} (section 6.1). We refer the reader to those papers for full details. The data are then encapsulated into the specific file format.<br />
<br />
Each dataset comes with its own self check. Whenever the code is used to read a data file, a computation will be done against an included test spectrum/nuisance parameter, and the log-likelihood will be displayed along with the expected result. Difference of the order of 10<math>^{-6}</math> or less are expected depending of the architecture.<br />
<br />
==Inputs==<br />
<br />
===Likelihood===<br />
<br />
; ''commander'' :<br />
* all Planck channels maps<br />
* compact source catalogs<br />
* common masks<br />
* beam transfer functions for all channels<br />
<br />
; ''lowlike'' :<br />
* WMAP9 likelihood data<br />
* Low-<math>\ell</math> Commander map<br />
<br />
; ''CAMspec'' :<br />
* 100, 143 and 217 GHz detector and detsets maps<br />
* 857GHz channel map<br />
* compact source catalog<br />
* common masks (0,1 & 3)<br />
* beam transfer function and error eigenmodes and covariance for 100, 143 and 217 GHz detectors & detsets<br />
* theoretical templates for the tSZ and kSZ contributions<br />
* color corrections for the CIB emission for the 143 and 217GHz detectors and detsets<br />
* fiducial CMB model (bootstrapped from WMAP7 best fit spectrum) estimated noise contribution from the half-ring maps for 100, 143 and 217 GHz<br />
<br />
; ''lensing'' :<br />
* the lensing map<br />
* beam error eigenmodes and covariance for the 143 and 217GHz channel maps<br />
* fiducial CMB model (from Planck cosmological parameter best fit)<br />
<br />
; ''act/spt'' :<br />
* data and code from [http://lambda.gsfc.nasa.gov/product/act/act_fulllikelihood_get.cfm here]<br />
* the tSZ andkSZ template are changed to match those of CAMspec<br />
<br />
== File names and Meta data ==<br />
<br />
===Likelihood===<br />
<span style="color:red"> ALL OF THE FOLLOWING IN THE LIKELIHOOD SECTION IS OLD. </span><br />
<br />
'''Likelihood source code'''<br />
<br />
The source code is in the file<br />
: {{PLASingleFile |fileType=cosmo|name=COM_Code_Likelihood-v1.0_R1.10.tar.gz|link=COM_Code_Likelihood-v1.0_R1.10.tar.gz}} (C, f90 and python likelihood library and tools)<br />
<br />
'''Likelihood data packages'''<br />
<br />
The {{PLALikelihood|type=Data|link=data packages}} are<br />
: ''{{PLASingleFile | fileType=cosmo | name=COM_Data_Likelihood-commander_R1.10.tar.gz | link=COM_Data_Likelihood-commander_R1.10.tar.gz}}'' (low-ell TT likelihood)<br />
: ''{{PLASingleFile | fileType=cosmo | name=COM_Data_Likelihood-lowlike_R1.10.tar.gz | link=COM_Data_Likelihood-lowlike_R1.10.tar.gz}}'' (low-ell TE,EE,BB likelihood)<br />
: ''{{PLASingleFile | fileType=cosmo | name=COM_Data_Likelihood-CAMspec_R1.10.tar.gz | link=COM_Data_Likelihood-CAMspec_R1.10.tar.gz}}'' (high-ell TT likelihood)<br />
: ''{{PLASingleFile | fileType=cosmo | name=COM_Data_Likelihood-actspt_R1.10.tar | link=COM_Data_Likelihood-actspt_R1.10.tar.gz}}'' (high-ell TT likelihood)<br />
: ''{{PLASingleFile | fileType=cosmo | name=COM_Data_Likelihood-lensing_R1.10.tar.gz | link=COM_Data_Likelihood-lensing_R1.10.tar.gz}}'' (lensing likelihood)<br />
<br />
Untar and unzip all files to recover the code and likelihood data. Each package comes with a README file; follow the instructions inclosed to<br />
build the code and use it. To compute the CMB likelihood one has to sum the log likelihood of each of the commander_v4.1_lm49.clik, lowlike_v222.clik and CAMspec_v6.2TN_2013_02_26.clik, actspt_2013_01.clik. To compute the CMB+lensing likelihood, one has to sum the log likelihood of all 5 files.<br />
<br />
The CMB and lensing likelihood format are different. The CMB files have the termination .clik, the lensing one .clik_lensing. The lensing data being simpler (due to the less detailled modeling permitted by the lower signal-noise), the file is a simple ascii file containing all the data along with comments describing it, and linking the different quantities to the lensing paper. The CMB file format is more complex and must accommodate different forms of data (maps, power spectrum, distribution samples, covariance matrices...). It consists of a tree structure containing the data. At each level of the tree structure a given directory can contain array data (in the form of FITS files or ascii files for strings) and scalar data (joined in a single ascii file "_mdb"). Those files are not user modifiable and do not contain interesting meta data for the user. Tools to manipulate those files are included in the code package as optional python tools. They are documented in the code package.<br />
<br />
'''Likelihood masks'''<br />
<br />
The masks used in the Likelihood paper {{PlanckPapers|planck2013-p08}} are found in<br />
{{PLASingleFile|fileType=map|name=COM_Mask_Likelihood_2048_R1.10.fits|link=COM_Mask_Likelihood_2048_R1.10.fits}}<br />
<br />
which contains ten masks which are written into a single ''BINTABLE'' extension of 10 columns by 50331648 rows (the number of Healpix pixels in an Nside = 2048 map). The structure is as follows, where the column names are the names of the masks: <br />
<br />
{| border="1" cellpadding="3" cellspacing="0" align="center" style="text-align:left" width=800px<br />
|+ '''Likelihodd masks file data structure'''<br />
|- bgcolor="ffdead" <br />
!colspan="4" | 1. EXTNAME = 'MSK-LIKE' : Data columns<br />
|- bgcolor="ffdead" <br />
! Column Name || Data Type || Units || Description<br />
|-<br />
|CL31 || Real*4 || none || mask<br />
|-<br />
|CL39 || Real*4 || none || mask<br />
|-<br />
|CL49 || Real*4 || none || mask<br />
|-<br />
|G22 || Real*4 || none || mask <br />
|-<br />
|G35 || Real*4 || none || mask<br />
|-<br />
|G45 || Real*4 || none || mask<br />
|-<br />
|G56 || Real*4 || none || mask<br />
|-<br />
|G65 || Real*4 || none || mask<br />
|-<br />
|PS96 || Real*4 || none || mask<br />
|-<br />
|PSA82 || Real*4 || none || mask<br />
|-<br />
|- bgcolor="ffdead" <br />
! Keyword || Data Type || Value || Description<br />
|-<br />
|PIXTYPE || string || HEALPIX ||<br />
|-<br />
|COORDSYS || string || GALACTIC ||Coordinate system <br />
|-<br />
|ORDERING || string || NESTED || Healpix ordering<br />
|-<br />
|NSIDE || Int || 2048 || Healpix Nside <br />
|-<br />
|FIRSTPIX || Int*4 || 0 || First pixel number<br />
|-<br />
|LASTPIX || Int*4 || 50331647 || Last pixel number, for LFI and HFI, respectively<br />
<br />
|}<br />
--><br />
<br />
== References ==<br />
<References /><br />
<br />
<br />
<br />
[[Category:Mission products|008]]</div>
Xdupac
https://wiki.cosmos.esa.int/planckpla2015/index.php?title=CMB_spectrum_%26_Likelihood_Code&diff=11443
CMB spectrum & Likelihood Code
2015-02-09T09:43:00Z
<p>Xdupac: /* TT */</p>
<hr />
<div>{{DISPLAYTITLE:2015 CMB spectra and likelihood code}}<br />
<br />
==2015 CMB spectra==<br />
<br />
<br />
===General description===<br />
====TT====<br />
The Planck best-fit CMB temperature power spectrum, shown in the figure below, covers the wide range of multipoles <math> \ell </math> = 2-2508. Over the multipole range <math> \ell </math> = 2–29, the power spectrum is derived from the ''Commander'': component separation algorithm applied to the combination of Planck 2015 temperature data between 30 and 857 GHz, the 9-year WMAP sky maps, and the 408 MHz Haslam et al. (1982) survey, including 93% of the sky {{PlanckPapers|planck2014-a12}} . The asymmetric error bars associated to this spectrum are the 68% confidence limits and include the uncertainties due to foreground subtraction.<br />
<br />
For multipoles equal or greater than <math>\ell=30</math>, instead, the spectrum is derived from the ''Plik'' likelihood {{PlanckPapers|planck2014-a13}} by optimally combining the spectra in the frequency range 100-217 GHz, and correcting them for unresolved foregrounds using the best-fit foreground solution from a Planck TT+lowP <math>\Lambda</math>CDM run. Associated 1-sigma errors include beam uncertainties. Both ''Commander'' and ''Plik'' are described in more details in the sections below.<br />
<br />
[[File: A15_TT.png|thumb|center|700px|'''The Planck 2015 TT power spectrum. Logarithmic x-scale up to <math>\ell = 30 </math> , linear at higher <math>\ell</math>. The red line is the Planck best-fit primordial power spectrum (cf Planck TT+lowP in Table 3 of Planck-2015-A15[3]). Residuals with respect to this model are shown in the lower panel. The error bars show <math>\pm 1\sigma</math> uncertainties.''']]<br />
<br />
====TE and EE====<br />
The Planck best-fit CMB polarization and temperature-polarization cross-correlation power spectra, shown in the figure below, cover the multipole range <math> \ell </math> = 30-1996. The data points relative to the multipole range <math> \ell </math> = 2-29 will be released in a second moment.<br />
Analogously to the TT case, the <math> \ell\ge 30 </math> spectrum is derived from the ''Plik'' likelihood {{PlanckPapers|planck2014-a13}} by optimally combining the spectra in the frequency range 100-217 GHz, and correcting them for unresolved foregrounds using the best-fit foreground solution from a Planck TT,TE,EE+lowP <math>\Lambda</math>CDM run. <br />
<br />
{|style="margin: 0 auto;"<br />
|[[File: A15_EE.png|thumb|center|500px|'''2015 CMB EE spectrum. The red line is the Planck best-fit primordial power spectrum (cf Planck TT+lowP in Table 3 of {{PlanckPapers|planck2014-a15}}). The blue shaded area shows the uncertainties due to cosmic variance alone.''']]<br />
|[[File: A15_TE.png|thumb|center|500px|'''2015 CMB TE spectrum. The red line is the Planck best-fit primordial power spectrum (cf Planck TT+lowP in Table 3 of {{PlanckPapers|planck2014-a15}}). The blue shaded area shows the uncertainties due to cosmic variance alone.''']]<br />
|}<br />
<br />
===Production process===<br />
The <math>\ell</math> < 30 part of the Planck TT power spectrum is derived from the Commander approach, which implements Bayesian component separation in pixel space, fitting a parametric model to the data by sampling the posterior distribution for the model parameters {{PlanckPapers|planck2014-a12}}. The power spectrum at any multipole <math>\ell</math> is given as the maximum probability point for the posterior <math>C_\ell</math> distribution, marginalized over the other multipoles, and the error bars are 68% confidence level; see {{PlanckPapers|planck2014-a12}}. <br />
<br />
The <math>\ell \ge 30</math> part of the TT, TE and EE power spectra have been derived by the Plik likelihood, a code that implements a pseudo-Cl based technique, extensively described in Sec. 2 and the Appendix of {{PlanckPapers|planck2013-p08}} and {{PlanckPapers|planck2014-a13}}. Frequency spectra are computed as cross-spectra between half-mission maps. Mask and multipole range choices for each frequency spectrum are summarized in Section 3.3 of {{PlanckPapers|planck2014-a15}} and in {{PlanckPapers|planck2014-a13}}. The final power spectrum is an optimal combination of the 100, 143, 143x217 and 217 GHz spectra, corrected for the best-fit unresolved foregrounds and inter-frequency calibration factors, as derived from the full likelihood analysis (for TT we use the best-fit solutions for the nuisance parameters from the Planck+TT+lowP data combination, while for TE and EE we use the best fit from Planck+TT+lowP, cf Table 3 of {{PlanckPapers|planck2014-a15}}). A thorough description of the models of unresolved foregrounds is given in {{PlanckPapers|planck2014-a13}}. The spectrum covariance matrix accounts for cosmic variance and noise contributions, together with beam uncertainties. The <math>\ell \ge 30</math> CMB TT spectrum and associated covariance matrix are available in two formats:<br />
#Unbinned. TT: 2479 bandpowers (<math>\ell=30-2508</math>); TE or EE: 1697 bandpowers (<math>\ell=30-1996</math>).<br />
#Binned, in bins of <math> \Delta\ell=30 </math>. TT: 83 bandpowers. TE or EE: 66 bandpowers. We bin the <math> C_\ell </math> power spectrum with a weight proportional to <math> \ell (\ell+1) </math>, so that the <math> C_{\ell_b} </math> binned bandpower centered in <math> \ell_b </math> is: <math> \\ C_{\ell_b}=\Sigma_{\ell \in b} w_{\ell_b\ell} C_\ell \quad \text{with} \quad w_{\ell_b\ell}=\frac{\ell (\ell+1)}{\Sigma_{\ell \in b} \ell (\ell+1)}. \\</math> Equivalently, using the matrix formalism, we can construct the binning matrix B as: <math>\\ B_{\ell_b \ell}=w_{\ell_b\ell} \\ </math> where B is a <math> n_b\times n_\ell</math> matrix, with <math>n_b=83</math> the number of bins and <math>n_\ell=2479</math> the number of unbinned multipoles. Thus: <math> \\ \vec{C}_\mathrm{binned}=B \, \vec{C} \\ \mathrm{cov_\mathrm{binned}}= B\, \mathrm{cov}\, B^T \\ \ell_b=B\, \ell \\ </math> Here, <math> \vec{C}_{binned}\, (\vec{C}) </math> is the vector containing all the binned (unbinned) <math>C_\ell</math> bandpowers, <math>\mathrm{cov} </math> is the covariance matrix and <math>\ell_b</math> is the weighted average multipole in each bin. Note that following this definition, <math>\ell_b</math> can be a non-integer. The binned <math>D_{\ell_B}</math> power spectrum is then calculated as: <math> \\ D_{\ell_b}=\frac{\ell_b (\ell_b+1)}{2\pi} C_{\ell_b} </math>.<br />
<br />
===Inputs===<br />
<br />
; Low-l spectrum (<math>\ell < 30</math>):<br />
* Planck 30 and 44 GHz frequency maps<br />
* Planck 70 to 857 GHz detector and detector set maps<br />
* 9-year WMAP temperature sky maps between 23 and 94 GHz<br />
* 408 MHz survey by Haslam et al. (1982) <br />
* Commander <math>\chi^2</math> based LM93 confidence mask {{PlanckPapers|planck2014-a12}}<br />
<br />
; High-l spectrum (<math>30 \le \ell \le 2508</math>): <br />
<br />
* 100, 143, 143x217 and 217 GHz spectra and their covariance matrix (Sec. 3.3 {{PlanckPapers|planck2014-a15}})<br />
* best-fit foreground templates and inter-frequency calibration factors (Table 3 of {{PlanckPapers|planck2014-a15}})<br />
* Beam transfer function uncertainties {{PlanckPapers|planck2014-a08}}<br />
=== File names and Meta data ===<br />
<br />
The CMB spectrum and its covariance matrix are distributed in a single FITS file named <br />
<!--- * ''{{PLASingleFile | fileType=cosmo | name=COM_PowerSpect_CMB_R2.00.fits | link=COM_PowerSpect_CMB_R1.10.fits}}'' ---><br />
* ''COM_PowerSpect_CMB_R2.nn.fits''<br />
which contains 7 ''BINTABLE'' extensions<br />
<br />
; 1. TT low-ell, unbinned (TTLOLUNB)<br />
: with the low ell part of the spectrum, not binned, and for l=2-29. The table columns are<br />
# ''ELL'' (integer): multipole number<br />
# ''D_ELL'' (float): <math>D_ell</math> as described above<br />
# ''ERRUP'' (float): the upward uncertainty<br />
# ''ERRDOWN'' (float): the downward uncertainty<br />
<br />
; 2. TT high-ell, binned (TTHILBIN)<br />
: with the high-ell part of the spectrum, binned into 83 bins covering <math>\langle l \rangle = 47-2499\ </math> in bins of width <math>l=30</math> (with the exception of the last bin that is smaller). The table columns are as follows:<br />
# ''ELL'' (integer): mean multipole number of bin<br />
# ''L_MIN'' (integer): lowest multipole of bin<br />
# ''L_MAX'' (integer): highest multipole of bin<br />
# ''D_ELL'' (float): <math>D_\ell</math> as described above<br />
# ''ERR'' (float): the uncertainty<br />
<br />
; 3. TT high-ell unbinned (TTHILUNB) <br />
: with the high-ell part of the spectrum, unbinned, in 2979 bins covering <math>\langle l \rangle = 30-2508\ </math>. The table columns are as follows:<br />
# ''ELL'' (integer): multipole <br />
# ''D_ELL'' (float): <math>D_\ell</math> as described above<br />
# ''ERR'' (float): the uncertainty<br />
<br />
; 4. TE high-ell, binned (TEHILBIN) <br />
: with the high-ell part of the spectrum, binned into 83 bins covering <math>\langle l \rangle = 47-1988\ </math> in bins of width <math>l=30</math> (with the exception of the last bin that is smaller). The table columns are as follows:<br />
# ''ELL'' (integer): mean multipole number of bin<br />
# ''L_MIN'' (integer): lowest multipole of bin<br />
# ''L_MAX'' (integer): highest multipole of bin<br />
# ''D_ELL'' (float): <math>D_\ell</math> as described above<br />
# ''ERR'' (float): the uncertainty<br />
<br />
; 5. TE high-ell, unbinned (TEHILUNB) <br />
: with the high-ell part of the spectrum, unbinned, in 2979 bins covering <math>\langle l \rangle = 30-1996\ </math>. The table columns are as follows:<br />
# ''ELL'' (integer): multipole <br />
# ''D_ELL'' (float): <math>D_\ell</math> as described above<br />
# ''ERR'' (float): the uncertainty<br />
<br />
; 6. EE high-ell, binned (EELOLBIN) <br />
: with the high-ell part of the spectrum, binned into 83 bins covering <math>\langle l \rangle = 47-1988\ </math> in bins of width <math>l=30</math> (with the exception of the last bin that is smaller). The table columns are as follows:<br />
# ''ELL'' (integer): mean multipole number of bin<br />
# ''L_MIN'' (integer): lowest multipole of bin<br />
# ''L_MAX'' (integer): highest multipole of bin<br />
# ''D_ELL'' (float): <math>D_\ell</math> as described above<br />
# ''ERR'' (float): the uncertainty<br />
<br />
; 7. EE high-ell, unbinned (EEHILUNB) <br />
: with the high-ell part of the spectrum, unbinned, in 2979 bins covering <math>\langle l \rangle = 30-1996\ </math>. The table columns are as follows:<br />
# ''ELL'' (integer): multipole <br />
# ''D_ELL'' (float): <math>D_\ell</math> as described above<br />
# ''ERR'' (float): the uncertainty<br />
<br />
<br />
The spectra give <math>D_\ell = \ell(\ell+1)C_\ell / 2\pi </math> in units of <math>\mu\, K^2</math>. The covariance matrices of the spectra will be released in a second moment.<br />
<!-- <br />
<br />
The CMB spectrum is also given in a simple text comma-separated file:<br />
* ''{{PLASingleFile | fileType=cosmo | name=COM_PowerSpect_CMB_R1.10.txt |link=COM_PowerSpect_CMB_R1.10.txt}}''<br />
<br />
--><br />
<br />
==Likelihood==<br />
The likelihood code will released in March-April 2015 with an accompanying paper and an Explanatory Supplement update. <br />
<!-- <br />
===Likelihood===<br />
<span style="color:red"> ALL OF THE FOLLOWING IN THE LIKELIHOOD SECTION IS OLD. </span><br />
The likelihood code (and the data that comes with it) used to compute the likelihood of a model that predicts the CMB power spectra, lensing power spectrum, together with some foreground and some instrumental parameters. The data files are built primarily from the Planck mission results, but include also some results from the WMAP-9 data release. The data files are written in a specific format that can only be read by the code. The code consists in a c/f90 library, along with some optional tools in python. The code is used to read the data files, and given model power spectra and nuisance parameters it computes the log likelihood of that model. <br />
<br />
Detailed description of the installation and usage of the likelihood code and data is provided in the package. The package includes five data files: four for the CMB likelihoods and one for the lensing likelihood. All of the likelihoods delivered are described in detail in the {{PlanckPapers|planck2013-p08|1|Power spectrum & Likelihood Paper}} (for the CMB based likelihood) and in the {{PlanckPapers|planck2013-p12|1|Lensing Paper}} (for the lensing likelihood) .<br />
<br />
The CMB full likelihood has been divided into four parts to allow using selectively different ranges of multipoles. It also reflects the fact that the mathematical approximations used for those different parts are very different, as is the underlying data. In detail, we distribute<br />
* one low-<math>\ell</math> temperature only likelihood (commander), <br />
* one low-<math>\ell</math> temperature and polarisation likelihood (lowlike), and <br />
* one higl-<math>\ell</math> likelihood CAMspec. <br />
<br />
The ''Commander'' likelihood covers the multipoles 2 to 49. It uses a semi-analytic method to sample the low-<math>\ell</math> temperature likelihood on an intermediate product of one of the component separated maps. The samples are used along with an analytical approximation of the likelihood posterior to perform the likelihood computation in the code. See {{PlanckPapers|planck2013-p08}} section 8.1 for more details.<br />
<br />
The ''lowlike'' likelihood covers the multipoles 2 to 32 for temperature and polarization data. Since Planck is not releasing polarisation data at this time, the polarization map from WMAP9 is used instead. A temperature map is needed to perform the computation nevertheless, and we use here the same commander map. The likelihood is computed using a map-based approximation at low resolution and a master one at intermediate resolution, as in WMAP. The likelihood code actually calls a very slightly modified version of the WMAP9 code. This piece of the likelihood essentially provides a prior on the optical depth and has almost no other impact on cosmological parameter estimation. As such it could be replaced by a simple prior, and a user can decide to do so, which is one of the motivation to leave the three pieces of the CMB likelihood as different data packages; see {{PlanckPapers|planck2013-p08}} section 8.3 for more details. Note that the version of the WMAP code used here (code version v1.0) does not perform any test on the positive definiteness of the TT, TE, EE covariance matrices, and will return a null log likelihood in the unphysical cases where the absolute value of TE is too large. This will be corrected in a later version.<br />
<br />
The ''CAMspec'' likelihood covers the multipoles 50 to 2500 for temperature only. The likelihood is computed using a quadratic approximation, including mode to mode correlations that have been precomputed on a fiducial model. The likelihood uses data from the 100, 143 and 217 GHz channels. To do so it models the foreground at each frequency using the model described in the likelihood paper. Uncertainties on the relative calibration and on the beam transfer functions are included either as parametric models, or marginalized and integrated in the covariance matrix. Detailed description of the different nuisance parameters is given below. Priors are included in the likelihood on the CIB spectral index, relative calibration factors and beam error eigenmodes. See {{PlanckPapers|planck2013-p08}} section 2.1 for more details.<br />
<br />
The ''act/spt'' likelihood covers the multipoles 1500 to 10000 for temperature. It is described in{{BibCite|dun2013}}{{BibCite|Keis2011}}{{BibCite|Reic2012}}. It uses the code and data that can be retrieved from the [http://lambda.gsfc.nasa.gov/ Lambda archive] for [http://lambda.gsfc.nasa.gov/product/act/act_prod_table.cfm ACT] and [http://lambda.gsfc.nasa.gov/product/spt/spt_prod_table.cfm SPT]. It has been slightly modified to use a thermal and kinetic SZ model that matches the one used in CAMspec. As stated in{{BibCite|dun2013}}, the dust parameters a_ge and a_gs must be explored with the following priors: a_ge = 0.8 ± 0.2 and a_gs = 0.4 ± 0.2. Those priors are not included in the log likelihood computed by the code.<br />
<br />
The ''lensing'' likelihood covers the multipoles 40 to 400 using the result of the [[Specially_processed_maps | lensing reconstruction]]. It uses a quadratic approximation for the likelihood, with a covariance matrix including the marginalized contribution of the beam transfer function uncertainties, the diffuse point source correction uncertainties and the cosmological model uncertainty affecting the first order non-gaussian bias (N1). The correlation between temperature and lensing is not taken into account. Cosmological uncertainty effects on the normalization are dealt with using a first order renormalization procedure. This means that the code will need both the TT and $\phi\phi$ power spectrum up to <math>\ell</math> = 2048 to correctly perform the integrals needed for the renormalization. Nevertheless, the code will only produce an estimate based on the data between <math>\ell</math> = 40 to 400. See {{PlanckPapers|planck2013-p12}} section 6.1 for more details.<br />
</span><br />
<span style="color:red">OUTSTANDING: description of likelihood masks </span><br />
==Production process==<br />
<br />
===Likelihood===<br />
<span style="color:red"> ALL OF THE FOLLOWING IN THE LIKELIHOOD SECTION IS OLD. </span><br />
The code is based on some basic routines from the libpmc library in the [http://arxiv.org/abs/1101.0950 cosmoPMC] code. It also uses some code from the [http://lambda.gsfc.nasa.gov/product/map/dr5/likelihood_get.cfm WMAP9 likelihood] for the lowlike likelihood and{{BibCite|dun2013}}{{BibCite|Keis2011}}{{BibCite|Reic2012}} for the act/spt one. The rest of the code has been specifically written for the Planck data. Each likelihood file has been processed using a different and dedicated pipeline as described in the likelihood paper {{PlanckPapers|planck2013-p08}} (section 2 and 8) and in the lensing paper {{PlanckPapers|planck2013-p12}} (section 6.1). We refer the reader to those papers for full details. The data are then encapsulated into the specific file format.<br />
<br />
Each dataset comes with its own self check. Whenever the code is used to read a data file, a computation will be done against an included test spectrum/nuisance parameter, and the log-likelihood will be displayed along with the expected result. Difference of the order of 10<math>^{-6}</math> or less are expected depending of the architecture.<br />
<br />
==Inputs==<br />
<br />
===Likelihood===<br />
<br />
; ''commander'' :<br />
* all Planck channels maps<br />
* compact source catalogs<br />
* common masks<br />
* beam transfer functions for all channels<br />
<br />
; ''lowlike'' :<br />
* WMAP9 likelihood data<br />
* Low-<math>\ell</math> Commander map<br />
<br />
; ''CAMspec'' :<br />
* 100, 143 and 217 GHz detector and detsets maps<br />
* 857GHz channel map<br />
* compact source catalog<br />
* common masks (0,1 & 3)<br />
* beam transfer function and error eigenmodes and covariance for 100, 143 and 217 GHz detectors & detsets<br />
* theoretical templates for the tSZ and kSZ contributions<br />
* color corrections for the CIB emission for the 143 and 217GHz detectors and detsets<br />
* fiducial CMB model (bootstrapped from WMAP7 best fit spectrum) estimated noise contribution from the half-ring maps for 100, 143 and 217 GHz<br />
<br />
; ''lensing'' :<br />
* the lensing map<br />
* beam error eigenmodes and covariance for the 143 and 217GHz channel maps<br />
* fiducial CMB model (from Planck cosmological parameter best fit)<br />
<br />
; ''act/spt'' :<br />
* data and code from [http://lambda.gsfc.nasa.gov/product/act/act_fulllikelihood_get.cfm here]<br />
* the tSZ andkSZ template are changed to match those of CAMspec<br />
<br />
== File names and Meta data ==<br />
<br />
===Likelihood===<br />
<span style="color:red"> ALL OF THE FOLLOWING IN THE LIKELIHOOD SECTION IS OLD. </span><br />
<br />
'''Likelihood source code'''<br />
<br />
The source code is in the file<br />
: {{PLASingleFile |fileType=cosmo|name=COM_Code_Likelihood-v1.0_R1.10.tar.gz|link=COM_Code_Likelihood-v1.0_R1.10.tar.gz}} (C, f90 and python likelihood library and tools)<br />
<br />
'''Likelihood data packages'''<br />
<br />
The {{PLALikelihood|type=Data|link=data packages}} are<br />
: ''{{PLASingleFile | fileType=cosmo | name=COM_Data_Likelihood-commander_R1.10.tar.gz | link=COM_Data_Likelihood-commander_R1.10.tar.gz}}'' (low-ell TT likelihood)<br />
: ''{{PLASingleFile | fileType=cosmo | name=COM_Data_Likelihood-lowlike_R1.10.tar.gz | link=COM_Data_Likelihood-lowlike_R1.10.tar.gz}}'' (low-ell TE,EE,BB likelihood)<br />
: ''{{PLASingleFile | fileType=cosmo | name=COM_Data_Likelihood-CAMspec_R1.10.tar.gz | link=COM_Data_Likelihood-CAMspec_R1.10.tar.gz}}'' (high-ell TT likelihood)<br />
: ''{{PLASingleFile | fileType=cosmo | name=COM_Data_Likelihood-actspt_R1.10.tar | link=COM_Data_Likelihood-actspt_R1.10.tar.gz}}'' (high-ell TT likelihood)<br />
: ''{{PLASingleFile | fileType=cosmo | name=COM_Data_Likelihood-lensing_R1.10.tar.gz | link=COM_Data_Likelihood-lensing_R1.10.tar.gz}}'' (lensing likelihood)<br />
<br />
Untar and unzip all files to recover the code and likelihood data. Each package comes with a README file; follow the instructions inclosed to<br />
build the code and use it. To compute the CMB likelihood one has to sum the log likelihood of each of the commander_v4.1_lm49.clik, lowlike_v222.clik and CAMspec_v6.2TN_2013_02_26.clik, actspt_2013_01.clik. To compute the CMB+lensing likelihood, one has to sum the log likelihood of all 5 files.<br />
<br />
The CMB and lensing likelihood format are different. The CMB files have the termination .clik, the lensing one .clik_lensing. The lensing data being simpler (due to the less detailled modeling permitted by the lower signal-noise), the file is a simple ascii file containing all the data along with comments describing it, and linking the different quantities to the lensing paper. The CMB file format is more complex and must accommodate different forms of data (maps, power spectrum, distribution samples, covariance matrices...). It consists of a tree structure containing the data. At each level of the tree structure a given directory can contain array data (in the form of FITS files or ascii files for strings) and scalar data (joined in a single ascii file "_mdb"). Those files are not user modifiable and do not contain interesting meta data for the user. Tools to manipulate those files are included in the code package as optional python tools. They are documented in the code package.<br />
<br />
'''Likelihood masks'''<br />
<br />
The masks used in the Likelihood paper {{PlanckPapers|planck2013-p08}} are found in<br />
{{PLASingleFile|fileType=map|name=COM_Mask_Likelihood_2048_R1.10.fits|link=COM_Mask_Likelihood_2048_R1.10.fits}}<br />
<br />
which contains ten masks which are written into a single ''BINTABLE'' extension of 10 columns by 50331648 rows (the number of Healpix pixels in an Nside = 2048 map). The structure is as follows, where the column names are the names of the masks: <br />
<br />
{| border="1" cellpadding="3" cellspacing="0" align="center" style="text-align:left" width=800px<br />
|+ '''Likelihodd masks file data structure'''<br />
|- bgcolor="ffdead" <br />
!colspan="4" | 1. EXTNAME = 'MSK-LIKE' : Data columns<br />
|- bgcolor="ffdead" <br />
! Column Name || Data Type || Units || Description<br />
|-<br />
|CL31 || Real*4 || none || mask<br />
|-<br />
|CL39 || Real*4 || none || mask<br />
|-<br />
|CL49 || Real*4 || none || mask<br />
|-<br />
|G22 || Real*4 || none || mask <br />
|-<br />
|G35 || Real*4 || none || mask<br />
|-<br />
|G45 || Real*4 || none || mask<br />
|-<br />
|G56 || Real*4 || none || mask<br />
|-<br />
|G65 || Real*4 || none || mask<br />
|-<br />
|PS96 || Real*4 || none || mask<br />
|-<br />
|PSA82 || Real*4 || none || mask<br />
|-<br />
|- bgcolor="ffdead" <br />
! Keyword || Data Type || Value || Description<br />
|-<br />
|PIXTYPE || string || HEALPIX ||<br />
|-<br />
|COORDSYS || string || GALACTIC ||Coordinate system <br />
|-<br />
|ORDERING || string || NESTED || Healpix ordering<br />
|-<br />
|NSIDE || Int || 2048 || Healpix Nside <br />
|-<br />
|FIRSTPIX || Int*4 || 0 || First pixel number<br />
|-<br />
|LASTPIX || Int*4 || 50331647 || Last pixel number, for LFI and HFI, respectively<br />
<br />
|}<br />
--><br />
<br />
== References ==<br />
<References /><br />
<br />
<br />
<br />
[[Category:Mission products|008]]</div>
Xdupac
https://wiki.cosmos.esa.int/planckpla2015/index.php?title=CMB_spectrum_%26_Likelihood_Code&diff=11442
CMB spectrum & Likelihood Code
2015-02-09T09:42:12Z
<p>Xdupac: /* TT */</p>
<hr />
<div>{{DISPLAYTITLE:2015 CMB spectra and likelihood code}}<br />
<br />
==2015 CMB spectra==<br />
<br />
<br />
===General description===<br />
====TT====<br />
The Planck best-fit CMB temperature power spectrum, shown in the figure below, covers the wide range of multipoles <math> \ell </math> = 2-2508. Over the multipole range <math> \ell </math> = 2–29, the power spectrum is derived from the ''Commander'': component separation algorithm applied to the combination of Planck 2015 temperature data between 30 and 857 GHz, the 9-year WMAP sky maps, and the 408 MHz Haslam et al. (1982) survey, including 93% of the sky {{PlanckPapers|planck2014-a12}} . The asymmetric error bars associated to this spectrum are the 68% confidence limits and include the uncertainties due to foreground subtraction.<br />
<br />
For multipoles equal or greater than <math>\ell=30</math>, instead, the spectrum is derived from the ''Plik'' likelihood {{PlanckPapers|planck2014-a13}} by optimally combining the spectra in the frequency range 100-217 GHz, and correcting them for unresolved foregrounds using the best-fit foreground solution from a Planck TT+lowP <math>\Lambda</math>CDM run. Associated 1-sigma errors include beam uncertainties. Both ''Commander'' and ''Plik'' are described in more details in the sections below.<br />
<br />
[[File: A15_TT.png|thumb|center|700px|'''The Planck 2015 TT power spectrum. Logarithmic x-scale up to <math>\ell = 30 </math> , linear at higher <math>\ell. The red line is the Planck best-fit primordial power spectrum (cf Planck TT+lowP in Table 3 of Planck-2015-A15[3]). Residuals with respect to this model are shown in the lower panel. The error bars show <math>\pm 1\sigma</math> uncertainties.''']]<br />
<br />
====TE and EE====<br />
The Planck best-fit CMB polarization and temperature-polarization cross-correlation power spectra, shown in the figure below, cover the multipole range <math> \ell </math> = 30-1996. The data points relative to the multipole range <math> \ell </math> = 2-29 will be released in a second moment.<br />
Analogously to the TT case, the <math> \ell\ge 30 </math> spectrum is derived from the ''Plik'' likelihood {{PlanckPapers|planck2014-a13}} by optimally combining the spectra in the frequency range 100-217 GHz, and correcting them for unresolved foregrounds using the best-fit foreground solution from a Planck TT,TE,EE+lowP <math>\Lambda</math>CDM run. <br />
<br />
{|style="margin: 0 auto;"<br />
|[[File: A15_EE.png|thumb|center|500px|'''2015 CMB EE spectrum. The red line is the Planck best-fit primordial power spectrum (cf Planck TT+lowP in Table 3 of {{PlanckPapers|planck2014-a15}}). The blue shaded area shows the uncertainties due to cosmic variance alone.''']]<br />
|[[File: A15_TE.png|thumb|center|500px|'''2015 CMB TE spectrum. The red line is the Planck best-fit primordial power spectrum (cf Planck TT+lowP in Table 3 of {{PlanckPapers|planck2014-a15}}). The blue shaded area shows the uncertainties due to cosmic variance alone.''']]<br />
|}<br />
<br />
===Production process===<br />
The <math>\ell</math> < 30 part of the Planck TT power spectrum is derived from the Commander approach, which implements Bayesian component separation in pixel space, fitting a parametric model to the data by sampling the posterior distribution for the model parameters {{PlanckPapers|planck2014-a12}}. The power spectrum at any multipole <math>\ell</math> is given as the maximum probability point for the posterior <math>C_\ell</math> distribution, marginalized over the other multipoles, and the error bars are 68% confidence level; see {{PlanckPapers|planck2014-a12}}. <br />
<br />
The <math>\ell \ge 30</math> part of the TT, TE and EE power spectra have been derived by the Plik likelihood, a code that implements a pseudo-Cl based technique, extensively described in Sec. 2 and the Appendix of {{PlanckPapers|planck2013-p08}} and {{PlanckPapers|planck2014-a13}}. Frequency spectra are computed as cross-spectra between half-mission maps. Mask and multipole range choices for each frequency spectrum are summarized in Section 3.3 of {{PlanckPapers|planck2014-a15}} and in {{PlanckPapers|planck2014-a13}}. The final power spectrum is an optimal combination of the 100, 143, 143x217 and 217 GHz spectra, corrected for the best-fit unresolved foregrounds and inter-frequency calibration factors, as derived from the full likelihood analysis (for TT we use the best-fit solutions for the nuisance parameters from the Planck+TT+lowP data combination, while for TE and EE we use the best fit from Planck+TT+lowP, cf Table 3 of {{PlanckPapers|planck2014-a15}}). A thorough description of the models of unresolved foregrounds is given in {{PlanckPapers|planck2014-a13}}. The spectrum covariance matrix accounts for cosmic variance and noise contributions, together with beam uncertainties. The <math>\ell \ge 30</math> CMB TT spectrum and associated covariance matrix are available in two formats:<br />
#Unbinned. TT: 2479 bandpowers (<math>\ell=30-2508</math>); TE or EE: 1697 bandpowers (<math>\ell=30-1996</math>).<br />
#Binned, in bins of <math> \Delta\ell=30 </math>. TT: 83 bandpowers. TE or EE: 66 bandpowers. We bin the <math> C_\ell </math> power spectrum with a weight proportional to <math> \ell (\ell+1) </math>, so that the <math> C_{\ell_b} </math> binned bandpower centered in <math> \ell_b </math> is: <math> \\ C_{\ell_b}=\Sigma_{\ell \in b} w_{\ell_b\ell} C_\ell \quad \text{with} \quad w_{\ell_b\ell}=\frac{\ell (\ell+1)}{\Sigma_{\ell \in b} \ell (\ell+1)}. \\</math> Equivalently, using the matrix formalism, we can construct the binning matrix B as: <math>\\ B_{\ell_b \ell}=w_{\ell_b\ell} \\ </math> where B is a <math> n_b\times n_\ell</math> matrix, with <math>n_b=83</math> the number of bins and <math>n_\ell=2479</math> the number of unbinned multipoles. Thus: <math> \\ \vec{C}_\mathrm{binned}=B \, \vec{C} \\ \mathrm{cov_\mathrm{binned}}= B\, \mathrm{cov}\, B^T \\ \ell_b=B\, \ell \\ </math> Here, <math> \vec{C}_{binned}\, (\vec{C}) </math> is the vector containing all the binned (unbinned) <math>C_\ell</math> bandpowers, <math>\mathrm{cov} </math> is the covariance matrix and <math>\ell_b</math> is the weighted average multipole in each bin. Note that following this definition, <math>\ell_b</math> can be a non-integer. The binned <math>D_{\ell_B}</math> power spectrum is then calculated as: <math> \\ D_{\ell_b}=\frac{\ell_b (\ell_b+1)}{2\pi} C_{\ell_b} </math>.<br />
<br />
===Inputs===<br />
<br />
; Low-l spectrum (<math>\ell < 30</math>):<br />
* Planck 30 and 44 GHz frequency maps<br />
* Planck 70 to 857 GHz detector and detector set maps<br />
* 9-year WMAP temperature sky maps between 23 and 94 GHz<br />
* 408 MHz survey by Haslam et al. (1982) <br />
* Commander <math>\chi^2</math> based LM93 confidence mask {{PlanckPapers|planck2014-a12}}<br />
<br />
; High-l spectrum (<math>30 \le \ell \le 2508</math>): <br />
<br />
* 100, 143, 143x217 and 217 GHz spectra and their covariance matrix (Sec. 3.3 {{PlanckPapers|planck2014-a15}})<br />
* best-fit foreground templates and inter-frequency calibration factors (Table 3 of {{PlanckPapers|planck2014-a15}})<br />
* Beam transfer function uncertainties {{PlanckPapers|planck2014-a08}}<br />
=== File names and Meta data ===<br />
<br />
The CMB spectrum and its covariance matrix are distributed in a single FITS file named <br />
<!--- * ''{{PLASingleFile | fileType=cosmo | name=COM_PowerSpect_CMB_R2.00.fits | link=COM_PowerSpect_CMB_R1.10.fits}}'' ---><br />
* ''COM_PowerSpect_CMB_R2.nn.fits''<br />
which contains 7 ''BINTABLE'' extensions<br />
<br />
; 1. TT low-ell, unbinned (TTLOLUNB)<br />
: with the low ell part of the spectrum, not binned, and for l=2-29. The table columns are<br />
# ''ELL'' (integer): multipole number<br />
# ''D_ELL'' (float): <math>D_ell</math> as described above<br />
# ''ERRUP'' (float): the upward uncertainty<br />
# ''ERRDOWN'' (float): the downward uncertainty<br />
<br />
; 2. TT high-ell, binned (TTHILBIN)<br />
: with the high-ell part of the spectrum, binned into 83 bins covering <math>\langle l \rangle = 47-2499\ </math> in bins of width <math>l=30</math> (with the exception of the last bin that is smaller). The table columns are as follows:<br />
# ''ELL'' (integer): mean multipole number of bin<br />
# ''L_MIN'' (integer): lowest multipole of bin<br />
# ''L_MAX'' (integer): highest multipole of bin<br />
# ''D_ELL'' (float): <math>D_\ell</math> as described above<br />
# ''ERR'' (float): the uncertainty<br />
<br />
; 3. TT high-ell unbinned (TTHILUNB) <br />
: with the high-ell part of the spectrum, unbinned, in 2979 bins covering <math>\langle l \rangle = 30-2508\ </math>. The table columns are as follows:<br />
# ''ELL'' (integer): multipole <br />
# ''D_ELL'' (float): <math>D_\ell</math> as described above<br />
# ''ERR'' (float): the uncertainty<br />
<br />
; 4. TE high-ell, binned (TEHILBIN) <br />
: with the high-ell part of the spectrum, binned into 83 bins covering <math>\langle l \rangle = 47-1988\ </math> in bins of width <math>l=30</math> (with the exception of the last bin that is smaller). The table columns are as follows:<br />
# ''ELL'' (integer): mean multipole number of bin<br />
# ''L_MIN'' (integer): lowest multipole of bin<br />
# ''L_MAX'' (integer): highest multipole of bin<br />
# ''D_ELL'' (float): <math>D_\ell</math> as described above<br />
# ''ERR'' (float): the uncertainty<br />
<br />
; 5. TE high-ell, unbinned (TEHILUNB) <br />
: with the high-ell part of the spectrum, unbinned, in 2979 bins covering <math>\langle l \rangle = 30-1996\ </math>. The table columns are as follows:<br />
# ''ELL'' (integer): multipole <br />
# ''D_ELL'' (float): <math>D_\ell</math> as described above<br />
# ''ERR'' (float): the uncertainty<br />
<br />
; 6. EE high-ell, binned (EELOLBIN) <br />
: with the high-ell part of the spectrum, binned into 83 bins covering <math>\langle l \rangle = 47-1988\ </math> in bins of width <math>l=30</math> (with the exception of the last bin that is smaller). The table columns are as follows:<br />
# ''ELL'' (integer): mean multipole number of bin<br />
# ''L_MIN'' (integer): lowest multipole of bin<br />
# ''L_MAX'' (integer): highest multipole of bin<br />
# ''D_ELL'' (float): <math>D_\ell</math> as described above<br />
# ''ERR'' (float): the uncertainty<br />
<br />
; 7. EE high-ell, unbinned (EEHILUNB) <br />
: with the high-ell part of the spectrum, unbinned, in 2979 bins covering <math>\langle l \rangle = 30-1996\ </math>. The table columns are as follows:<br />
# ''ELL'' (integer): multipole <br />
# ''D_ELL'' (float): <math>D_\ell</math> as described above<br />
# ''ERR'' (float): the uncertainty<br />
<br />
<br />
The spectra give <math>D_\ell = \ell(\ell+1)C_\ell / 2\pi </math> in units of <math>\mu\, K^2</math>. The covariance matrices of the spectra will be released in a second moment.<br />
<!-- <br />
<br />
The CMB spectrum is also given in a simple text comma-separated file:<br />
* ''{{PLASingleFile | fileType=cosmo | name=COM_PowerSpect_CMB_R1.10.txt |link=COM_PowerSpect_CMB_R1.10.txt}}''<br />
<br />
--><br />
<br />
==Likelihood==<br />
The likelihood code will released in March-April 2015 with an accompanying paper and an Explanatory Supplement update. <br />
<!-- <br />
===Likelihood===<br />
<span style="color:red"> ALL OF THE FOLLOWING IN THE LIKELIHOOD SECTION IS OLD. </span><br />
The likelihood code (and the data that comes with it) used to compute the likelihood of a model that predicts the CMB power spectra, lensing power spectrum, together with some foreground and some instrumental parameters. The data files are built primarily from the Planck mission results, but include also some results from the WMAP-9 data release. The data files are written in a specific format that can only be read by the code. The code consists in a c/f90 library, along with some optional tools in python. The code is used to read the data files, and given model power spectra and nuisance parameters it computes the log likelihood of that model. <br />
<br />
Detailed description of the installation and usage of the likelihood code and data is provided in the package. The package includes five data files: four for the CMB likelihoods and one for the lensing likelihood. All of the likelihoods delivered are described in detail in the {{PlanckPapers|planck2013-p08|1|Power spectrum & Likelihood Paper}} (for the CMB based likelihood) and in the {{PlanckPapers|planck2013-p12|1|Lensing Paper}} (for the lensing likelihood) .<br />
<br />
The CMB full likelihood has been divided into four parts to allow using selectively different ranges of multipoles. It also reflects the fact that the mathematical approximations used for those different parts are very different, as is the underlying data. In detail, we distribute<br />
* one low-<math>\ell</math> temperature only likelihood (commander), <br />
* one low-<math>\ell</math> temperature and polarisation likelihood (lowlike), and <br />
* one higl-<math>\ell</math> likelihood CAMspec. <br />
<br />
The ''Commander'' likelihood covers the multipoles 2 to 49. It uses a semi-analytic method to sample the low-<math>\ell</math> temperature likelihood on an intermediate product of one of the component separated maps. The samples are used along with an analytical approximation of the likelihood posterior to perform the likelihood computation in the code. See {{PlanckPapers|planck2013-p08}} section 8.1 for more details.<br />
<br />
The ''lowlike'' likelihood covers the multipoles 2 to 32 for temperature and polarization data. Since Planck is not releasing polarisation data at this time, the polarization map from WMAP9 is used instead. A temperature map is needed to perform the computation nevertheless, and we use here the same commander map. The likelihood is computed using a map-based approximation at low resolution and a master one at intermediate resolution, as in WMAP. The likelihood code actually calls a very slightly modified version of the WMAP9 code. This piece of the likelihood essentially provides a prior on the optical depth and has almost no other impact on cosmological parameter estimation. As such it could be replaced by a simple prior, and a user can decide to do so, which is one of the motivation to leave the three pieces of the CMB likelihood as different data packages; see {{PlanckPapers|planck2013-p08}} section 8.3 for more details. Note that the version of the WMAP code used here (code version v1.0) does not perform any test on the positive definiteness of the TT, TE, EE covariance matrices, and will return a null log likelihood in the unphysical cases where the absolute value of TE is too large. This will be corrected in a later version.<br />
<br />
The ''CAMspec'' likelihood covers the multipoles 50 to 2500 for temperature only. The likelihood is computed using a quadratic approximation, including mode to mode correlations that have been precomputed on a fiducial model. The likelihood uses data from the 100, 143 and 217 GHz channels. To do so it models the foreground at each frequency using the model described in the likelihood paper. Uncertainties on the relative calibration and on the beam transfer functions are included either as parametric models, or marginalized and integrated in the covariance matrix. Detailed description of the different nuisance parameters is given below. Priors are included in the likelihood on the CIB spectral index, relative calibration factors and beam error eigenmodes. See {{PlanckPapers|planck2013-p08}} section 2.1 for more details.<br />
<br />
The ''act/spt'' likelihood covers the multipoles 1500 to 10000 for temperature. It is described in{{BibCite|dun2013}}{{BibCite|Keis2011}}{{BibCite|Reic2012}}. It uses the code and data that can be retrieved from the [http://lambda.gsfc.nasa.gov/ Lambda archive] for [http://lambda.gsfc.nasa.gov/product/act/act_prod_table.cfm ACT] and [http://lambda.gsfc.nasa.gov/product/spt/spt_prod_table.cfm SPT]. It has been slightly modified to use a thermal and kinetic SZ model that matches the one used in CAMspec. As stated in{{BibCite|dun2013}}, the dust parameters a_ge and a_gs must be explored with the following priors: a_ge = 0.8 ± 0.2 and a_gs = 0.4 ± 0.2. Those priors are not included in the log likelihood computed by the code.<br />
<br />
The ''lensing'' likelihood covers the multipoles 40 to 400 using the result of the [[Specially_processed_maps | lensing reconstruction]]. It uses a quadratic approximation for the likelihood, with a covariance matrix including the marginalized contribution of the beam transfer function uncertainties, the diffuse point source correction uncertainties and the cosmological model uncertainty affecting the first order non-gaussian bias (N1). The correlation between temperature and lensing is not taken into account. Cosmological uncertainty effects on the normalization are dealt with using a first order renormalization procedure. This means that the code will need both the TT and $\phi\phi$ power spectrum up to <math>\ell</math> = 2048 to correctly perform the integrals needed for the renormalization. Nevertheless, the code will only produce an estimate based on the data between <math>\ell</math> = 40 to 400. See {{PlanckPapers|planck2013-p12}} section 6.1 for more details.<br />
</span><br />
<span style="color:red">OUTSTANDING: description of likelihood masks </span><br />
==Production process==<br />
<br />
===Likelihood===<br />
<span style="color:red"> ALL OF THE FOLLOWING IN THE LIKELIHOOD SECTION IS OLD. </span><br />
The code is based on some basic routines from the libpmc library in the [http://arxiv.org/abs/1101.0950 cosmoPMC] code. It also uses some code from the [http://lambda.gsfc.nasa.gov/product/map/dr5/likelihood_get.cfm WMAP9 likelihood] for the lowlike likelihood and{{BibCite|dun2013}}{{BibCite|Keis2011}}{{BibCite|Reic2012}} for the act/spt one. The rest of the code has been specifically written for the Planck data. Each likelihood file has been processed using a different and dedicated pipeline as described in the likelihood paper {{PlanckPapers|planck2013-p08}} (section 2 and 8) and in the lensing paper {{PlanckPapers|planck2013-p12}} (section 6.1). We refer the reader to those papers for full details. The data are then encapsulated into the specific file format.<br />
<br />
Each dataset comes with its own self check. Whenever the code is used to read a data file, a computation will be done against an included test spectrum/nuisance parameter, and the log-likelihood will be displayed along with the expected result. Difference of the order of 10<math>^{-6}</math> or less are expected depending of the architecture.<br />
<br />
==Inputs==<br />
<br />
===Likelihood===<br />
<br />
; ''commander'' :<br />
* all Planck channels maps<br />
* compact source catalogs<br />
* common masks<br />
* beam transfer functions for all channels<br />
<br />
; ''lowlike'' :<br />
* WMAP9 likelihood data<br />
* Low-<math>\ell</math> Commander map<br />
<br />
; ''CAMspec'' :<br />
* 100, 143 and 217 GHz detector and detsets maps<br />
* 857GHz channel map<br />
* compact source catalog<br />
* common masks (0,1 & 3)<br />
* beam transfer function and error eigenmodes and covariance for 100, 143 and 217 GHz detectors & detsets<br />
* theoretical templates for the tSZ and kSZ contributions<br />
* color corrections for the CIB emission for the 143 and 217GHz detectors and detsets<br />
* fiducial CMB model (bootstrapped from WMAP7 best fit spectrum) estimated noise contribution from the half-ring maps for 100, 143 and 217 GHz<br />
<br />
; ''lensing'' :<br />
* the lensing map<br />
* beam error eigenmodes and covariance for the 143 and 217GHz channel maps<br />
* fiducial CMB model (from Planck cosmological parameter best fit)<br />
<br />
; ''act/spt'' :<br />
* data and code from [http://lambda.gsfc.nasa.gov/product/act/act_fulllikelihood_get.cfm here]<br />
* the tSZ andkSZ template are changed to match those of CAMspec<br />
<br />
== File names and Meta data ==<br />
<br />
===Likelihood===<br />
<span style="color:red"> ALL OF THE FOLLOWING IN THE LIKELIHOOD SECTION IS OLD. </span><br />
<br />
'''Likelihood source code'''<br />
<br />
The source code is in the file<br />
: {{PLASingleFile |fileType=cosmo|name=COM_Code_Likelihood-v1.0_R1.10.tar.gz|link=COM_Code_Likelihood-v1.0_R1.10.tar.gz}} (C, f90 and python likelihood library and tools)<br />
<br />
'''Likelihood data packages'''<br />
<br />
The {{PLALikelihood|type=Data|link=data packages}} are<br />
: ''{{PLASingleFile | fileType=cosmo | name=COM_Data_Likelihood-commander_R1.10.tar.gz | link=COM_Data_Likelihood-commander_R1.10.tar.gz}}'' (low-ell TT likelihood)<br />
: ''{{PLASingleFile | fileType=cosmo | name=COM_Data_Likelihood-lowlike_R1.10.tar.gz | link=COM_Data_Likelihood-lowlike_R1.10.tar.gz}}'' (low-ell TE,EE,BB likelihood)<br />
: ''{{PLASingleFile | fileType=cosmo | name=COM_Data_Likelihood-CAMspec_R1.10.tar.gz | link=COM_Data_Likelihood-CAMspec_R1.10.tar.gz}}'' (high-ell TT likelihood)<br />
: ''{{PLASingleFile | fileType=cosmo | name=COM_Data_Likelihood-actspt_R1.10.tar | link=COM_Data_Likelihood-actspt_R1.10.tar.gz}}'' (high-ell TT likelihood)<br />
: ''{{PLASingleFile | fileType=cosmo | name=COM_Data_Likelihood-lensing_R1.10.tar.gz | link=COM_Data_Likelihood-lensing_R1.10.tar.gz}}'' (lensing likelihood)<br />
<br />
Untar and unzip all files to recover the code and likelihood data. Each package comes with a README file; follow the instructions inclosed to<br />
build the code and use it. To compute the CMB likelihood one has to sum the log likelihood of each of the commander_v4.1_lm49.clik, lowlike_v222.clik and CAMspec_v6.2TN_2013_02_26.clik, actspt_2013_01.clik. To compute the CMB+lensing likelihood, one has to sum the log likelihood of all 5 files.<br />
<br />
The CMB and lensing likelihood format are different. The CMB files have the termination .clik, the lensing one .clik_lensing. The lensing data being simpler (due to the less detailled modeling permitted by the lower signal-noise), the file is a simple ascii file containing all the data along with comments describing it, and linking the different quantities to the lensing paper. The CMB file format is more complex and must accommodate different forms of data (maps, power spectrum, distribution samples, covariance matrices...). It consists of a tree structure containing the data. At each level of the tree structure a given directory can contain array data (in the form of FITS files or ascii files for strings) and scalar data (joined in a single ascii file "_mdb"). Those files are not user modifiable and do not contain interesting meta data for the user. Tools to manipulate those files are included in the code package as optional python tools. They are documented in the code package.<br />
<br />
'''Likelihood masks'''<br />
<br />
The masks used in the Likelihood paper {{PlanckPapers|planck2013-p08}} are found in<br />
{{PLASingleFile|fileType=map|name=COM_Mask_Likelihood_2048_R1.10.fits|link=COM_Mask_Likelihood_2048_R1.10.fits}}<br />
<br />
which contains ten masks which are written into a single ''BINTABLE'' extension of 10 columns by 50331648 rows (the number of Healpix pixels in an Nside = 2048 map). The structure is as follows, where the column names are the names of the masks: <br />
<br />
{| border="1" cellpadding="3" cellspacing="0" align="center" style="text-align:left" width=800px<br />
|+ '''Likelihodd masks file data structure'''<br />
|- bgcolor="ffdead" <br />
!colspan="4" | 1. EXTNAME = 'MSK-LIKE' : Data columns<br />
|- bgcolor="ffdead" <br />
! Column Name || Data Type || Units || Description<br />
|-<br />
|CL31 || Real*4 || none || mask<br />
|-<br />
|CL39 || Real*4 || none || mask<br />
|-<br />
|CL49 || Real*4 || none || mask<br />
|-<br />
|G22 || Real*4 || none || mask <br />
|-<br />
|G35 || Real*4 || none || mask<br />
|-<br />
|G45 || Real*4 || none || mask<br />
|-<br />
|G56 || Real*4 || none || mask<br />
|-<br />
|G65 || Real*4 || none || mask<br />
|-<br />
|PS96 || Real*4 || none || mask<br />
|-<br />
|PSA82 || Real*4 || none || mask<br />
|-<br />
|- bgcolor="ffdead" <br />
! Keyword || Data Type || Value || Description<br />
|-<br />
|PIXTYPE || string || HEALPIX ||<br />
|-<br />
|COORDSYS || string || GALACTIC ||Coordinate system <br />
|-<br />
|ORDERING || string || NESTED || Healpix ordering<br />
|-<br />
|NSIDE || Int || 2048 || Healpix Nside <br />
|-<br />
|FIRSTPIX || Int*4 || 0 || First pixel number<br />
|-<br />
|LASTPIX || Int*4 || 50331647 || Last pixel number, for LFI and HFI, respectively<br />
<br />
|}<br />
--><br />
<br />
== References ==<br />
<References /><br />
<br />
<br />
<br />
[[Category:Mission products|008]]</div>
Xdupac
https://wiki.cosmos.esa.int/planckpla2015/index.php?title=CMB_spectrum_%26_Likelihood_Code&diff=11441
CMB spectrum & Likelihood Code
2015-02-09T09:41:18Z
<p>Xdupac: /* TT */</p>
<hr />
<div>{{DISPLAYTITLE:2015 CMB spectra and likelihood code}}<br />
<br />
==2015 CMB spectra==<br />
<br />
<br />
===General description===<br />
====TT====<br />
The Planck best-fit CMB temperature power spectrum, shown in the figure below, covers the wide range of multipoles <math> \ell </math> = 2-2508. Over the multipole range <math> \ell </math> = 2–29, the power spectrum is derived from the ''Commander'': component separation algorithm applied to the combination of Planck 2015 temperature data between 30 and 857 GHz, the 9-year WMAP sky maps, and the 408 MHz Haslam et al. (1982) survey, including 93% of the sky {{PlanckPapers|planck2014-a12}} . The asymmetric error bars associated to this spectrum are the 68% confidence limits and include the uncertainties due to foreground subtraction.<br />
<br />
For multipoles equal or greater than <math>\ell=30</math>, instead, the spectrum is derived from the ''Plik'' likelihood {{PlanckPapers|planck2014-a13}} by optimally combining the spectra in the frequency range 100-217 GHz, and correcting them for unresolved foregrounds using the best-fit foreground solution from a Planck TT+lowP <math>\Lambda</math>CDM run. Associated 1-sigma errors include beam uncertainties. Both ''Commander'' and ''Plik'' are described in more details in the sections below.<br />
<br />
[[File: A15_TT.png|thumb|center|700px|'''The Planck 2015 TT power spectrum. Logarithmic x-scale up to <math>\ell = 30 </math> , linear at higher <math \ell>. The red line is the Planck best-fit primordial power spectrum (cf Planck TT+lowP in Table 3 of Planck-2015-A15[3]). Residuals with respect to this model are shown in the lower panel. The error bars show <math>\pm 1\sigma</math> uncertainties.''']]<br />
<br />
====TE and EE====<br />
The Planck best-fit CMB polarization and temperature-polarization cross-correlation power spectra, shown in the figure below, cover the multipole range <math> \ell </math> = 30-1996. The data points relative to the multipole range <math> \ell </math> = 2-29 will be released in a second moment.<br />
Analogously to the TT case, the <math> \ell\ge 30 </math> spectrum is derived from the ''Plik'' likelihood {{PlanckPapers|planck2014-a13}} by optimally combining the spectra in the frequency range 100-217 GHz, and correcting them for unresolved foregrounds using the best-fit foreground solution from a Planck TT,TE,EE+lowP <math>\Lambda</math>CDM run. <br />
<br />
{|style="margin: 0 auto;"<br />
|[[File: A15_EE.png|thumb|center|500px|'''2015 CMB EE spectrum. The red line is the Planck best-fit primordial power spectrum (cf Planck TT+lowP in Table 3 of {{PlanckPapers|planck2014-a15}}). The blue shaded area shows the uncertainties due to cosmic variance alone.''']]<br />
|[[File: A15_TE.png|thumb|center|500px|'''2015 CMB TE spectrum. The red line is the Planck best-fit primordial power spectrum (cf Planck TT+lowP in Table 3 of {{PlanckPapers|planck2014-a15}}). The blue shaded area shows the uncertainties due to cosmic variance alone.''']]<br />
|}<br />
<br />
===Production process===<br />
The <math>\ell</math> < 30 part of the Planck TT power spectrum is derived from the Commander approach, which implements Bayesian component separation in pixel space, fitting a parametric model to the data by sampling the posterior distribution for the model parameters {{PlanckPapers|planck2014-a12}}. The power spectrum at any multipole <math>\ell</math> is given as the maximum probability point for the posterior <math>C_\ell</math> distribution, marginalized over the other multipoles, and the error bars are 68% confidence level; see {{PlanckPapers|planck2014-a12}}. <br />
<br />
The <math>\ell \ge 30</math> part of the TT, TE and EE power spectra have been derived by the Plik likelihood, a code that implements a pseudo-Cl based technique, extensively described in Sec. 2 and the Appendix of {{PlanckPapers|planck2013-p08}} and {{PlanckPapers|planck2014-a13}}. Frequency spectra are computed as cross-spectra between half-mission maps. Mask and multipole range choices for each frequency spectrum are summarized in Section 3.3 of {{PlanckPapers|planck2014-a15}} and in {{PlanckPapers|planck2014-a13}}. The final power spectrum is an optimal combination of the 100, 143, 143x217 and 217 GHz spectra, corrected for the best-fit unresolved foregrounds and inter-frequency calibration factors, as derived from the full likelihood analysis (for TT we use the best-fit solutions for the nuisance parameters from the Planck+TT+lowP data combination, while for TE and EE we use the best fit from Planck+TT+lowP, cf Table 3 of {{PlanckPapers|planck2014-a15}}). A thorough description of the models of unresolved foregrounds is given in {{PlanckPapers|planck2014-a13}}. The spectrum covariance matrix accounts for cosmic variance and noise contributions, together with beam uncertainties. The <math>\ell \ge 30</math> CMB TT spectrum and associated covariance matrix are available in two formats:<br />
#Unbinned. TT: 2479 bandpowers (<math>\ell=30-2508</math>); TE or EE: 1697 bandpowers (<math>\ell=30-1996</math>).<br />
#Binned, in bins of <math> \Delta\ell=30 </math>. TT: 83 bandpowers. TE or EE: 66 bandpowers. We bin the <math> C_\ell </math> power spectrum with a weight proportional to <math> \ell (\ell+1) </math>, so that the <math> C_{\ell_b} </math> binned bandpower centered in <math> \ell_b </math> is: <math> \\ C_{\ell_b}=\Sigma_{\ell \in b} w_{\ell_b\ell} C_\ell \quad \text{with} \quad w_{\ell_b\ell}=\frac{\ell (\ell+1)}{\Sigma_{\ell \in b} \ell (\ell+1)}. \\</math> Equivalently, using the matrix formalism, we can construct the binning matrix B as: <math>\\ B_{\ell_b \ell}=w_{\ell_b\ell} \\ </math> where B is a <math> n_b\times n_\ell</math> matrix, with <math>n_b=83</math> the number of bins and <math>n_\ell=2479</math> the number of unbinned multipoles. Thus: <math> \\ \vec{C}_\mathrm{binned}=B \, \vec{C} \\ \mathrm{cov_\mathrm{binned}}= B\, \mathrm{cov}\, B^T \\ \ell_b=B\, \ell \\ </math> Here, <math> \vec{C}_{binned}\, (\vec{C}) </math> is the vector containing all the binned (unbinned) <math>C_\ell</math> bandpowers, <math>\mathrm{cov} </math> is the covariance matrix and <math>\ell_b</math> is the weighted average multipole in each bin. Note that following this definition, <math>\ell_b</math> can be a non-integer. The binned <math>D_{\ell_B}</math> power spectrum is then calculated as: <math> \\ D_{\ell_b}=\frac{\ell_b (\ell_b+1)}{2\pi} C_{\ell_b} </math>.<br />
<br />
===Inputs===<br />
<br />
; Low-l spectrum (<math>\ell < 30</math>):<br />
* Planck 30 and 44 GHz frequency maps<br />
* Planck 70 to 857 GHz detector and detector set maps<br />
* 9-year WMAP temperature sky maps between 23 and 94 GHz<br />
* 408 MHz survey by Haslam et al. (1982) <br />
* Commander <math>\chi^2</math> based LM93 confidence mask {{PlanckPapers|planck2014-a12}}<br />
<br />
; High-l spectrum (<math>30 \le \ell \le 2508</math>): <br />
<br />
* 100, 143, 143x217 and 217 GHz spectra and their covariance matrix (Sec. 3.3 {{PlanckPapers|planck2014-a15}})<br />
* best-fit foreground templates and inter-frequency calibration factors (Table 3 of {{PlanckPapers|planck2014-a15}})<br />
* Beam transfer function uncertainties {{PlanckPapers|planck2014-a08}}<br />
=== File names and Meta data ===<br />
<br />
The CMB spectrum and its covariance matrix are distributed in a single FITS file named <br />
<!--- * ''{{PLASingleFile | fileType=cosmo | name=COM_PowerSpect_CMB_R2.00.fits | link=COM_PowerSpect_CMB_R1.10.fits}}'' ---><br />
* ''COM_PowerSpect_CMB_R2.nn.fits''<br />
which contains 7 ''BINTABLE'' extensions<br />
<br />
; 1. TT low-ell, unbinned (TTLOLUNB)<br />
: with the low ell part of the spectrum, not binned, and for l=2-29. The table columns are<br />
# ''ELL'' (integer): multipole number<br />
# ''D_ELL'' (float): <math>D_ell</math> as described above<br />
# ''ERRUP'' (float): the upward uncertainty<br />
# ''ERRDOWN'' (float): the downward uncertainty<br />
<br />
; 2. TT high-ell, binned (TTHILBIN)<br />
: with the high-ell part of the spectrum, binned into 83 bins covering <math>\langle l \rangle = 47-2499\ </math> in bins of width <math>l=30</math> (with the exception of the last bin that is smaller). The table columns are as follows:<br />
# ''ELL'' (integer): mean multipole number of bin<br />
# ''L_MIN'' (integer): lowest multipole of bin<br />
# ''L_MAX'' (integer): highest multipole of bin<br />
# ''D_ELL'' (float): <math>D_\ell</math> as described above<br />
# ''ERR'' (float): the uncertainty<br />
<br />
; 3. TT high-ell unbinned (TTHILUNB) <br />
: with the high-ell part of the spectrum, unbinned, in 2979 bins covering <math>\langle l \rangle = 30-2508\ </math>. The table columns are as follows:<br />
# ''ELL'' (integer): multipole <br />
# ''D_ELL'' (float): <math>D_\ell</math> as described above<br />
# ''ERR'' (float): the uncertainty<br />
<br />
; 4. TE high-ell, binned (TEHILBIN) <br />
: with the high-ell part of the spectrum, binned into 83 bins covering <math>\langle l \rangle = 47-1988\ </math> in bins of width <math>l=30</math> (with the exception of the last bin that is smaller). The table columns are as follows:<br />
# ''ELL'' (integer): mean multipole number of bin<br />
# ''L_MIN'' (integer): lowest multipole of bin<br />
# ''L_MAX'' (integer): highest multipole of bin<br />
# ''D_ELL'' (float): <math>D_\ell</math> as described above<br />
# ''ERR'' (float): the uncertainty<br />
<br />
; 5. TE high-ell, unbinned (TEHILUNB) <br />
: with the high-ell part of the spectrum, unbinned, in 2979 bins covering <math>\langle l \rangle = 30-1996\ </math>. The table columns are as follows:<br />
# ''ELL'' (integer): multipole <br />
# ''D_ELL'' (float): <math>D_\ell</math> as described above<br />
# ''ERR'' (float): the uncertainty<br />
<br />
; 6. EE high-ell, binned (EELOLBIN) <br />
: with the high-ell part of the spectrum, binned into 83 bins covering <math>\langle l \rangle = 47-1988\ </math> in bins of width <math>l=30</math> (with the exception of the last bin that is smaller). The table columns are as follows:<br />
# ''ELL'' (integer): mean multipole number of bin<br />
# ''L_MIN'' (integer): lowest multipole of bin<br />
# ''L_MAX'' (integer): highest multipole of bin<br />
# ''D_ELL'' (float): <math>D_\ell</math> as described above<br />
# ''ERR'' (float): the uncertainty<br />
<br />
; 7. EE high-ell, unbinned (EEHILUNB) <br />
: with the high-ell part of the spectrum, unbinned, in 2979 bins covering <math>\langle l \rangle = 30-1996\ </math>. The table columns are as follows:<br />
# ''ELL'' (integer): multipole <br />
# ''D_ELL'' (float): <math>D_\ell</math> as described above<br />
# ''ERR'' (float): the uncertainty<br />
<br />
<br />
The spectra give <math>D_\ell = \ell(\ell+1)C_\ell / 2\pi </math> in units of <math>\mu\, K^2</math>. The covariance matrices of the spectra will be released in a second moment.<br />
<!-- <br />
<br />
The CMB spectrum is also given in a simple text comma-separated file:<br />
* ''{{PLASingleFile | fileType=cosmo | name=COM_PowerSpect_CMB_R1.10.txt |link=COM_PowerSpect_CMB_R1.10.txt}}''<br />
<br />
--><br />
<br />
==Likelihood==<br />
The likelihood code will released in March-April 2015 with an accompanying paper and an Explanatory Supplement update. <br />
<!-- <br />
===Likelihood===<br />
<span style="color:red"> ALL OF THE FOLLOWING IN THE LIKELIHOOD SECTION IS OLD. </span><br />
The likelihood code (and the data that comes with it) used to compute the likelihood of a model that predicts the CMB power spectra, lensing power spectrum, together with some foreground and some instrumental parameters. The data files are built primarily from the Planck mission results, but include also some results from the WMAP-9 data release. The data files are written in a specific format that can only be read by the code. The code consists in a c/f90 library, along with some optional tools in python. The code is used to read the data files, and given model power spectra and nuisance parameters it computes the log likelihood of that model. <br />
<br />
Detailed description of the installation and usage of the likelihood code and data is provided in the package. The package includes five data files: four for the CMB likelihoods and one for the lensing likelihood. All of the likelihoods delivered are described in detail in the {{PlanckPapers|planck2013-p08|1|Power spectrum & Likelihood Paper}} (for the CMB based likelihood) and in the {{PlanckPapers|planck2013-p12|1|Lensing Paper}} (for the lensing likelihood) .<br />
<br />
The CMB full likelihood has been divided into four parts to allow using selectively different ranges of multipoles. It also reflects the fact that the mathematical approximations used for those different parts are very different, as is the underlying data. In detail, we distribute<br />
* one low-<math>\ell</math> temperature only likelihood (commander), <br />
* one low-<math>\ell</math> temperature and polarisation likelihood (lowlike), and <br />
* one higl-<math>\ell</math> likelihood CAMspec. <br />
<br />
The ''Commander'' likelihood covers the multipoles 2 to 49. It uses a semi-analytic method to sample the low-<math>\ell</math> temperature likelihood on an intermediate product of one of the component separated maps. The samples are used along with an analytical approximation of the likelihood posterior to perform the likelihood computation in the code. See {{PlanckPapers|planck2013-p08}} section 8.1 for more details.<br />
<br />
The ''lowlike'' likelihood covers the multipoles 2 to 32 for temperature and polarization data. Since Planck is not releasing polarisation data at this time, the polarization map from WMAP9 is used instead. A temperature map is needed to perform the computation nevertheless, and we use here the same commander map. The likelihood is computed using a map-based approximation at low resolution and a master one at intermediate resolution, as in WMAP. The likelihood code actually calls a very slightly modified version of the WMAP9 code. This piece of the likelihood essentially provides a prior on the optical depth and has almost no other impact on cosmological parameter estimation. As such it could be replaced by a simple prior, and a user can decide to do so, which is one of the motivation to leave the three pieces of the CMB likelihood as different data packages; see {{PlanckPapers|planck2013-p08}} section 8.3 for more details. Note that the version of the WMAP code used here (code version v1.0) does not perform any test on the positive definiteness of the TT, TE, EE covariance matrices, and will return a null log likelihood in the unphysical cases where the absolute value of TE is too large. This will be corrected in a later version.<br />
<br />
The ''CAMspec'' likelihood covers the multipoles 50 to 2500 for temperature only. The likelihood is computed using a quadratic approximation, including mode to mode correlations that have been precomputed on a fiducial model. The likelihood uses data from the 100, 143 and 217 GHz channels. To do so it models the foreground at each frequency using the model described in the likelihood paper. Uncertainties on the relative calibration and on the beam transfer functions are included either as parametric models, or marginalized and integrated in the covariance matrix. Detailed description of the different nuisance parameters is given below. Priors are included in the likelihood on the CIB spectral index, relative calibration factors and beam error eigenmodes. See {{PlanckPapers|planck2013-p08}} section 2.1 for more details.<br />
<br />
The ''act/spt'' likelihood covers the multipoles 1500 to 10000 for temperature. It is described in{{BibCite|dun2013}}{{BibCite|Keis2011}}{{BibCite|Reic2012}}. It uses the code and data that can be retrieved from the [http://lambda.gsfc.nasa.gov/ Lambda archive] for [http://lambda.gsfc.nasa.gov/product/act/act_prod_table.cfm ACT] and [http://lambda.gsfc.nasa.gov/product/spt/spt_prod_table.cfm SPT]. It has been slightly modified to use a thermal and kinetic SZ model that matches the one used in CAMspec. As stated in{{BibCite|dun2013}}, the dust parameters a_ge and a_gs must be explored with the following priors: a_ge = 0.8 ± 0.2 and a_gs = 0.4 ± 0.2. Those priors are not included in the log likelihood computed by the code.<br />
<br />
The ''lensing'' likelihood covers the multipoles 40 to 400 using the result of the [[Specially_processed_maps | lensing reconstruction]]. It uses a quadratic approximation for the likelihood, with a covariance matrix including the marginalized contribution of the beam transfer function uncertainties, the diffuse point source correction uncertainties and the cosmological model uncertainty affecting the first order non-gaussian bias (N1). The correlation between temperature and lensing is not taken into account. Cosmological uncertainty effects on the normalization are dealt with using a first order renormalization procedure. This means that the code will need both the TT and $\phi\phi$ power spectrum up to <math>\ell</math> = 2048 to correctly perform the integrals needed for the renormalization. Nevertheless, the code will only produce an estimate based on the data between <math>\ell</math> = 40 to 400. See {{PlanckPapers|planck2013-p12}} section 6.1 for more details.<br />
</span><br />
<span style="color:red">OUTSTANDING: description of likelihood masks </span><br />
==Production process==<br />
<br />
===Likelihood===<br />
<span style="color:red"> ALL OF THE FOLLOWING IN THE LIKELIHOOD SECTION IS OLD. </span><br />
The code is based on some basic routines from the libpmc library in the [http://arxiv.org/abs/1101.0950 cosmoPMC] code. It also uses some code from the [http://lambda.gsfc.nasa.gov/product/map/dr5/likelihood_get.cfm WMAP9 likelihood] for the lowlike likelihood and{{BibCite|dun2013}}{{BibCite|Keis2011}}{{BibCite|Reic2012}} for the act/spt one. The rest of the code has been specifically written for the Planck data. Each likelihood file has been processed using a different and dedicated pipeline as described in the likelihood paper {{PlanckPapers|planck2013-p08}} (section 2 and 8) and in the lensing paper {{PlanckPapers|planck2013-p12}} (section 6.1). We refer the reader to those papers for full details. The data are then encapsulated into the specific file format.<br />
<br />
Each dataset comes with its own self check. Whenever the code is used to read a data file, a computation will be done against an included test spectrum/nuisance parameter, and the log-likelihood will be displayed along with the expected result. Difference of the order of 10<math>^{-6}</math> or less are expected depending of the architecture.<br />
<br />
==Inputs==<br />
<br />
===Likelihood===<br />
<br />
; ''commander'' :<br />
* all Planck channels maps<br />
* compact source catalogs<br />
* common masks<br />
* beam transfer functions for all channels<br />
<br />
; ''lowlike'' :<br />
* WMAP9 likelihood data<br />
* Low-<math>\ell</math> Commander map<br />
<br />
; ''CAMspec'' :<br />
* 100, 143 and 217 GHz detector and detsets maps<br />
* 857GHz channel map<br />
* compact source catalog<br />
* common masks (0,1 & 3)<br />
* beam transfer function and error eigenmodes and covariance for 100, 143 and 217 GHz detectors & detsets<br />
* theoretical templates for the tSZ and kSZ contributions<br />
* color corrections for the CIB emission for the 143 and 217GHz detectors and detsets<br />
* fiducial CMB model (bootstrapped from WMAP7 best fit spectrum) estimated noise contribution from the half-ring maps for 100, 143 and 217 GHz<br />
<br />
; ''lensing'' :<br />
* the lensing map<br />
* beam error eigenmodes and covariance for the 143 and 217GHz channel maps<br />
* fiducial CMB model (from Planck cosmological parameter best fit)<br />
<br />
; ''act/spt'' :<br />
* data and code from [http://lambda.gsfc.nasa.gov/product/act/act_fulllikelihood_get.cfm here]<br />
* the tSZ andkSZ template are changed to match those of CAMspec<br />
<br />
== File names and Meta data ==<br />
<br />
===Likelihood===<br />
<span style="color:red"> ALL OF THE FOLLOWING IN THE LIKELIHOOD SECTION IS OLD. </span><br />
<br />
'''Likelihood source code'''<br />
<br />
The source code is in the file<br />
: {{PLASingleFile |fileType=cosmo|name=COM_Code_Likelihood-v1.0_R1.10.tar.gz|link=COM_Code_Likelihood-v1.0_R1.10.tar.gz}} (C, f90 and python likelihood library and tools)<br />
<br />
'''Likelihood data packages'''<br />
<br />
The {{PLALikelihood|type=Data|link=data packages}} are<br />
: ''{{PLASingleFile | fileType=cosmo | name=COM_Data_Likelihood-commander_R1.10.tar.gz | link=COM_Data_Likelihood-commander_R1.10.tar.gz}}'' (low-ell TT likelihood)<br />
: ''{{PLASingleFile | fileType=cosmo | name=COM_Data_Likelihood-lowlike_R1.10.tar.gz | link=COM_Data_Likelihood-lowlike_R1.10.tar.gz}}'' (low-ell TE,EE,BB likelihood)<br />
: ''{{PLASingleFile | fileType=cosmo | name=COM_Data_Likelihood-CAMspec_R1.10.tar.gz | link=COM_Data_Likelihood-CAMspec_R1.10.tar.gz}}'' (high-ell TT likelihood)<br />
: ''{{PLASingleFile | fileType=cosmo | name=COM_Data_Likelihood-actspt_R1.10.tar | link=COM_Data_Likelihood-actspt_R1.10.tar.gz}}'' (high-ell TT likelihood)<br />
: ''{{PLASingleFile | fileType=cosmo | name=COM_Data_Likelihood-lensing_R1.10.tar.gz | link=COM_Data_Likelihood-lensing_R1.10.tar.gz}}'' (lensing likelihood)<br />
<br />
Untar and unzip all files to recover the code and likelihood data. Each package comes with a README file; follow the instructions inclosed to<br />
build the code and use it. To compute the CMB likelihood one has to sum the log likelihood of each of the commander_v4.1_lm49.clik, lowlike_v222.clik and CAMspec_v6.2TN_2013_02_26.clik, actspt_2013_01.clik. To compute the CMB+lensing likelihood, one has to sum the log likelihood of all 5 files.<br />
<br />
The CMB and lensing likelihood format are different. The CMB files have the termination .clik, the lensing one .clik_lensing. The lensing data being simpler (due to the less detailled modeling permitted by the lower signal-noise), the file is a simple ascii file containing all the data along with comments describing it, and linking the different quantities to the lensing paper. The CMB file format is more complex and must accommodate different forms of data (maps, power spectrum, distribution samples, covariance matrices...). It consists of a tree structure containing the data. At each level of the tree structure a given directory can contain array data (in the form of FITS files or ascii files for strings) and scalar data (joined in a single ascii file "_mdb"). Those files are not user modifiable and do not contain interesting meta data for the user. Tools to manipulate those files are included in the code package as optional python tools. They are documented in the code package.<br />
<br />
'''Likelihood masks'''<br />
<br />
The masks used in the Likelihood paper {{PlanckPapers|planck2013-p08}} are found in<br />
{{PLASingleFile|fileType=map|name=COM_Mask_Likelihood_2048_R1.10.fits|link=COM_Mask_Likelihood_2048_R1.10.fits}}<br />
<br />
which contains ten masks which are written into a single ''BINTABLE'' extension of 10 columns by 50331648 rows (the number of Healpix pixels in an Nside = 2048 map). The structure is as follows, where the column names are the names of the masks: <br />
<br />
{| border="1" cellpadding="3" cellspacing="0" align="center" style="text-align:left" width=800px<br />
|+ '''Likelihodd masks file data structure'''<br />
|- bgcolor="ffdead" <br />
!colspan="4" | 1. EXTNAME = 'MSK-LIKE' : Data columns<br />
|- bgcolor="ffdead" <br />
! Column Name || Data Type || Units || Description<br />
|-<br />
|CL31 || Real*4 || none || mask<br />
|-<br />
|CL39 || Real*4 || none || mask<br />
|-<br />
|CL49 || Real*4 || none || mask<br />
|-<br />
|G22 || Real*4 || none || mask <br />
|-<br />
|G35 || Real*4 || none || mask<br />
|-<br />
|G45 || Real*4 || none || mask<br />
|-<br />
|G56 || Real*4 || none || mask<br />
|-<br />
|G65 || Real*4 || none || mask<br />
|-<br />
|PS96 || Real*4 || none || mask<br />
|-<br />
|PSA82 || Real*4 || none || mask<br />
|-<br />
|- bgcolor="ffdead" <br />
! Keyword || Data Type || Value || Description<br />
|-<br />
|PIXTYPE || string || HEALPIX ||<br />
|-<br />
|COORDSYS || string || GALACTIC ||Coordinate system <br />
|-<br />
|ORDERING || string || NESTED || Healpix ordering<br />
|-<br />
|NSIDE || Int || 2048 || Healpix Nside <br />
|-<br />
|FIRSTPIX || Int*4 || 0 || First pixel number<br />
|-<br />
|LASTPIX || Int*4 || 50331647 || Last pixel number, for LFI and HFI, respectively<br />
<br />
|}<br />
--><br />
<br />
== References ==<br />
<References /><br />
<br />
<br />
<br />
[[Category:Mission products|008]]</div>
Xdupac
https://wiki.cosmos.esa.int/planckpla2015/index.php?title=Questions_and_Answers&diff=11439
Questions and Answers
2015-02-05T13:01:02Z
<p>Xdupac: /* Where can I find the Planck data? */</p>
<hr />
<div>==Where can I find the Planck data?==<br />
In the Planck Legacy Archive : [http://archives.esac.esa.int/pla]<br />
<br />
==Do you provide any links to the Planck products in the archive?==<br />
Yes. All the products page in the [[Mission products]] page provide links to the products they describe. However, we do not recommend you use this as your main source of data. We provide a GUI for you to directly access the archive (see question 1 above)and the functionality it offers makes it much easier to search for and download data than the links offered in the Explanatory supplement.<br />
<br />
==What's wrong with the links to the ES in fits file headers?==<br />
The fits files with the Planck products contain the url for their corresponding pages in the Explanatory supplement in a fits header COMMENT but some of these urls are wrong. This is a problem with the urls in the COMMENT fields not with the pages in the ES. Do not attempt to use any urls in COMMENT fields in the headers of the fits files containing the products.<br />
<br />
==What browser should I use to view the Explanatory supplement?==<br />
Any recent version of firefox should work fine. We know that IE should also work but some versions are very slow loading the formulas. In general any recent browser should work.<br />
<br />
==IE has problems with formulas. What should I do?==<br />
We use MathJax to display equations. It is well known that some combinations of IE and MathJax have problems. For a possible solution to you problem look at the [http://www.mathjax.org/resources/faqs/#IE-issues MathJax FAQ]<br />
<br />
==I have several questions and problems not covered in this page. Is there someone I can contact for help?==<br />
Yes. Please contact the [http://www.sciops.esa.int/helpdesk_pia PLA help desk].<br />
<br />
==Have you got any plans to update the Explanatory supplement?==<br />
Yes. The Explanatory supplement is a live document. It will be updated regularly to match any product updates and it will also suffer a major upgrade to accompany any future Planck data release.<br />
<br />
==Do you offer the Explanatory supplement as a pdf file?==<br />
Yes, you can find it here but you should be aware this is still very much an experimental product. We use the same software wikipedia uses to produce books but there are still several problems we are trying to solve. The two major isses at the moment are: some figures disapear from the pdf file, and the references you can find at the end of most pages are not printed. We are looking into these (and a few other) problems and expect to provide a solution at some point. If you want to build your own book using your selection of pages you will find a brief guide [[Help:books | here ]]. As this is an experimental product it is at this point not fully supported and we ask you not to use the Planck Help desk asking us support for this.</div>
Xdupac
https://wiki.cosmos.esa.int/planckpla2015/index.php?title=Product_Table_for_PLAv2&diff=11436
Product Table for PLAv2
2015-02-05T12:21:07Z
<p>Xdupac: /* Other products */</p>
<hr />
<div>{{DISPLAYTITLE:Products table for PLAv2}}<br />
==Product categories==<br />
*New products for this release that I believe have been confirmed appear in <span style="color:Blue">blue font</span>, products that are still TBC in <span style="color:Red">red font</span> (if it is one entire category of products I will just use color in the products category name, e.g. <span style="color:Blue">1 year maps</span>). Please check this in the tables and let me know whether there are any errors.<br />
*The Obs column contains links to notes at the end of each table. Please check the notes and let me know your feedback.<br />
*More general comments appear at the end of the numbered notes.<br />
<br />
I suggest you use the [[Talk:Product_Table_for_PLAv2|discussion page associated with this page]] to provide your feedback or make any comments relate to the list of products. The discussion page has the same structures in terms of sections as this page. Please try to write your comments/feedback in the appropriate section. I would also ask you to put your initials in the comments you write so that I can more easily get back to you to try to clarify any questions. Yes, it is true I can find out who wrote what in the history page but it makes my life easier if you associate your name to the comments you provide.<br />
<br />
The '''Description''' column will be used to add a one line description of the product that will appear in the archive as a tooltip associated with the product to allow a quick identification by users.<br />
===Time Series===<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=1050px<br />
|+ '''FITS filenames'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" rowspan="9" | <span style="color:Blue">Detector timeseries</span><br />
|rowspan="3" align="center" | LFI <br />
| LFI_TOI_030-SCI_R2.xx_ODXXXX.fits<br />
| <br />
| <br />
|00 <br />
| 10-09-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| LFI_TOI_044-SCI_R2.xx_ODXXXX.fits<br />
| <br />
| <br />
| 00<br />
| 10-09-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| LFI_TOI_070-SCI_R2.xx_ODXXXX.fits<br />
| <br />
| <br />
| 00<br />
| 10-09-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
|rowspan="6" align="center" | HFI <br />
| HFI_TOI_100-SCI_R2.xx_ODXXXX.fits<br />
| Only PSB: not for Feb. 2015 release<br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
|<br />
|-<br />
| HFI_TOI_143-SCI_R2.xx_ODXXXX.fits<br />
| without PSBs<br />
| <br />
| 00<br />
| 20/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_TOI_217-SCI_R2.xx_ODXXXX.fits<br />
| without PSBs<br />
| <br />
| 00<br />
| 20/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_TOI_353-SCI_R2.xx_ODXXXX.fits<br />
| with PSBs<br />
| <br />
| 00<br />
| 19/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_TOI_545-SCI_R2.xx_ODXXXX.fits<br />
| <br />
| <br />
| 00<br />
| 23/01/2015<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_TOI_857-SCI_R2.xx_ODXXXX.fits<br />
| <br />
| <br />
| 00<br />
| 23/01/2015<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="7" | <span style="color:Blue">Offsets</span><br />
| rowspan="6" align="center"| LFI <br />
| LFI_TOI_030-OFF_R2.xx_ODXXXX-full.fits<br />
| <br />
| <br />
| 00<br />
| 19-09-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_TOI_044-OFF_R2.xx_ODXXXX-full.fits<br />
| <br />
| <br />
| 00<br />
| 19-09-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_TOI_070-OFF_R2.xx_ODXXXX-full.fits<br />
| <br />
| <br />
|00<br />
| 19-09-2014 <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_TOI_030-OFF_R2.xx_ODXXXX-full-ringhalf.fits<br />
| <br />
| <br />
| 00<br />
| 11-11-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_TOI_044-OFF_R2.xx_ODXXXX-full-ringhalf.fits<br />
| <br />
| <br />
| 00<br />
| 11-11-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_TOI_070-OFF_R2.xx_ODXXXX-full-ringhalf.fits<br />
| <br />
| <br />
| 00<br />
| 11-11-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
|align="center"| HFI <br />
| HFI_TOI_AllFreqs-OFF_R2.xx.fits<br />
|<br />
|<br />
|00<br />
|13/01/2015<br />
|style="background-color: green;" |<br />
|style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan=9| <span style="color:Blue">Pointing</span><br />
| align="center" rowspan="3"| LFI <br />
| LFI_TOI_030-PTG_R2.xx_ODXXXX.fits <br />
|<br />
| <br />
|00 <br />
|18-07-2014 <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_TOI_044-PTG_R2.xx_ODXXXX.fits <br />
|<br />
| <br />
| 00 <br />
| 18-07-2014 <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_TOI_070-PTG_R2.xx_ODXXXX.fits <br />
|<br />
| <br />
| 00 <br />
| 18-07-2014 <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| rowspan=6 align="center"| HFI <br />
| HFI_TOI_100-PTG_R2.xx_ODXXXX.fits <br />
|<br />
| <br />
| 01 <br />
| 26-08-2014 <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_TOI_143-PTG_R2.xx_ODXXXX.fits <br />
|<br />
| <br />
| 01 <br />
| 26-08-2014 <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_TOI_217-PTG_R2.xx_ODXXXX.fits <br />
|<br />
| <br />
| 01 <br />
| 26-08-2014 <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_TOI_353-PTG_R2.xx_ODXXXX.fits <br />
|<br />
| <br />
| 01 <br />
| 26-08-2014 <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_TOI_545-PTG_R2.xx_ODXXXX.fits <br />
|<br />
| <br />
| 01 <br />
| 26-08-2014 <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_TOI_857-PTG_R2.xx_ODXXXX.fits <br />
|<br />
| <br />
| 01 <br />
| 26-08-2014 <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="4"| <span style="color:Blue">Time stamps</span><br />
| align="center" rowspan="3"| LFI <br />
| LFI_TOI_030-TAI_R2.xx_ODXXXX.fits <br />
|<br />
| <br />
|00 <br />
| 20-09-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_TOI_044-TAI_R2.xx_ODXXXX.fits <br />
|<br />
| <br />
| 00 <br />
| 20-09-2014 <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_TOI_070-TAI_R2.xx_ODXXXX.fits <br />
|<br />
| <br />
| 00<br />
| 20-09-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| align="center"| HFI <br />
| HFI_TOI_AllFreqs-TAI_R2.xx_ODXXXX.fits <br />
|<br />
| <br />
| 00<br />
| 20-09-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan=8| <span style="color:Blue">HK</span> <br />
|align="center" rowspan="8"| LFI <br />
| LFI_TOI_DAE-FAST-HK_R2.XX_ODXXX.fits<br />
| <br />
| <br />
|00 <br />
|14-08-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| LFI_TOI_DAE-SlowConfiguration-HK_R2.XX_ODXXXX.fits<br />
| <br />
| <br />
|00 <br />
|14-08-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| LFI_TOI_DAE-SlowCurrent-HK_R2.XX_ODXXXX.fits<br />
| <br />
| <br />
|00 <br />
|14-08-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| LFI_TOI_DAE-SlowPhaseSwitch-HK_R2.XX_ODXXXX.fits<br />
| <br />
| <br />
|00 <br />
|14-08-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" | <br />
| <br />
|<br />
|-<br />
| LFI_TOI_DAE-SlowVoltage-HK_R2.XX_ODXXXX.fits<br />
| <br />
| <br />
|00 <br />
|14-08-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" | <br />
| <br />
|<br />
|-<br />
| LFI_TOI_REBA-HK_R2.XX_ODXXXX.fits<br />
| <br />
| <br />
|00 <br />
|14-08-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" | <br />
| <br />
|<br />
|-<br />
| SCS_TOI_EssentialASW(R)-HK_R2.XX_ODXXXX.fits<br />
| <br />
| <br />
|00 <br />
|14-08-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" | <br />
| <br />
| <br />
|-<br />
| SCS_TOI_NonEssentialASW(R)-HK_R2.XX_ODXXXX.fits<br />
| <br />
| <br />
|00 <br />
|14-08-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" | <br />
| <br />
| <br />
|-<br />
|}<br />
<br />
===Maps===<br />
====Sky Maps====<br />
=====All detectors=====<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=1050px<br />
|+ '''All Detectors'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" rowspan="56" | Survey maps<br />
| rowspan="32" align="center"| LFI<br />
| LFI_SkyMap_030_1024_R2.xx_survey-1.fits<br />
| <br />
| <br />
| 01<br />
| 26/01/2015<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_030_1024_R2.xx_survey-2.fits<br />
| <br />
| <br />
| 01<br />
| <br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_030_1024_R2.xx_survey-3.fits<br />
| <br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_030_1024_R2.xx_survey-4.fits<br />
| <br />
| <br />
|01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_030_1024_R2.xx_survey-5.fits<br />
| <br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_030_1024_R2.xx_survey-6.fits<br />
| <br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_030_1024_R2.xx_survey-7.fits<br />
| <br />
|<br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_030_1024_R2.xx_survey-8.fits<br />
| <br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_survey-1.fits<br />
| <br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_survey-2.fits<br />
| <br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_survey-3.fits<br />
| <br />
|<br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_survey-4.fits<br />
|<br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_survey-5.fits<br />
| <br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_survey-6.fits<br />
| <br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_survey-7.fits<br />
| <br />
|<br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_survey-8.fits<br />
| <br />
|<br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_survey-1.fits<br />
|<br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_survey-2.fits<br />
| <br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_survey-3.fits<br />
| <br />
| <br />
|01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_survey-4.fits<br />
| <br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_survey-5.fits<br />
| <br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_survey-6.fits<br />
| <br />
|<br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_survey-7.fits<br />
| <br />
|<br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_survey-8.fits<br />
| <br />
|<br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_2048_R2.xx_survey-1.fits<br />
| <br />
|<br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_2048_R2.xx_survey-2.fits<br />
| <br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_2048_R2.xx_survey-3.fits<br />
| <br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_2048_R2.xx_survey-4.fits<br />
| <br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_2048_R2.xx_survey-5.fits<br />
| <br />
|<br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_2048_R2.xx_survey-6.fits<br />
|<br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_2048_R2.xx_survey-7.fits<br />
| <br />
| <br />
| 01<br />
|<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_2048_R2.xx_survey-8.fits<br />
| <br />
| <br />
| 01<br />
|<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| rowspan="24" align="center"| HFI<br />
| HFI_SkyMap_100_2048_R2.xx_survey-1.fits<br />
| <br />
|<br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_100_2048_R2.xx_survey-2.fits<br />
| <br />
|<br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_100_2048_R2.xx_survey-3.fits<br />
| <br />
|<br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_100_2048_R2.xx_survey-4.fits<br />
| <br />
| <br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_143_2048_R2.xx_survey-1.fits<br />
| <br />
| <br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_143_2048_R2.xx_survey-2.fits<br />
|<br />
| <br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_143_2048_R2.xx_survey-3.fits<br />
| <br />
| <br />
|00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_143_2048_R2.xx_survey-4.fits<br />
| <br />
|<br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_217_2048_R2.xx_survey-1.fits<br />
| <br />
| <br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_217_2048_R2.xx_survey-2.fits<br />
| <br />
| <br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_217_2048_R2.xx_survey-3.fits<br />
| <br />
|<br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_217_2048_R2.xx_survey-4.fits<br />
| <br />
|<br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_353_2048_R2.xx_survey-1.fits<br />
| <br />
| <br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_353_2048_R2.xx_survey-2.fits<br />
| <br />
|<br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_353_2048_R2.xx_survey-3.fits<br />
| <br />
| <br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_353_2048_R2.xx_survey-4.fits<br />
| <br />
| <br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_545_2048_R2.xx_survey-1.fits<br />
| <br />
| <br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_545_2048_R2.xx_survey-2.fits<br />
| <br />
|<br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_545_2048_R2.xx_survey-3.fits<br />
| <br />
| <br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_545_2048_R2.xx_survey-4.fits<br />
| <br />
| <br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_857_2048_R2.xx_survey-1.fits<br />
| <br />
| <br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_857_2048_R2.xx_survey-2.fits<br />
|<br />
| <br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_857_2048_R2.xx_survey-3.fits<br />
| <br />
| <br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_857_2048_R2.xx_survey-4.fits<br />
| <br />
| <br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="28" | <span style="color:Blue">1 year maps</span> <br />
1 year = 2 surveys<br />
<br />
y1=s1+s2<br />
<br />
y2=s3+s4<br />
<br />
y3=s5+s6<br />
<br />
y4=s7+s8<br />
| rowspan="16" align="center" | LFI<br />
| LFI_SkyMap_030_1024_R2.xx_year-1.fits<br />
| <br />
|<br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_030_1024_R2.xx_year-2.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_030_1024_R2.xx_year-3.fits<br />
| <br />
|<br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_030_1024_R2.xx_year-4.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_year-1.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_year-2.fits<br />
| <br />
| <br />
|00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_year-3.fits<br />
| <br />
|<br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_year-4.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_year-1.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_year-2.fits<br />
| <br />
|<br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_year-3.fits<br />
| <br />
|<br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_year-4.fits<br />
| <br />
| <br />
|00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_2048_R2.xx_year-1.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_2048_R2.xx_year-2.fits<br />
| <br />
|<br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_2048_R2.xx_year-3.fits<br />
| <br />
|<br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_2048_R2.xx_year-4.fits<br />
| <br />
| <br />
|00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| rowspan="12" align="center" | HFI<br />
| HFI_SkyMap_100_2048_R2.xx_year-1.fits<br />
| <br />
| <br />
| 00 <br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_100_2048_R2.xx_year-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_143_2048_R2.xx_year-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_143_2048_R2.xx_year-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_217_2048_R2.xx_year-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_217_2048_R2.xx_year-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_353_2048_R2.xx_year-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_353_2048_R2.xx_year-2.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_545_2048_R2.xx_year-1.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_545_2048_R2.xx_year-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_857_2048_R2.xx_year-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_857_2048_R2.xx_year-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="12" | <span style="color:Blue">Half mission maps</span><br />
| rowspan="12" align="center"| HFI<br />
| HFI_SkyMap_100_2048_R2.xx_halfmission-1.fits<br />
| <br />
| <br />
| 00 <br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_100_2048_R2.xx_halfmission-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_143_2048_R2.xx_halfmission-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_143_2048_R2.xx_halfmission-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_217_2048_R2.xx_halfmission-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_217_2048_R2.xx_halfmission-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_353_2048_R2.xx_halfmission-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_353_2048_R2.xx_halfmission-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_545_2048_R2.xx_halfmission-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_545_2048_R2.xx_halfmission-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_857_2048_R2.xx_halfmission-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_857_2048_R2.xx_halfmission-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="12" | <span style="color:Blue">Multi year maps</span><br />
| rowspan="12" align="center"| LFI<br />
| LFI_SkyMap_030_1024_R2.xx_year-1-2.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_030_1024_R2.xx_year-1-3.fits<br />
| <br />
| <br />
| 00<br />
| 21/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_030_1024_R2.xx_year-2-4.fits<br />
| <br />
| <br />
| 00<br />
| 21/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_030_1024_R2.xx_year-3-4.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_year-1-2.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_year-1-3.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_year-2-4.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_year-3-4.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_year-1-2.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_year-1-3.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_year-2-4.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_year-3-4.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="20" | Half-ring maps <br />
| rowspan="8" align="center" | LFI <br />
| LFI_SkyMap_030_1024_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
|00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_030_1024_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| rowspan="12" align="center" | HFI <br />
| HFI_SkyMap_100_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_100_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_143_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_143_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_217_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_217_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_353_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_353_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_545_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_545_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_857_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_857_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="10" | Frequency Maps <br />
| rowspan="4" align="center" | LFI <br />
| LFI_SkyMap_030_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| rowspan="6" align="center" | HFI <br />
| HFI_SkyMap_100_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_143_2048_R2.xx_full.fits<br />
| <br />
|<br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_217_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_353_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_545_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_857_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" | Zodi correction maps <br />
| align="center" | HFI <br />
| HFI_CorrMap_<Freq>-Zodi_2048_R2.xx_<Coverage>.fits<br />
| <br />
| <br />
| 00<br />
| 16/12/2014<br />
| style="background-color: green;" |<br />
|style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
|}<br />
<br />
=====Detector maps=====<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=950px<br />
|+ '''HFI detector maps/LFI radiometer maps'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" rowspan="40" | <span style="color:Blue">Full mission</span><br />
| rowspan="22" align="center" | LFI<br />
| LFI_SkyMap_030-27M_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_030-27S_1024_R2.xx_full.fits<br />
| <br />
| <br />
|00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_030-28M_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_030-28S_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_044-24M_1024_R2.xx_full.fits<br />
| <br />
|<br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
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!bgcolor="ffdead" scope="row" rowspan="80" | <span style="color:Blue">Half rings</span><br />
| rowspan="44" align="center" | LFI<br />
| LFI_SkyMap_030-27M_1024_R2.xx_full-ringhalf-1.fits<br />
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| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_070-21S_1024_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
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| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
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|-<br />
| LFI_SkyMap_070-21S_1024_R2.xx_full-ringhalf-2.fits<br />
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| 00<br />
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| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_070-22M_1024_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
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| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
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| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_070-22M_1024_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
|00<br />
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| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
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| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_070-22S_1024_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
|00<br />
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| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
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| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_070-22S_1024_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
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| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_070-23M_1024_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_070-23M_1024_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
|00<br />
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| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_070-23S_1024_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
|00<br />
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| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
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| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_070-23S_1024_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
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| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| rowspan="36" align="center" | HFI<br />
| HFI_SkyMap_143-5_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
|style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_143-5_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
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|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_143-6_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
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| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
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| HFI_SkyMap_143-6_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
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|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_143-7_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
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| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
|| HFI_SkyMap_143-7_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
|<br />
| 00 <br />
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| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_217-1_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_217-1_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_217-2_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
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|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
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| [[#note8|[8]]][[#note9|[9]]]<br />
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| HFI_SkyMap_217-2_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
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| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_217-3_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
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|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_217-3_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
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| style="background-color: green;" |<br />
|style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_217-4_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
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| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_217-4_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
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|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_353-1_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
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| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_353-1_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_353-2_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
|00<br />
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| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_353-2_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_353-7_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
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|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_353-7_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
|<br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_353-8_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_353-8_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_545-1_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_545-1_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_545-2_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_545-2_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_545-4_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_545-4_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_857-1_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
|00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_857-1_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_857-2_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_857-2_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_857-3_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
|00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_857-3_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_857-4_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_857-4_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|}<br />
<br />
=====Detector set maps=====<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=1050px<br />
|+ '''Detector set maps'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" rowspan="16" | <span style="color:Blue">Full mission</span><br />
| rowspan="8" align="center" | LFI<br />
| LFI_SkyMap_044-24_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| [[#note12|[12]]]<br />
|-<br />
| LFI_SkyMap_044-25-26_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| [[#note12|[12]]]<br />
|-<br />
| LFI_SkyMap_070-18-23_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note12|[12]]]<br />
|-<br />
| LFI_SkyMap_070-19-22_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note12|[12]]]<br />
|-<br />
| LFI_SkyMap_070-20-21_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note12|[12]]]<br />
|-<br />
| LFI_SkyMap_070-18-23_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note12|[12]]]<br />
|-<br />
| LFI_SkyMap_070-19-22_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note12|[12]]]<br />
|-<br />
| LFI_SkyMap_070-20-21_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note12|[12]]]<br />
|-<br />
| rowspan="8" align="center" | HFI<br />
| HFI_SkyMap_100-ds1_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_100-ds2_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_143-ds1_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_143-ds2_2048_R2.xx_full.fits<br />
| <br />
| <br />
|00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_217-ds1_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_217-ds2_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_353-ds1_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_353-ds2_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="26" | <span style="color:Blue">Half rings</span><br />
| rowspan="10" align="center" | LFI<br />
| LFI_SkyMap_044-24_1024_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044-24_1024_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044-25-26_1024_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044-25-26_1024_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070-18-23_1024_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
|00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070-18-23_1024_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070-19-22_1024_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070-19-22_1024_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070-20-21_1024_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070-20-21_1024_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| rowspan="16" align="center" | HFI<br />
| HFI_SkyMap_100-ds1_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
|<br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_100-ds1_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_100-ds2_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_100-ds2_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_143-ds1_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_143-ds1_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
|style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_143-ds2_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_143-ds2_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_217-ds1_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
|00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
|| HFI_SkyMap_217-ds1_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
|00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_217-ds2_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_217-ds2_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_353-ds1_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_353-ds1_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_353-ds2_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_353-ds2_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|}<br />
<br />
=====Low resolution maps=====<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=950px<br />
|+ '''Low resolution maps (with noise cov. mat.)'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" rowspan="2"|Low resolution maps (with noise cov. mat.)<br />
| align="center" | LFI<br />
| LFI_SkyMap_fff_0016_R2.xx_full.fits<br />
| <br />
| <br />
|00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| align="center" | HFI <br />
| HFI_SkyMap_fff_0016_R2.xx_full.fits<br />
| Not for PR2<br />
| <br />
| 01<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|}<br />
<br />
=====Correction maps=====<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=1300px<br />
|+ '''Correction maps'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" rowspan="1"| <span style="color:Red">A correction maps</span><br />
| rowspan="10" align="center" | LFI<br />
| <strike>LFI_CorrMap_030-ACorr_NSNS_R2.xx_full.fits</strike><br />
| <br />
| <br />
| <br />
| <br />
|<br />
| <br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="9"| <span style="color:Blue">Band pass correction<br>maps</span><br />
| LFI_CorrMap_030-BPassCorr_0256_R2.xx_full.fits<br />
| <br />
| <br />
|00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_CorrMap_044-BPassCorr_0256_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
| LFI_CorrMap_070-BPassCorr_0256_R2.xx_full.fits<br />
| <br />
| <br />
|00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_CorrMap_030-BPassCorr_0128_R2.xx_full.fits<br />
| <br />
| <br />
|00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_CorrMap_044-BPassCorr_0128_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
| LFI_CorrMap_070-BPassCorr_0128_R2.xx_full.fits<br />
| <br />
| <br />
|00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_CorrMap_030-BPassCorr_0064_R2.xx_full.fits<br />
| <br />
| <br />
|00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_CorrMap_044-BPassCorr_0064_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
| LFI_CorrMap_070-BPassCorr_0064_R2.xx_full.fits<br />
| <br />
| <br />
|00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="12"| <span style="color:Blue">Dust correction<br>maps</span><br />
| rowspan="12" align="center" |HFI <br />
| HFI_CorrMap 353 GHz leakage global fits maps<br />
| <br />
| <br />
| 00<br />
| 09/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| <strike>HFI_CorrMap_100-dustleak-ground_2048_R2.xx_full.fits</strike><br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
|<br />
|-<br />
| <strike>HFI_CorrMap_353-dustleak-diff_2048_R2.xx_full.fits</strike><br />
| <br />
| <br />
| <br />
| <br />
|<br />
| <br />
| <br />
| <br />
|-<br />
| HFI_CorrMap_353-dustleak-ground_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
|24/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| <strike>HFI_CorrMap_353_dustleak-diff_2048_R2.xx_year-1.fits</strike><br />
| <br />
| <br />
| <br />
|<br />
| <br />
| <br />
| <br />
| <br />
|-<br />
| <strike>HFI_CorrMap_353_dustleak-diff_2048_R2.xx_year-2.fits</strike><br />
| <br />
| <br />
| <br />
| <br />
|<br />
| <br />
| <br />
| <br />
|-<br />
| HFI_CorrMap_353_dustleak-ground_2048_R2.xx_year-1.fits<br />
| <br />
| <br />
| 00<br />
| 24/11/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_CorrMap_353_dustleak-ground_2048_R2.xx_year-2.fits<br />
| <br />
| <br />
| 00<br />
| 24/11/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| <strike>HFI_CorrMap_353-ds1-dustleak-diff_2048_R2.xx_full.fits</strike><br />
| <br />
|<br />
| <br />
| <br />
| <br />
| <br />
| <br />
|<br />
|-<br />
| <strike>HFI_CorrMap_353-ds2-dustleak-diff_2048_R2.xx_full.fits</strike><br />
| <br />
| <br />
| <br />
|<br />
| <br />
| <br />
| <br />
| <br />
|-<br />
| HFI_CorrMap_353-ds1-dustleak-ground_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 24/11/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_CorrMap_353-ds2-dustleak-ground_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 24/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="1"| <span style="color:Blue">CO correction<br>maps</span><br />
| rowspan="1" align="center" | HFI <br />
| <strike>HFI_CorrMap_<freq>-coleak-'''METHOD1'''_2048_R2.xx_full.fits</strike><br />
| <br />
| <br />
| <br />
| <br />
|<br />
| <br />
| <br />
| <br />
|}<br />
<br />
====Covariance matrices====<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=850px<br />
|+ '''Covariance matrices'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" rowspan="4"| Cov. Matrices<br />
| style="text-align:center" rowspan="4"| HFI+LFI<br />
| LFI_NoiseCovMat_030_0016_R2.xx.tgz<br />
| <br />
| <br />
|00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| LFI_NoiseCovMat_044_0016_R2.xx.tgz<br />
| <br />
| <br />
| 00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_NoiseCovMat_070_0016_R2.xx.tgz<br />
| <br />
| <br />
| 00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI covariance matrices<br />
| Not for PR2<br />
| <br />
| 01<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|}<br />
<br />
====CMB maps====<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=1050px<br />
|+ '''CMB Maps'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" rowspan="6" | CMB anisotropy maps<br />
| rowspan="6" align="center" | COM<br />
| COM_CMB_IQU-nilc-field-X_Nside_R2.xx.fits<br />
| <br />
|<br />
|00 <br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_CMB_IQU-sevem-field-X_Nside_R2.xx.fits<br />
| <br />
| <br />
| 00<br />
|09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| COM_CMB_IQU-smica-field-X_Nside_R2.xx.fits<br />
| <br />
| <br />
| 00<br />
|09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_CMB_IQU-commander-field-X_Nside_R2.xx.fits<br />
| <br />
| <br />
| 00<br />
| 09/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| <strike>COM_CMB_IQU-commrul_0256_R2.xx.fits</strike><br />
| <br />
| <br />
| <br />
|<br />
| <br />
| <br />
| <br />
| <br />
|-<br />
| <span style="color:Red"><strike>Other representations</strike></span><br />
| <br />
| <br />
| <br />
|<br />
| <br />
| <br />
| <br />
| <br />
|-<br />
|}<br />
<br />
====Component maps====<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=950px<br />
|+ '''Component Maps'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" rowspan="3" | CO maps<br />
| align="center" rowspan="3"| HFI<br />
| HFI_CompMap_CO-Type1_2048_R2.xx.fits<br />
| <br />
|<br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_CompMap_CO-Type2_2048_R2.xx.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| <strike>HFI_CompMap_CO-Type3_2048_R2.xx.fits</strike><br />
| <br />
| <br />
| <br />
|<br />
| <br />
| <br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="12" | Commander foregrounds<br />
| align="center" rowspan="12"| COM<br />
| COM_CompMap_AME-commander_0256_R2.xx.fits<br />
|<br />
|<br />
| 00<br />
| 11/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| COM_CompMap_CMB-commander_0256_R2.xx.fits<br />
|<br />
|<br />
| 00<br />
| 11/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| COM_CompMap_CO21-commander_2048_R2.xx.fits<br />
|<br />
|<br />
| 00<br />
| 11/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| COM_CompMap_CO-commander_0256_R2.xx.fits<br />
|<br />
|<br />
| 00<br />
| 11/12/2014<br />
| style="background-color: green;" |<br />
|style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_CompMap_dust-commander_0256_R2.xx.fits<br />
|<br />
|<br />
| 00<br />
| 11/12/2014<br />
| style="background-color: green;" |<br />
|style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_CompMap_DustPol-commander_1024_R2.xx.fits<br />
|<br />
|<br />
| 00<br />
| 11/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_CompMap_freefree-commander_0256_R2.xx.fits<br />
|<br />
|<br />
| 00<br />
| 11/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| COM_CompMap_Synchrotron-commander_0256_R2.xx.fits<br />
|<br />
|<br />
| 00<br />
| 11/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| COM_CompMap_SynchrotronPol-commander_0256_R2.xx.fits<br />
|<br />
|<br />
| 00<br />
| 11/12/2014<br />
| style="background-color: green;" |<br />
|style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_CompMap_SZ-commander_0256_R2.xx.fits<br />
|<br />
|<br />
| 00<br />
| 11/12/2014<br />
| style="background-color: green;" |<br />
|style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_CompMap_ThermalDust-commander_2048_R2.xx.fits<br />
|<br />
|<br />
| 00<br />
| 11/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_CompMap_xline-commander_0256_R2.xx.fits<br />
|<br />
|<br />
| 00<br />
| 11/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" | Lensing maps<br />
| align="center" | COM<br />
| COM_CompMap_Lensing_2048_R2.xx.tar + SimMap tars<br />
|<br />
| <br />
|00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
|}<br />
<br />
====Masks====<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=850px<br />
|+ '''Masks'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" rowspan='4'| Masks<br />
| style="text-align:center" | <strike>LFI</strike><br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
|-<br />
| style="text-align:center" | HFI<br />
| HFI_Mask_GalPlane-apo 0 2 5 _2048_R2.xx.fits<br />
|<br />
| <br />
| 00<br />
| 19/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| style="text-align:center" rowspan='2'| COM<br />
| COM_CMB_IQU-common-field-MaskInt_2048_R2.xx.fits<br />
| <br />
|<br />
| 00<br />
| 10/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_CMB_IQU-common-field-MaskPol_1024_R2.xx.fits<br />
| <br />
| <br />
| 00<br />
| 10/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan='2'| Point source masks<br />
| style="text-align:center" rowspan='1'| LFI<br />
| LFI_Mask_PointSrc_2048_R2.xx.fits<br />
| <br />
| <br />
| 00<br />
|27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| style="text-align:center" | HFI<br />
| HFI_Mask_PointSrc_2048_R2.xx.fits<br />
| <br />
| <br />
|00<br />
| 19/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
|}<br />
<br />
===Angular power spectra===<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=1050px<br />
|+ '''Angular power spectra'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" rowspan="2" | CMB angular power spectra<br />
| style="text-align:center" rowspan="2" |COM<br />
| COM_PowerSpect_CMB_R2.xx.fits<br />
|<br />
| <br />
| 00<br />
| 05/02/2015<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| <strike>COM_PowerSpect_CMB_R2.xx.txt</strike><br />
|<br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="1"| <strike>Sky Angular power spectrum</strike><br />
| style="text-align:center" rowspan="4" |<br />
| <strike>LFI_PowerSpect_030_R2.xx.fits</strike><br />
|<br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
| [[#note37|[37]]]<br />
|-<br />
|}<br />
<div id="note37"></div>[37] For this release detector and detector set power spectra will not be provided. Instead the detector and detector set maps will be provided.<br />
<br />
===Characterisation===<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=850px<br />
|+ '''Characterization'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" rowspan="3"| RIMO<br />
| style="text-align:center" | LFI<br />
| LFI_RIMO_R2.xx.fits<br />
| <br />
| <br />
|50<br />
| 16/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| style="text-align:center" | HFI<br />
| HFI_RIMO_R2.xx.fits<br />
| <br />
| <br />
| 00<br />
| 20/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| style="text-align:center" | HFI<br />
| HFI beams RIMO(s)<br />
| <br />
| <br />
| 00<br />
| 05/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
|}<br />
<br />
===Catalogues===<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=850px<br />
|+ '''Catalogues'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" rowspan="9"| PCCS<br />
| style="text-align:center" rowspan="9"| COM<br />
| COM_PCCS_030_R2.xx.fits + excl.<br />
| <br />
| <br />
| 02<br />
|15/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_PCCS_044_R2.xx.fits + excl.<br />
| <br />
| <br />
| 02<br />
|15/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_PCCS_070_R2.xx.fits + excl.<br />
| <br />
| <br />
| 02<br />
| 15/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_PCCS_100_R2.xx.fits<br />
| <br />
| <br />
| 01<br />
| 19/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_PCCS_143_R2.xx.fits<br />
| <br />
| <br />
| 01<br />
| 19/11/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_PCCS_217_R2.xx.fits<br />
| <br />
| <br />
|01<br />
| 19/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_PCCS_353_R2.xx.fits<br />
| <br />
| <br />
| 01<br />
| 19/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_PCCS_545_R2.xx.fits<br />
| <br />
| <br />
| 01<br />
|19/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_PCCS_857_R2.xx.fits<br />
| <br />
| <br />
| 01<br />
|19/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="4"| SZ catalogues<br />
| style="text-align:center" rowspan="4"| COM<br />
| COM_PCCS_SZ-MMF1_R2.xx.fits<br />
| <br />
| <br />
| 08<br />
| 29/01/2015<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_PCCS_SZ-MMF3_R2.xx.fits<br />
| <br />
| <br />
| 08<br />
| 29/01/2015<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
|<br />
|-<br />
| COM_PCCS_SZ-PwS_R2.xx.fits<br />
| <br />
| <br />
| 08<br />
| 29/01/2015<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_PCCS_SZ-union_R2.xx.fits<br />
| <br />
| <br />
| 08<br />
| 03/02/2015<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
|<br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="4"| Other catalogues<br />
| style="text-align:center" rowspan="4"| HFI<br />
| <span style="color:Red"><strike>Dusty source catalogue</strike></span><br />
| <br />
| <br />
|<br />
| <br />
| <br />
| <br />
| <br />
| <br />
|-<br />
| <span style="color:Red"><strike>Radio sources catalogue</strike></span><br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
|-<br />
| <span style="color:Blue">HFI_PCCS_GCC_R2.xx.fits</span><br />
| <br />
| <br />
| 02<br />
| 16/01/2015<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| <span style="color:Blue">High-z catalogue</span><br />
| <br />
| <br />
| <br />
| <br />
|<br />
| <br />
| <br />
| <br />
|-<br />
|}<br />
<br />
===Other products===<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=850px<br />
|+ '''Other products'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" | Cosmological parameters<br />
| style="text-align:center" rowspan="1"| COM<br />
| Cosmological parameter tables<br />
| <br />
| <br />
| 00<br />
| 28/01/2015<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="1"| Codes<br />
| style="text-align:center" rowspan="1"| COM<br />
| Likelihood code<br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
|<br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="11"| Beams<br />
| style="text-align:center" rowspan="5"| <br />
| LFI scanning beams<br />
| <br />
| <br />
| 00<br />
| 21-11-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
| HFI scanning beams<br />
| <br />
| <br />
| 00<br />
| 05/02/2015<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
| Effective beams 30GHz<br />
| <br />
| <br />
| <br />
| 22-09-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
| Effective beams 44GHz<br />
| <br />
| <br />
| <br />
| 24-09-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
| Effective beams 70GHz<br />
| <br />
| <br />
| <br />
| 24-09-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
| style="text-align:center" rowspan="6"| <br />
| Effective beams 100 GHz<br />
| <br />
| <br />
| <br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
| Effective beams 143 GHz<br />
| <br />
| <br />
| <br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
| Effective beams 217 GHz<br />
| <br />
| <br />
| <br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
| Effective beams 353 GHz<br />
| <br />
| <br />
| <br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
| Effective beams 545 GHz<br />
| <br />
| <br />
| <br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
| Effective beams 857 GGz<br />
| <br />
| <br />
| <br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="2"| 4D maps<br />
| style="text-align:center" rowspan="2"| LFI<br />
| Code<br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
|<br />
| [[#noteA|[A]]]<br />
|-<br />
| map4D_calib_DDX11_LFIXX_gal_nsideXXX_npsiXXXX.fits<br />
| <br />
| <br />
| <br />
| 19/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| [[#noteA|[A]]]<br />
|-<br />
!bgcolor="ffdead" scope="row" | Datesobs<br />
| USPDC<br />
| HFI_DatesObs_<Freq>_2048_R2.xx_surveyX.fits.gz<br />
| <br />
| <br />
| 01<br />
|29/01/2015<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" | YSZ package<br />
| COM<br />
| COM_CompMap_YSZ_R2.nn.fits.tgz<br />
| <br />
| 12 Gb<br />
|00<br />
| 05/02/2015<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
|}<br />
<div id="noteA"></div>[A] '''This is not an official product.'''</div>
Xdupac
https://wiki.cosmos.esa.int/planckpla2015/index.php?title=Effective_Beams&diff=11422
Effective Beams
2015-02-05T10:37:20Z
<p>Xdupac: </p>
<hr />
<div>{{DISPLAYTITLE:2015 Effective Beams}}<br />
<span style="color:red"></span><br />
<br />
==Product description==<br />
The '''effective beam''' is the average of all scanning beams pointing at a certain direction within a given pixel of the sky map for a given scan strategy. It takes into account the coupling between azimuthal asymmetry of the beam and the uneven distribution of scanning angles across the sky.<br />
It captures the complete information about the difference between the true and observed image of the sky. The effective beams are, by definition, the objects whose convolution with the true CMB sky produce the observed sky map. <br />
<br />
Details of the beam processing are given in the respective pages for [[Beams|HFI]] and [[Beams_LFI|LFI]].<br />
<br />
The full algebra involving the effective beams for temperature and polarisation was presented in {{BibCite|mitra2010}}, and a discussion of its application to Planck data is given in the appropriate LFI {{PlanckPapers|planck2013-p02d}}, {{PlanckPapers|planck2014-a05||Planck-2015-A05}} and HFI {{PlanckPapers|planck2013-p03c}} papers. Relevant details of the processing steps are given in the [[Beams|Effective Beams]] section of this document.<br />
<br />
<!-- Everything from here down to the "Production Process" section should eventually be moved to a new section the Joint Processing pages --><br />
<br />
===Comparison of the images of compact sources observed by Planck with FEBeCoP products===<br />
We show here a comparison of the FEBeCoP-derived effective beams, and associated point spread functions, PSF (the transpose of the beam matrix), to the actual images of a few compact sources observed by Planck, for all LFI and HFI frequency channels, as an example. We show below a few panels of source images organized as follows:<br />
* Row #1- DX9 images of four ERCSC objects with their galactic (l,b) coordinates shown under the color bar<br />
* Row #2- linear scale FEBeCoP PSFs computed using input scanning beams, Grasp Beams, GB, for LFI and B-Spline beams,BS, Mars12 apodized for the CMB channels and the BS Mars12 for the sub-mm channels, for HFI (see section Inputs below).<br />
* Row #3- log scale of #2; PSF iso-contours shown in solid line, elliptical Gaussian fit iso-contours shown in broken line<br />
<br />
<center><br />
<br />
<gallery widths=400px heights=400px perrow=2 caption="Comparison images of compact sources and effective beams, PSFs"><br />
File:30.png| '''30GHz'''<br />
File:44.png| '''44GHz'''<br />
File:70.png| '''70GHz'''<br />
File:100.png| '''100GHz'''<br />
File:143.png| '''143GHz'''<br />
File:217.png| '''217GHz'''<br />
File:353.png| '''353GHz'''<br />
File:545.png| '''545GHz'''<br />
File:857.png| '''857GHz'''<br />
</gallery><br />
</center><br />
<br />
===Histograms of the effective beam parameters===<br />
Here we present histograms of the three fit parameters - beam FWHM, ellipticity, and orientation with respect to the local meridian and of the beam solid angle. The sky is sampled (pretty sparsely) at 3072 directions which were chosen as HEALpix nside=16 pixel centers for HFI and at 768 directions which were chosen as HEALpix nside=8 pixel centers for LFI. These uniformly sample the sky.<br />
<br />
Where beam solid angle is estimated according to the definition: '''<math> 4 \pi \sum</math>(effbeam)/max(effbeam)'''<br />
i.e., <math> 4 \pi \sum(B_{ij}) / max(B_{ij}) </math><br />
<br />
<br />
[[File:ist_GB.png | 800px| thumb | center| '''Histograms for LFI effective beam parameters''' ]] <br />
[[File:ist_BS_Mars12.png | 800px| thumb | center| '''Histograms for HFI effective beam parameters''' ]]<br />
<br />
===Sky variation of effective beams solid angle and ellipticity of the best-fit Gaussian===<br />
* The discontinuities at the Healpix domain edges in the maps are a visual artifact due to the interplay of the discretized effective beam and the Healpix pixel grid.<br />
<br />
<br />
<gallery widths=300px heights=220px perrow=3 caption="Sky variation of effective beams ellipticity of the best-fit Gaussian"><br />
File:e_030_GB.png| '''ellipticity - 30GHz'''<br />
File:e_044_GB.png| '''ellipticity - 44GHz'''<br />
File:e_070_GB.png| '''ellipticity - 70GHz'''<br />
File:e_100_BS_Mars12.png| '''ellipticity - 100GHz'''<br />
File:e_143_BS_Mars12.png| '''ellipticity - 143GHz'''<br />
File:e_217_BS_Mars12.png| '''ellipticity - 217GHz'''<br />
File:e_353_BS_Mars12.png| '''ellipticity - 353GHz'''<br />
File:e_545_BS_Mars12.png| '''ellipticity - 545GHz'''<br />
File:e_857_BS_Mars12.png| '''ellipticity - 857GHz'''<br />
</gallery><br />
<br />
<br />
<gallery widths=300px heights=220px perrow=3 caption="Sky (relative) variation of effective beams solid angle of the best-fit Gaussian"><br />
File:solidarc_030_GB.png| '''beam solid angle (relative) variations wrt scanning beam - 30GHz'''<br />
File:solidarc_044_GB.png| '''beam solid angle (relative) variations wrt scanning beam - 44GHz'''<br />
File:solidarc_070_GB.png| '''beam solid angle (relative) variations wrt scanning beam - 70GHz'''<br />
File:solidarc_100_BS_Mars12.png| '''beam solid angle (relative) variations wrt scanning beam - 100GHz'''<br />
File:solidarc_143_BS_Mars12.png| '''beam solid angle (relative) variations wrt scanning beam - 143GHz'''<br />
File:solidarc_217_BS_Mars12.png| '''beam solid angle (relative) variations wrt scanning beam - 217GHz'''<br />
File:solidarc_353_BS_Mars12.png| '''beam solid angle (relative) variations wrt scanning beam - 353GHz'''<br />
File:solidarc_545_BS_Mars12.png| '''beam solid angle (relative) variations wrt scanning beam - 545GHz'''<br />
File:solidarc_857_BS_Mars12.png| '''beam solid angle (relative) variations wrt scanning beam - 857GHz'''<br />
</gallery><br />
<br />
<br />
<gallery widths=300px heights=220px perrow=3 caption="Sky (relative) variation of effective beams fwhm of the best-fit Gaussian"><br />
File:fwhm_030_GB.png| '''fwhm (relative) variations wrt scanning beam - 30GHz'''<br />
File:fwhm_044_GB.png| '''fwhm (relative) variations wrt scanning beam - 44GHz'''<br />
File:fwhm_070_GB.png| '''fwhm (relative) variations wrt scanning beam - 70GHz'''<br />
File:fwhm_100_BS_Mars12.png| '''fwhm (relative) variations wrt scanning beam - 100GHz'''<br />
File:fwhm_143_BS_Mars12.png| '''fwhm (relative) variations wrt scanning beam - 143GHz'''<br />
File:fwhm_217_BS_Mars12.png| '''fwhm (relative) variations wrt scanning beam - 217GHz'''<br />
File:fwhm_353_BS_Mars12.png| '''fwhm (relative) variations wrt scanning beam - 353GHz'''<br />
File:fwhm_545_BS_Mars12.png| '''fwhm (relative) variations wrt scanning beam - 545GHz'''<br />
File:fwhm_857_BS_Mars12.png| '''fwhm (relative) variations wrt scanning beam - 857GHz'''<br />
</gallery><br />
<br />
<br />
<gallery widths=300px heights=220px perrow=3 caption="Sky variation of effective beams <math>\psi</math> angle of the best-fit Gaussian"><br />
File:psi_030_GB.png| '''<math>\psi</math> - 30GHz'''<br />
File:psi_044_GB.png| '''<math>\psi</math> - 44GHz'''<br />
File:psi_070_GB.png| '''<math>\psi</math> - 70GHz'''<br />
File:psi_100_BS_Mars12.png| '''<math>\psi</math> - 100GHz'''<br />
File:psi_143_BS_Mars12.png| '''<math>\psi</math> - 143GHz'''<br />
File:psi_217_BS_Mars12.png| '''<math>\psi</math> - 217GHz'''<br />
File:psi_353_BS_Mars12.png| '''<math>\psi</math> - 353GHz'''<br />
File:psi_545_BS_Mars12.png| '''<math>\psi</math> - 545GHz'''<br />
File:psi_857_BS_Mars12.png| '''<math>\psi</math> - 857GHz'''<br />
</gallery><br />
<br />
<!--<br />
<gallery widths=500px heights=500px perrow=2 caption="Sky variation of effective beams solid angle and ellipticity of the best-fit Gaussian"><br />
File:e_030_GB.png| '''ellipticity - 30GHz'''<br />
File:solidarc_030_GB.png| '''beam solid angle (relative variations wrt scanning beam - 30GHz'''<br />
File:e_100_BS_Mars12.png| '''ellipticity - 100GHz'''<br />
File:solidarc_100_BS_Mars12.png| '''beam solid angle (relative variations wrt scanning beam - 100GHz'''<br />
</gallery><br />
--><br />
<br />
===Statistics of the effective beams computed using FEBeCoP===<br />
<br />
We tabulate the simple statistics of FWHM, ellipticity (e), orientation (<math> \psi</math>) and beam solid angle, (<math> \Omega </math>), for a sample of 3072 and 768 directions on the sky for HFI and LFI data respectively. Statistics shown in the Table are derived from the histograms shown above.<br />
<br />
* The derived beam parameters are representative of the DPC NSIDE 1024 and 2048 healpix maps (they include the pixel window function).<br />
* The reported FWHM_eff are derived from the beam solid angles, under a Gaussian approximation. These are best used for flux determination while the the Gaussian fits to the effective beam maps are more suited for source identification.<br />
<br />
<br />
<br />
{| border="1" cellpadding="5" cellspacing="0" align="center" style="text-align:center"<br />
|+ '''Statistics of the FEBeCoP Effective Beams Computed with the BS Mars12 apodized for the CMB channels and oversampled'''<br />
|-<br />
! '''frequency''' || '''mean(fwhm)''' [arcmin] || '''sd(fwhm)''' [arcmin] || '''mean(e)''' || '''sd(e)''' || '''mean(<math> \psi</math>)''' [degree] || '''sd(<math> \psi</math>)''' [degree] || '''mean(<math> \Omega </math>)''' [arcmin<math>^{2}</math>] || '''sd(<math> \Omega </math>)''' [arcmin<math>^{2}</math>] || '''FWHM_eff''' [arcmin] <br />
|-<br />
| 030 || 32.239 || 0.013 || 1.320 || 0.031 || -0.304 || 55.349 || 1189.513 || 0.842 || 32.34<br />
|-<br />
| 044 || 27.005 || 0.552 || 1.034 || 0.033 || 0.059 || 53.767 || 832.946 || 31.774 || 27.12<br />
|-<br />
| 070 || 13.252 || 0.033 || 1.223 || 0.026 || 0.587 || 55.066 || 200.742 || 1.027 || 13.31 <br />
|-<br />
| 100 || 9.651 || 0.014 || 1.186 || 0.023 || -0.024 || 55.400 || 105.778 || 0.311 || 9.66 <br />
|-<br />
| 143 || 7.248 || 0.015 || 1.036 || 0.009 || 0.383 || 54.130 || 59.954 || 0.246 || 7.27 <br />
|-<br />
| 217 || 4.990 || 0.025 || 1.177 || 0.030 || 0.836 || 54.999 || 28.447 || 0.271 || 5.01<br />
|-<br />
| 353 || 4.818 || 0.024 || 1.147 || 0.028 || 0.655 || 54.745 || 26.714 || 0.250 || 4.86<br />
|- <br />
| 545 || 4.682 || 0.044 || 1.161 || 0.036 || 0.544 || 54.876 || 26.535 || 0.339 || 4.84 <br />
|-<br />
| 857 || 4.325 || 0.055 || 1.393 || 0.076 || 0.876 || 54.779 || 24.244 || 0.193 || 4.63 <br />
|}<br />
<br />
<br />
<br />
<br />
====Beam solid angles for the PCCS====<br />
<br />
* <math>\Omega_{eff}</math> - is the mean beam solid angle of the effective beam, where beam solid angle is estimated according to the definition: '''<math>4 \pi \sum </math>(effbeam)/max(effbeam)''', i.e. as an integral over the full extent of the effective beam, i.e. <math> 4 \pi \sum(B_{ij}) / max(B_{ij}) </math>.<br />
<br />
* from <math>\Omega_{eff}</math> we estimate the <math>fwhm_{eff}</math>, under a Gaussian approximation - these are tabulated above<br />
** <math>\Omega^{(1)}_{eff}</math> is the beam solid angle estimated up to a radius equal to one <math>fwhm_{eff}</math> and <math>\Omega^{(2)}_{eff}</math> up to a radius equal to twice the <math>fwhm_{eff}</math>.<br />
*** These were estimated according to the procedure followed in the aperture photometry code for the PCCS: if the pixel centre does not lie within the given radius it is not included (so inclusive=0 in query disc).<br />
<br />
<br />
{|border="1" cellpadding="5" cellspacing="0" align="center" style="text-align:center"<br />
|+'''Band averaged beam solid angles'''<br />
| '''Band''' || '''<math>\Omega_{eff}</math>'''[arcmin<math>^{2}</math>] || '''spatial variation''' [arcmin<math>^{2}</math>] || '''<math>\Omega^{(1)}_{eff}</math>''' [arcmin<math>^{2}</math>]|| '''spatial variation-1''' [arcmin<math>^{2}</math>] || '''<math>\Omega^{(2)}_{eff}</math>''' [arcmin<math>^{2}</math>] || '''spatial variation-2''' [arcmin<math>^{2}</math>] <br />
|-<br />
|30 || 1189.513 || 0.842 || 1116.494 || 2.274 || 1188.945 || 0.847 <br />
|-<br />
| 44 || 832.946 || 31.774 || 758.684 || 29.701 || 832.168 || 31.811 <br />
|-<br />
| 70 || 200.742 || 1.027 || 186.260 || 2.300 || 200.591 || 1.027 <br />
|-<br />
| 100 || 105.778 || 0.311 || 100.830 || 0.410 || 105.777 || 0.311 <br />
|-<br />
| 143 || 59.954 || 0.246 || 56.811 || 0.419 || 59.952 || 0.246 <br />
|-<br />
| 217 || 28.447 || 0.271 || 26.442 || 0.537 || 28.426 || 0.271 <br />
|-<br />
| 353 || 26.714 || 0.250 || 24.827 || 0.435 || 26.653 || 0.250 <br />
|-<br />
| 545 || 26.535 || 0.339 || 24.287 || 0.455 || 26.302 || 0.337 <br />
|-<br />
| 857 || 24.244 || 0.193 || 22.646 || 0.263 || 23.985 || 0.191 <br />
|}<br />
<br />
==Production process==<br />
FEBeCoP, or Fast Effective Beam Convolution in Pixel space{{BibCite|mitra2010}}, is an approach to representing and computing effective beams (including both intrinsic beam shapes and the effects of scanning) that comprises the following steps:<br />
* identify the individual detectors' instantaneous optical response function (presently we use elliptical Gaussian fits of Planck beams from observations of planets; eventually, an arbitrary mathematical representation of the beam can be used on input)<br />
* follow exactly the Planck scanning, and project the intrinsic beam on the sky at each actual sampling position<br />
* project instantaneous beams onto the pixelized map over a small region (typically <2.5 FWHM diameter)<br />
* add up all beams that cross the same pixel and its vicinity over the observing period of interest<br />
*create a data object of all beams pointed at all N'_pix_' directions of pixels in the map at a resolution at which this precomputation was executed (dimension N'_pix_' x a few hundred)<br />
*use the resulting beam object for very fast convolution of all sky signals with the effective optical response of the observing mission<br />
<br />
<br />
Computation of the effective beams at each pixel for every detector is a challenging task for high resolution experiments. FEBeCoP is an efficient algorithm and implementation which enabled us to compute the pixel based effective beams using moderate computational resources. The algorithm used different mathematical and computational techniques to bring down the computation cost to a practical level, whereby several estimations of the effective beams were possible for all Planck detectors for different scan and beam models, as well as different lengths of datasets. <br />
<br />
<br />
===Pixel Ordered Detector Angles (PODA)===<br />
The main challenge in computing the effective beams is to go through the trillion samples, which gets severely limited by I/O. In the first stage, for a given dataset, ordered lists of pointing angles for each pixel - the Pixel Ordered Detector Angles (PODA) are made. This is an one-time process for each dataset. We used computers with large memory and used tedious memory management bookkeeping to make this step efficient.<br />
<br />
===effBeam===<br />
The effBeam part makes use of the precomputed PODA and unsynchronized reading from the disk to compute the beam. Here we tried to made sure that no repetition occurs in evaluating a trigonometric quantity.<br />
<br />
<br />
One important reason for separating the two steps is that they use different schemes of parallel computing. The PODA part requires parallelisation over time-order-data samples, while the effBeam part requires distribution of pixels among different computers.<br />
<br />
<br />
===Computational Cost===<br />
The computation of the effective beams has been performed at the NERSC Supercomputing Center. The table below shows the computation cost for FEBeCoP processing of the nominal mission.<br />
<br />
{|border="1" cellpadding="5" cellspacing="0" align="center" style="text-align:center"<br />
|+ '''Computational cost for PODA, Effective Beam and single map convolution. Wall-clock time is given as a guide, as found on the NERSC supercomputers.'''<br />
|-<br />
|Channel ||030 || 044 || 070 || 100 || 143 || 217 || 353 || 545 || 857<br />
|-<br />
|PODA/Detector Computation time (CPU hrs) || 85 || 100 || 250 || 500 || 500 || 500 || 500 || 500 || 500 <br />
|-<br />
|PODA/Detector Computation time (wall clock hrs) || 7 || 10 || 20 || 20 || 20 || 20 || 20 || 20 || 20<br />
|- <br />
|Beam/Channel Computation time (CPU hrs) || 900 || 2000 || 2300 || 2800 || 3800 || 3200 || 3000 || 900 || 1100<br />
|-<br />
|Beam/Channel Computation time (wall clock hrs) || 0.5 || 0.8 || 1 || 1.5 || 2 || 1.2 || 1 || 0.5 || 0.5<br />
|-<br />
|Convolution Computation time (CPU hr) || 1 || 1.2 || 1.3 || 3.6 || 4.8 || 4.0 || 4.1 || 4.1 || 3.7 <br />
|-<br />
|Convolution Computation time (wall clock sec) || 1 || 1 || 1 || 4 || 4 || 4 || 4 || 4 || 4 <br />
|-<br />
|Effective Beam Size (GB) || 173 || 123 || 28 || 187 || 182 || 146 || 132 || 139 || 124<br />
|}<br />
<br />
<br />
The computation cost, especially for PODA and Convolution, is heavily limited by the I/O capacity of the disc and so it depends on the overall usage of the cluster done by other users.<br />
<br />
==Inputs==<br />
In order to fix the convention of presentation of the scanning and effective beams, we show the classic view of the Planck focal plane as seen by the incoming CMB photon. The scan direction is marked, and the toward the center of the focal plane is at the 85 deg angle w.r.t spin axis pointing upward in the picture. <br />
<br />
<br />
[[File:PlanckFocalPlane.png | 500px| thumb | center|'''Planck Focal Plane''']]<br />
<br />
<br />
===The Focal Plane DataBase (FPDB)===<br />
The FPDB contains information on each detector, e.g., the orientation of the polarisation axis, different weight factors, (see the instrument [[The RIMO|RIMOs]]):<br />
<br />
*HFI - {{PLASingleFile|fileType=rimo|name=HFI_RIMO_R1.00.fits|link=The HFI RIMO}}<br />
*LFI - {{PLASingleFile|fileType=rimo|name=LFI_RIMO_R1.12.fits|link=The LFI RIMO}}<br />
<br />
<br />
<!--<br />
*HFI - LFI_RIMO_DX9_PTCOR6 - {{PLASingleFile|fileType=rimo|name=HFI_RIMO_R1.00.fits|link=The HFI RIMO}}<br />
*LFI - HFI-RIMO-3_16_detilt_t2_ptcor6.fits - {{PLASingleFile|fileType=rimo|name=LFI_RIMO_R1.12.fits|link=The LFI RIMO}}<br />
<br />
{{PLADoc|fileType=rimo|link=The Plank RIMOS}}<br />
--><br />
<br />
===The scanning strategy===<br />
The scanning strategy, the three pointing angle for each detector for each sample: Detector pointings for the nominal mission covers about 15 months of observation from Operational Day (OD) 91 to OD 563 covering 3 surveys and half.<br />
<br />
===The scanbeam===<br />
The scanbeam modeled for each detector through the observation of planets. Which was assumed to be constant over the whole mission, though FEBeCoP could be used for a few sets of scanbeams too.<br />
<br />
* LFI: [[Beams LFI#Main beams and Focalplane calibration|GRASP scanning beam]] - the scanning beams used are based on Radio Frequency Tuned Model (RFTM) smeared to simulate the in-flight optical response. <br />
* HFI: [[Beams#Scanning beams|B-Spline, BS]] based on 2 observations of Mars.<br />
<br />
(see the instrument [[The RIMO|RIMOs]]).<br />
<br />
<!--<br />
<br />
*HFI - LFI_RIMO_DX9_PTCOR6 - {{PLASingleFile|fileType=rimo|name=HFI_RIMO_R1.00.fits|link=The HFI RIMO}}<br />
*LFI - HFI-RIMO-3_16_detilt_t2_ptcor6.fits - {{PLASingleFile|fileType=rimo|name=LFI_RIMO_R1.12.fits|link=The LFI RIMO}}<br />
[[Beams LFI#Effective beams|LFI effective beams]]<br />
--><br />
<br />
===Beam cutoff radii===<br />
N times geometric mean of FWHM of all detectors in a channel, where N<br />
<br />
{|border="1" cellpadding="5" cellspacing="0" align="center" style="text-align:center"<br />
|+'''Beam cut off radius'''<br />
| '''channel''' || '''Cutoff Radii in units of fwhm''' || '''fwhm of full beam extent''' <br />
|-<br />
|30 - 44 - 70 || 2.5 ||<br />
|-<br />
|100 || 2.25 || 23.703699<br />
|-<br />
|143 || 3 || 21.057402<br />
|-<br />
|217-353 || 4 || 18.782754<br />
|-<br />
|sub-mm || 4 || 18.327635(545GHz) ; 17.093706(857GHz) <br />
|}<br />
<br />
===Map resolution for the derived beam data object===<br />
* <math>N_{side} = 1024 </math> for LFI frequency channels<br />
* <math>N_{side} = 2048 </math> for HFI frequency channels<br />
<br />
==Related products==<br />
===Monte Carlo simulations===<br />
<br />
FEBeCoP software enables fast, full-sky convolutions of the sky signals with the Effective beams in pixel domain. Hence, a large number of Monte Carlo simulations of the sky signal maps map convolved with realistically rendered, spatially varying, asymmetric Planck beams can be easily generated. We performed the following steps:<br />
<br />
* generate the effective beams with FEBeCoP for all frequencies for dDX9 data and Nominal Mission<br />
* generate 100 realizations of maps from a fiducial CMB power spectrum<br />
* convolve each one of these maps with the effective beams using FEBeCoP<br />
* estimate the average of the Power Spectrum of each convolved realization, and 1 <math>\sigma</math> errors<br />
<br />
<br />
As FEBeCoP enables fast convolutions of the input signal sky with the effective beam, thousands of simulations are generated. These Monte Carlo simulations of the signal (might it be CMB or a foreground (e.g. dust)) sky along with LevelS+Madam noise simulations were used widely for the analysis of Planck data. A suite of simulations were rendered during the mission tagged as Full Focalplane simulations, FFP#.<br />
For example [[HL-sims#FFP6 data set|FFP6]] <br />
<br />
===Beam Window Functions===<br />
The '''Transfer Function''' or the '''Beam Window Function''' <math> W_l </math> relates the true angular power spectra <math>C_l </math> with the observed angular power spectra <math>\widetilde{C}_l </math>:<br />
<br />
<math><br />
W_l= \widetilde{C}_l / C_l <br />
\label{eqn:wl1}</math> <br />
<br />
Note that, the window function can contain a pixel window function (depending on the definition) and it is {\em not the angular power spectra of the scanbeams}, though, in principle, one may be able to connect them though fairly complicated algebra.<br />
<br />
The window functions are estimated by performing Monte-Carlo simulations. We generate several random realisations of the CMB sky starting from a given fiducial <math> C_l </math>, convolve the maps with the pre-computed effective beams, compute the convolved power spectra <math> C^\text{conv}_l </math>, divide by the power spectra of the unconvolved map <math>C^\text{in}_l </math> and average over their ratio. Thus, the estimated window function<br />
<br />
<math><br />
W^{est}_l = < C^{conv}_l / C^{in}_l ><br />
\label{eqn:wl2}</math> <br />
<br />
For subtle reasons, we perform a more rigorous estimation of the window function by comparing C^{conv}_l with convolved power spectra of the input maps convolved with a symmetric Gaussian beam of comparable (but need not be exact) size and then scaling the estimated window function accordingly.<br />
<br />
Beam window functions are provided in the [[The RIMO#Beam Window Functions|RIMO]]. <br />
<br />
<br />
====Beam Window functions, Wl, for Planck mission====<br />
[[File:plot_dx9_LFI_GB_pix.png | 600px | thumb | center |'''Beam Window functions, Wl, for LFI channels''']] <br />
[[File:plot_dx9_HFI_BS_M12_CMB.png | 600px | thumb | |center |'''Beam Window functions, Wl, for HFI channels''']]<br />
<br />
==File Names==<br />
The effective beams are provided by the PLA as FITS files containg HEALPix maps of the beams. For the file names the following convention is used:<br />
*Single beam query: '''beams_FFF_''PixelNumber''.fits''' <br />
**FFF is the channel frequency (one of '''30''', '''44''', '''70''', '''100''', '''143''', '''217''', '''353''', '''545''', '''857'''); <br />
** ''PixelNumber'' is the number of the pixel to which the beam corresponds (<math>0</math> - <math>12 \times N_{\rm side}^2 - 1</math>). For the LFI <math>N_{\rm side}=1024</math>, for the HFI <math>N_{\rm side}=2048</math>;<br />
*Multiple beam query: '''beams_FFF_''FirstPixelNumber''-''LastPixelNumber''.zip''' <br /> The compressed files contains a set of files with the beams for the pixels covereing the selected region. FFF as for sinle beam query. The naming convention for the beam files contained in the ''.zip'' file is the same as for single beam queries.<br />
** ''FirstPixelNumber'' is the lowest pixel number for the area covered by the request;<br />
** ''LastPixelNumber'' is the highest pixel number for the area covered by the request;<br />
<br />
==File format==<br />
The FITS files provided by the PLA contain HEALPix maps of the beams.<br />
<br />
== References ==<br />
<References /><br />
<br />
<br />
<br />
<br />
<br />
[[Category:Mission products|004]]</div>
Xdupac
https://wiki.cosmos.esa.int/planckpla2015/index.php?title=Timelines&diff=11420
Timelines
2015-02-05T10:35:12Z
<p>Xdupac: /* LFI HouseKeeping files */</p>
<hr />
<div>{{DISPLAYTITLE:2015 Timelines}}<br />
==General description==<br />
<br />
The timelines, or TOIs for ''Time-Ordered Information'', are vectors of signal or of pointing or of some other quantity giving the value of that quantity as a function of time during the mission. The TOIs described here are sampled regularly at the (instrument dependent) detector sampling frequency and span the full science mission. They thus consist of a large amount of data. This section is concerned with the signal TOIs and their associated pointing TOIs. For selected detectors the DPCs provide a single timeline of cleaned and calibrated signal and 3 timelines of coordinates, corresponding to the two angular coordinates and one position angle. <br />
<br />
Obviously these vectors are very long (~1.38E10 samples for HFI, from ~2.5E06 to ~5.5E06 for LFI) and thus need to be split into multiple files for export. Here the data are split by Operational Day (OD) as follows:<br />
* HFI: 12 files per OD, one for pointing and one for signal for each channel, covering ODs 91 -- 974, all sampled at F<sub>samp</sub> = 180.3737 Hz. <br />
* LFI: 6 files per OD, 3 each for signal and pointing, since the sampling frequency is channel dependent, and covering ODs 91 -- 1543, sampled at F<sub>samp</sub> = 32.5079, F<sub>samp</sub> = 46.5455 and F<sub>samp</sub> = 78.7692 Hz.<br />
<br />
The signal timelines are encoded as Real*4, but the pointing vectors had to be encoded as Real*8 to maintain the required accuracy. The result is that the total volume of the full dataset is ~30 TB. All files also contain the OBT.<br />
<br />
The signal timelines have been cleaned of all known instrumental systematic effects, they have been calibrated in flux, and the solar and earth motion dipole signals have been removed. But they have not been cleaned of the low-frequency, ''1/f'' noise that needs to be removed via a destriping tool. The methods consists of removing offsets or ''baselines'' determined by minimizing the differences in the signals at points on the sky where they intersect. For HFI an offset per ring is determined; for LFI the the baseline is computed every 0.246, 0.988 and 1.000 second for the 30, 44 and 70 GHz respectively and maintain the same structure of the signal timelines.<br />
In case of HFI these offsets are determined using the full mission and all the valid detectors per channel, and they are then used for all the maps produced, i.e., for those maps using any fraction of the mission (year, survey) or any subset of the detectors (single detector, detector set), and it was shown that using offsets determined from a limited part of the mission and/or a subset of the detectors yields maps that are less consistent than otherwise. <br />
<br />
In case of LFI these offsets are determined using the full mission and all the valid detectors per channel, those values has been used for the production of the full mission period maps. Note that baseline used for shorter period maps are determined on those data period to avoid noise cross-correlation effect and those are not delivered.<br />
<br />
The offsets are delivered separately, as described below.<br />
<br />
Furthermore, for HFI and LFI, there are three sets of offsets produced: the primary set using the full rings, and the secondary ones using the first and second half rings, only. The difference between the primary and the secondary sets are fairly minor, but they are necessary to rebuild the maps as they were built by the HFI-DPC and LFI-DPC. Overall the offsets are useful for users wishing to build a map of a small area of the sky.<br />
<br />
The HFI delivers its offsets in a ROI, or "Ring-Ordered Information" file. That file contains a table of N<sub>rings</sub> = 26766 rows by N<sub>bolometers</sub> in which each cell contains a 3-elements vector containing the full-ring, first half-ring, and second half-ring offsets. The indices of the signal TOI delimiting the rings are given in a second ROI file with the same N<sub>rings</sub> rows containing global parameters.<br />
<br />
The LFI delivers its offsets in a TOI format, the structure is EXACTLY the same used by the Science Timelines. The user can simply subtract one-by-one the offset timelines from the Science Timelines and then generate a map with the result.<br />
In case of the half-ring baseline, a vector has been added in the OBT extension; this vector contains 1 or 2 depending to which half ring should be applied.<br />
<br />
===HFI Indexing===<br />
<br />
Each FITS file contains keywords giving the first and last index of the section of the full TOI contained in the file. These indices are those of the internal DPC representation; they begin at 0 corresponding to the switch-on of the instrument, and run to some very large number (~25 billion for HFI) representing the full mission. Only the ''science'' part of the mission is exported, which is about 60% of the total for HFI. Are left out the early mission phase (cool-down and validation phases) and the warm phase of HFI, during which LFI continued to collect data. The HFI keywords also indicated which rings are included in each OD, but be aware that normally an OD does not begin at the same time (with the same index) as a ring. <br />
<br />
Note that for historical reasons, the OD definitions of the two DPCs differ: for LFI they occur at the transition between pointing periods, whereas for HFI they do not. This has however no significant importance for the user, as this splitting is somewhat arbitrary anyway, and what counts is the full vector once it is rebuilt in the user's own work space.<br />
<br />
HFI timelines at the DPC are indexed from 0 to ~25E9, that correspond to instrument switch-on to switch-off. Of these the indices ~1.4E9 to 151.5E9 correspond to the science mission and are exported and delivered. Each file contains a keyword giving the first and last index of the data in that file, and EndIndex(OD)+1 = BeginIndex (OD+1). The ROI ''Global'' file gives the Begin/End Indices of each Ring, or Pointing Period, and can be used to destripe the signal TOIs with the offsets provided in the ''Destriping-Offsets'' ROI file.<br />
<br />
==Production process==<br />
<br />
=== HFI processing ===<br />
<br />
The input TOIs are in ADUs representing the voltage signal at the end of the electronics (see [[HFI_detection_chain | Detection chain]] for details). The processing applied to remove instrumental effects and to calibrate them is described in detail in the [[TOI processing | HFI TOI processing]] section, and in <span style="color:Red">Planck-2015-VII ref</span> we give a very brief summary here for convenience. That pipeline performs the following operations:<br />
<br />
; ADC correction: corrects for the uneven size of the ADC bins (see [[ADC correction]]).<br />
; demodulation: this is performed around a variable level which is determined from the valid input data (using a validity flag from a previous version of the processing), and the data are converted to engineering units (V) using known conversion coefficients.<br />
; despiking: the redundancy within a ring is used to determine where glitches occur. Once identified, the glitches are fitted with templates. A glitch flag is produced that identifies the strongest part of the glitches, and a timeline of glitch tails. produced from the template fits, is subtracted from the demodulated timeline. Finally, the flagged regions are replaced with data from an average over the pointing period in order to not leave holes in the timeline that would perturb the usage of Fourier methods on them<br />
; dark template removal: the two dark bolometers are demodulated and despiked as above; the resulting timelines are then smoothed and used as an indicator of the overall temperature variations of the bolometer plate. Where the variations are consistent with each other, they are combined and removed from the bolometer signal timelines using appropriate coupling coefficients. The few percent of the data where they are not consistent are flagged as not valid on the timelines.<br />
; conversion to absorbed power: the timeline is converted to watts of absorbed power using the bolometer function. This includes a non-linearity correction; removal of the 4K cooler lines: the electromagnetic interference of the 4K cooler with the bolometer readout wires induces some sharp lines in the signal power spectra at frequencies of the 4K cooler's fundamental and its multiples, folded by the signal modulations. Fourier coefficients of the relevant lines are determined on a per-ring basis, and then removed from the data. The quality of the removal depends on the bolometer.<br />
; deconvolution by the time transfer function: this is done to correct for the non-instantaneous time response of the bolometers. The function itself is modeled using up to 8 time constants which are adjusted primarily on the planet data and also from comparisons of the northward and southward scans of the Galactic Plane. It is then removed using Fourier techniques.<br />
; jump correction: corrects some pretty rare jumps in the signal baseline (there are on average ~ 0.3 jumps per bolometer per pointing period). The jumps are detected and characterised on smoothed TOIs, and corrected by adding a constant to part of the signal timeline. The origin of the jumps is not known.<br />
<br />
The results of this processing are a timeline of signal (in absorbed watts) and a ''valid data'' flag timeline for each of the 50 valid bolometers which are processed, out of the 52 HFI bolometers; these timelines contain the full sky signal, i.e., including the solar and orbital dipoles, the Zodiacal light, and contributions from the Far-Side lobes. The dipoles are necessary for the flux calibration and are removed at the mapmaking stage. The remaining two bolometers (143-8 and 545-3) show semi-random jumps in the signal level, typically jumping over 2-5 different ''pseudo-baseline'' levels, a behavior known as ''Random Telegraphic Signal'', so that these are commonly called the RTS bolometers. Finally, ring-level statistics of different types (mean, median, rms, kurtosis, etc.) are determined on a per-ring basis for all timelines, and a selection based on these statistics is used to discard anomalous rings, which are recorded in a ring-level flag for each valid bolometer timeline (see the [[TOI_processing#Discarded_rings | Discarded rings]] section). <br />
<br />
Throughout this processing, some planet signals are masked in the timeline in order to avoid ringing effects in the processing. It concerns only Jupiter at 100 and 143 GHz, Jupiter and Saturn at 217 GHz, Jupiter, Saturn and Mars at 353, 545 and 857 GHz (thanks to various improvements in the despiking and in the transfer functions it is no longer necessary to flag these three planets in the CMB channels as was done in Release 1). Since they move on the sky, the portion of the sky masked during one survey is observed during another one, and no hole is left in the final map. In parallel, the planet data are processed in a similar way, but with different parameters for the despiking step. These results are processed separately to determine the beam shapes and the focal plane geometry.<br />
<br />
Next, the TOIs are calibrated in astrophysical units using the results of the calibration pipeline (see the [[Map-making | Map-making and calibration]] section) and the best estimate of the zero-point offsets (a constant level for each bolometer). These values are given in the RIMO. Also, the solar and earth-motion dipole signals are computed and removed. <br />
<br />
These TOIs are accompanied by several flags that are described below. The most important one is the ''Total'' flag, which identifies all the samples that were discarded by the DPC mapmaking, ad described in [[TOI processing | HFI TOI processing]]. This flag includes the portion beyond 72 min for the rings that are longer, which is not used because of the slight drift of the satellite pointing direction (spin axis) during these long acquisition periods.<br />
<br />
At this point the TOIs still contain the low frequency (1/f) noise which should be removed before projection onto a map. That cleaning step is called "destriping" "baseline removal". The HFI-DPC does its destriping at ring-level, meaning that a constant is added to the signal of each ring in order to minimise the difference at the ring crossings, where the signal should be the same for all detectors (with the necessary precautions as described in [[Map-making | Map-making and calibration]] section); should the user want to use the DPC's offsets, they are provided separately (see [[Timelines#ROI_files | ROI files]] below). Maps produced from these TOIs, and after subtraction of the DPC's destriping offsets, are not identical to the maps delivered. This is discussed in Section A.2 by <span style="color:Red">Planck-2015-VII ref</span>.<br />
<br />
The pointing (see common [[Detector_pointing | Detector Pointing]] section for details) is determined from the AHF produced by MOC, which gives the direction and orientation of the LOS of a fiducial position in the focal plane at frequencies of 8Hz during stable pointing and 4 Hz during maneuvers. This is interpolated to the timestamps of data samples, corrected for the wobble and other time-dependent offsets determined from the observed positions of a large number of sources around the sky, and finally converted to the LOS of each detector using the quaternions in the IMO.<br />
<br />
=== LFI processing ===<br />
The input TOIs are in ADUs representing the voltage signal at the output of the electronics (see [[LFI design, qualification, and performance#Radiometer Chain Assembly (RCA) | Radiometer Chain Assembly (RCA)]] for details). The processing applied to remove instrumental effects and to calibrate them is described in detail in the [[TOI processing | LFI TOI processing]] section, and in {{PlanckPapers|planck2014-a03||Planck-2015-A03}} we give a very brief summary here for convenience. That pipeline performs the following operations:<br />
; ADC correction: due to ADC non-linearity under certain condition, this instrumental effect is removed by applying well know templates directly to the diode signal.<br />
; Electronics Spikes: caused by the interaction between the electronics clock and the scientific data lines. The<br />
signal is detected in all the LFI radiometers' time-domain outputs as a 1s square wave with a rising edge near 0.5s <br />
and a falling edge near 0.75s synchronous with the on-board time signal. In the frequency domain it appears as a spike signal at multiples of 1 Hz. The 44 GHz channels are the only LFI outputs significantly affected by this effect. Consequently the spike signal is removed from the data only in these channels.<br />
; Demodulation: each LFI diode switches at 4096 Hz between the sky and the 4K reference load. The data acquired in this way is dominated by 1\f noise that is highly correlated between the two streams; differencing those streams results in a strong reduction of 1\f noise. The procedure applied is described in [[TOI processing | LFI TOI processing]] taking into account that the gain modulation factor R was computed on timestreams with the Galaxy and point sources masked to avoid strong sky signals.<br />
; Diode combination: two detector diodes provide the output for each LFI receiver channel. To minimize the impact of imperfect isolation of the data stream of each diode, we perform a weighted average of the time-ordered data from the two diodes of each receiver. The procedure applied is detailed in [[TOI processing | LFI TOI processing]]; the weights used are kept fixed for the entire mission.<br />
; Scientific Calibration: calibrate the timelines to physical units K<sub>CMB</sub>, fitting the total CMB dipole convolved with the 4pi beam representation, without taking into account the signature due to Galactic straylight;<br />
; Gain regularization: the calibration constants computed using the model of the dipole signal suffer from large uncertainties when the Planck spacecraft is badly aligned with the dipole axis. To reduce the noise, we apply an adaptive smoothing algorithm<br />
that is also designed to preserve the discontinuities caused by abrupt changes in the working configuration of the radiometers<br />
(e.g., sudden temperature changes in the focal plane).<br />
; Removal of solar and orbital dipole signal: the combined solar and orbital dipole is convolved with the 4pi beam representation of each radiometer and the removed from its timeline.<br />
; Removal of Galactic Straylight: the light incident on the focal plane without reflecting on the primary mirror (straylight) is a major source of systematic effects, especially when the Galactic plane intersects the direction of the main spillover. This effect is corrected by removing the estimated straylight signal from the timelines. This signal is computed as the convolution of Galaxy simulation with the beam sidelobes, see details in [[TOI processing | LFI TOI processing]].<br />
<br />
At this point the timelines are used for the production of the maps.<br />
<br />
The pointing (see common [[Detector_pointing | Detector Pointing]] section for details) is determined from the AHF produced by the MOC, which gives the direction and orientation of the LOS of a fiducial position in the focal plane at frequencies of 8Hz during stable pointing and 4 Hz during maneuvers. This is interpolated to the timestamps of data samples, corrected for the wobble and other time-dependent offsets determined from the observed positions of a large number of sources around the sky and temperature sensor, and finally converted to the LOS of each detector.<br />
<br />
==File Names==<br />
<br />
The file names are of the form:<br />
<br />
''{H,L}FI_TOI_{fff}-{SCI,PTG,TAI,OFF}_R2.nn_ODxxxx.fits''<br />
<br />
where<br />
* ''fff'' denotes the frequency<br />
* SCI denote signal TOIs<br />
* PTG denote pointing TOIs<br />
* TAI denote OBT-MJD correlation TOI<br />
* OFF denote Baseline TOI<br />
* R2.nn is the version, and<br />
* ODxxxx indicates the OD.<br />
<br />
<br />
At the present time, HFI is providing signal TOIs for all the SWB (non-polarised) bolometers and for the PSB (polarised) bolometers at 353GHz only. The reasons for this are detailed in [###REF###]. On the other hand, the pointing TOIs are available for all bolometers. LFI is providing all signal TOI.<br />
<br />
==FITS file structure==<br />
<br />
All FITS files begin with a primary extension containing no data and a minimal header, which is followed by one or more ''BINTABLE'' extensions with data, and with a description of the data in the header keywords. In what follows will usually ignore the primary extension, and count only the extensions containing data.<br />
<br />
===TOI files===<br />
<br />
The signal FITS files contain N ,'BINTABLE', data extensions, where N is the number of detectors in that frequency channel. The first extension contains the OBT and its flags, called the ''global'' flags since they apply to all detectors, which is followed by one extension for each detector, containing the signal and its ''local'' flag. The flags columns are written as ''byte'' in which each of the 8 bits (max) encodes one flag timeline. The meaning of each bit is given in the header comments and is subject to change.<br />
For the global flag they include:<br />
* HFI<br />
** Unstable pointing: 1= pointing is not stable (e.g., during repointing maneuvers)<br />
** Dark correlation: 1 = darks are uncorrelated and data are flagged<br />
** First/Second half ring: which samples are in which half (only covers the stable pointing part of the ring)<br />
** HCM: in HCM mode (unstable pointing)<br />
** and more<br />
<br />
* LFI<br />
** Bit 0, unstable pointing: 1= pointing is not stable<br />
** Bit 1, time correlation quality: 1= outside specification<br />
** Bit 2, special observation: 1= special observation like deep scan<br />
<br />
And for the local flag they include<br />
<br />
* HFI<br />
** Total Flag: a combination of the various flags that is the one finally used in the map-making (all samples with Total Flag different from zero should not be used)<br />
** Data not valid: glitched samples<br />
** Despike Common: (for PSBs only) glitch on current or other of PSB pair<br />
** StrongSignal: on Galactic Plane<br />
** Strong Source: on point source<br />
** other<br />
<br />
* LFI<br />
** Bit 0, Data not valid: 1= Science sample not valid<br />
** Bit 2: Planet crossing: 1= Science Sample containing planet<br />
** Bit 3: Moving objects: 1= minor Solar System object (not yet used)<br />
** Bit 4: Gap: 1= this sample was artificially included due to gap in the data<br />
<br />
<br />
<br />
{| border="1" cellpadding="3" cellspacing="0" align="center" style="text-align:left" width=800px<br />
|+ '''TOI file data structure'''<br />
<br />
|- bgcolor="ffdead" <br />
!colspan="5" | 1. EXTNAME = 'OBT' : Data columns<br />
|- bgcolor="ffdead" <br />
! Column Name || Data Type || Units || Description || Comment<br />
|-<br />
|OBT || Int*8 || 2<sup>-16</sup> sec || On-board time ||<br />
|-<br />
|FLAG || Byte || none || the various bit-level flags ||<br />
<br />
|- bgcolor="ffdead" <br />
! Keyword || Data Type || Value || Description || Comment<br />
|-<br />
|OD || Int || || OD covered (as in filename) ||<br />
|-<br />
|BEGIDX || Int || || first sample index of given OD || Only HFI<br />
|-<br />
|ENDIDX || Int || || last sample index of given OD || Only HFI<br />
|-<br />
|BEGRING || Int || || first ring in given OD || Only HFI<br />
|-<br />
|ENDRING || Int || || last ring in given OD || Only HFI<br />
|-<br />
|TIMEZERO || String || 1958-01-01z00:00 || Origin of OBT || Only HFI<br />
|-<br />
|TIMEZERO || Float || 106744000000000. || Origin of OBT || Only LFI<br />
<br />
|- bgcolor="ffdead" <br />
!colspan="5" | n. EXTNAME = ''DETNAME'' : Data columns<br />
<br />
|- bgcolor="ffdead" <br />
! Column Name || Data Type || Units || Description || Comment<br />
|-<br />
|SIGNAL || Real*4 || K<sub>cmb</sub> or MJy/sr || Value of signal || Comment<br />
|-<br />
|FLAG || Byte || none || the various bit-level flags ||<br />
|- bgcolor="ffdead" <br />
<br />
! Keyword || Data Type || Value || Description || Comment<br />
|-<br />
|UNIT || String || || Units of signal || Only HFI, LFI always K<sub>cmb</sub><br />
|-<br />
|DESTRIPE || 1/0 || || whether timeline is destriped || Only HFI<br />
|-<br />
|OD || Int || || OD covered (as in filename) ||<br />
|-<br />
|BEGIDX || Int || || first sample index of given OD || Only HFI<br />
|-<br />
|ENDIDX || Int || || last sample index of given OD || Only HFI<br />
|-<br />
|BEGRING || Int || || first ring in given OD || Only HFI<br />
|-<br />
|ENDRING || Int || || last ring in given OD || Only HFI<br />
|}<br />
<br />
<br />
The pointing files have a similar structure, except that ''DETNAME'' extensions contain 3 columns of Real*8 with the phi, theta, and psi Galactic spherical coordinates of each sample in radians, as shown in the table below. There is no local flag for the coordinates.<br />
<br />
{| border="1" cellpadding="3" cellspacing="0" align="center" style="text-align:left" width=800px<br />
|+ '''Pointing TOI file DETNAME extension structure'''<br />
<br />
|- bgcolor="ffdead" <br />
!colspan="4" | n. EXTNAME = ''DETNAME'' : Data columns<br />
<br />
|- bgcolor="ffdead" <br />
! Column Name || Data Type || Units || Description<br />
|-<br />
|PHI || Real*8 || radian || longitude<br />
|-<br />
|THETA || Real*8 || radian || colatitude<br />
|-<br />
|PSI || Real*8 || radian || roll angle<br />
|}<br />
<br />
===HFI ROI files===<br />
<br />
The files provided by HFI are<br />
* ''HFI_ROI_GlobalParams_RelNum_full.fits''<br />
* ''HFI_ROI_DestripeOffsets_RelNum_full.fits''<br />
which are described below.<br />
<br />
;Global parameters: this ROI file contains a single ''BINTABLE'' extension with 3 columns that give, for each ring, the index number of the first sample, the ESA pointing ID of the ring, and the ring start time. All three are encoded as Int*8, and the time is given in units of 2<sup>-16</sup> sec from ''TIMEZERO'', 1958-01-01z00:00, as in the TOI files. Rings are numbered from 240 to 27005, as given in the ''BEGRING'' and ''ENDRING'' keywords<br />
<br />
; Destriping offsets: this ROI file contains a single ''BINTABLE'' extension with 3 columns that give, for each ring, the offsets to subtract from each bolometer signal timeline or vector. There are three offsets available for each bolometer: full-ring, first half-ring, and second half-ring, for building the full-ring or the two half-ring maps, respectively. The offsets must be subtracted from Index(N) to Index(N+1)-1 of the corresponding signal timeline, where N is the ring number, and the indices are given in the Global parameters file. The offsets are given in the same units as the signal vectors, that is K<sub>cmb</sub> for the 100-353 GHz channels, and MJy/sr for the 545 and 857 GHz channels. All values are encoded as Real*4. The rings for which the offsets are set to 0.000 are [[TOI_processing#Discarded_rings | ''badrings'' ]] which are rejected in the mapmaking process. These rings are also flagged by the ''TotalFlag'', as are the portions of rings longer than ~72.5 min, where the drift in the satellite's spin axis becomes important.<br />
<br />
===TAI TOI files===<br />
<br />
The TAI TOI files contains one extension with two column, the first is the OBT value (exactly the same reported in the SCI TOI), the second the corresponding Modified Julian day. Note that Leap second where not added.<br />
<br />
{| border="1" cellpadding="3" cellspacing="0" align="center" style="text-align:left" width=800px<br />
|+ '''Time TAI TOI file data structure'''<br />
<br />
|- bgcolor="ffdead" <br />
!colspan="5" | 1. EXTNAME = 'OBT-MJD' : Data columns<br />
|- bgcolor="ffdead" <br />
! Column Name || Data Type || Units || Description || Comment<br />
|-<br />
|OBT || Int*8 || 2<sup>-16</sup> sec || On-board time ||<br />
|-<br />
|MJD || Real*8 || day || Modified Julian day ||<br />
|}<br />
<br />
===LFI OFF TOI files===<br />
The OFF (baseline) TOI files adopt the same file structure of the Science TOI files. Note that in case of OFF timelines related to the half-ring, and addition column in included in the OBT extension to define for each sample if it belong to half-ring 1 or half-ring2.<br />
<br />
===LFI HouseKeeping files===<br />
House keeping timelines are:<br />
* LFI_TOI_DAE-FAST-HK_R2.nn_ODxxxx.fits<br />
* LFI_TOI_DAE-SlowConfiguration-HK_R2.nn_ODxxxx.fits<br />
* LFI_TOI_DAE-SlowCurrent-HK_R2.nn_ODxxxx.fits<br />
* LFI_TOI_DAE-SlowPhaseSwitch-HK_R2.nn_ODxxxx.fits<br />
* LFI_TOI_DAE-SlowVoltage-HK_R2.nn_ODxxxx.fits<br />
* LFI_TOI_REBA-HK_R2.nn_ODxxxx.fits<br />
* SCS_TOI_EssentialASW-HK_R2.nn_ODxxxx.fits<br />
* SCS_TOI_NonEssentialASW-HK_R2.nn_ODxxxx.fits<br />
<br />
Each file contains two extension, the first is the OBT (value are sampled at 1 or 10 seconds), the latter contain a variable number of column = 2* number of HouseKeeping stored. Each Housekeeping is accompanied by its flag (normally 0 is NOT 0 the value was considerate invalid or Out Of Limit). The Housekeeping name are the once defined in the LFI Instrnument Operation Manual.<br />
<br />
== References ==<br />
<br />
<References /><br />
<br />
[[Category:Mission products|001]]</div>
Xdupac
https://wiki.cosmos.esa.int/planckpla2015/index.php?title=Timelines&diff=11418
Timelines
2015-02-05T10:34:14Z
<p>Xdupac: /* General description */</p>
<hr />
<div>{{DISPLAYTITLE:2015 Timelines}}<br />
==General description==<br />
<br />
The timelines, or TOIs for ''Time-Ordered Information'', are vectors of signal or of pointing or of some other quantity giving the value of that quantity as a function of time during the mission. The TOIs described here are sampled regularly at the (instrument dependent) detector sampling frequency and span the full science mission. They thus consist of a large amount of data. This section is concerned with the signal TOIs and their associated pointing TOIs. For selected detectors the DPCs provide a single timeline of cleaned and calibrated signal and 3 timelines of coordinates, corresponding to the two angular coordinates and one position angle. <br />
<br />
Obviously these vectors are very long (~1.38E10 samples for HFI, from ~2.5E06 to ~5.5E06 for LFI) and thus need to be split into multiple files for export. Here the data are split by Operational Day (OD) as follows:<br />
* HFI: 12 files per OD, one for pointing and one for signal for each channel, covering ODs 91 -- 974, all sampled at F<sub>samp</sub> = 180.3737 Hz. <br />
* LFI: 6 files per OD, 3 each for signal and pointing, since the sampling frequency is channel dependent, and covering ODs 91 -- 1543, sampled at F<sub>samp</sub> = 32.5079, F<sub>samp</sub> = 46.5455 and F<sub>samp</sub> = 78.7692 Hz.<br />
<br />
The signal timelines are encoded as Real*4, but the pointing vectors had to be encoded as Real*8 to maintain the required accuracy. The result is that the total volume of the full dataset is ~30 TB. All files also contain the OBT.<br />
<br />
The signal timelines have been cleaned of all known instrumental systematic effects, they have been calibrated in flux, and the solar and earth motion dipole signals have been removed. But they have not been cleaned of the low-frequency, ''1/f'' noise that needs to be removed via a destriping tool. The methods consists of removing offsets or ''baselines'' determined by minimizing the differences in the signals at points on the sky where they intersect. For HFI an offset per ring is determined; for LFI the the baseline is computed every 0.246, 0.988 and 1.000 second for the 30, 44 and 70 GHz respectively and maintain the same structure of the signal timelines.<br />
In case of HFI these offsets are determined using the full mission and all the valid detectors per channel, and they are then used for all the maps produced, i.e., for those maps using any fraction of the mission (year, survey) or any subset of the detectors (single detector, detector set), and it was shown that using offsets determined from a limited part of the mission and/or a subset of the detectors yields maps that are less consistent than otherwise. <br />
<br />
In case of LFI these offsets are determined using the full mission and all the valid detectors per channel, those values has been used for the production of the full mission period maps. Note that baseline used for shorter period maps are determined on those data period to avoid noise cross-correlation effect and those are not delivered.<br />
<br />
The offsets are delivered separately, as described below.<br />
<br />
Furthermore, for HFI and LFI, there are three sets of offsets produced: the primary set using the full rings, and the secondary ones using the first and second half rings, only. The difference between the primary and the secondary sets are fairly minor, but they are necessary to rebuild the maps as they were built by the HFI-DPC and LFI-DPC. Overall the offsets are useful for users wishing to build a map of a small area of the sky.<br />
<br />
The HFI delivers its offsets in a ROI, or "Ring-Ordered Information" file. That file contains a table of N<sub>rings</sub> = 26766 rows by N<sub>bolometers</sub> in which each cell contains a 3-elements vector containing the full-ring, first half-ring, and second half-ring offsets. The indices of the signal TOI delimiting the rings are given in a second ROI file with the same N<sub>rings</sub> rows containing global parameters.<br />
<br />
The LFI delivers its offsets in a TOI format, the structure is EXACTLY the same used by the Science Timelines. The user can simply subtract one-by-one the offset timelines from the Science Timelines and then generate a map with the result.<br />
In case of the half-ring baseline, a vector has been added in the OBT extension; this vector contains 1 or 2 depending to which half ring should be applied.<br />
<br />
===HFI Indexing===<br />
<br />
Each FITS file contains keywords giving the first and last index of the section of the full TOI contained in the file. These indices are those of the internal DPC representation; they begin at 0 corresponding to the switch-on of the instrument, and run to some very large number (~25 billion for HFI) representing the full mission. Only the ''science'' part of the mission is exported, which is about 60% of the total for HFI. Are left out the early mission phase (cool-down and validation phases) and the warm phase of HFI, during which LFI continued to collect data. The HFI keywords also indicated which rings are included in each OD, but be aware that normally an OD does not begin at the same time (with the same index) as a ring. <br />
<br />
Note that for historical reasons, the OD definitions of the two DPCs differ: for LFI they occur at the transition between pointing periods, whereas for HFI they do not. This has however no significant importance for the user, as this splitting is somewhat arbitrary anyway, and what counts is the full vector once it is rebuilt in the user's own work space.<br />
<br />
HFI timelines at the DPC are indexed from 0 to ~25E9, that correspond to instrument switch-on to switch-off. Of these the indices ~1.4E9 to 151.5E9 correspond to the science mission and are exported and delivered. Each file contains a keyword giving the first and last index of the data in that file, and EndIndex(OD)+1 = BeginIndex (OD+1). The ROI ''Global'' file gives the Begin/End Indices of each Ring, or Pointing Period, and can be used to destripe the signal TOIs with the offsets provided in the ''Destriping-Offsets'' ROI file.<br />
<br />
==Production process==<br />
<br />
=== HFI processing ===<br />
<br />
The input TOIs are in ADUs representing the voltage signal at the end of the electronics (see [[HFI_detection_chain | Detection chain]] for details). The processing applied to remove instrumental effects and to calibrate them is described in detail in the [[TOI processing | HFI TOI processing]] section, and in <span style="color:Red">Planck-2015-VII ref</span> we give a very brief summary here for convenience. That pipeline performs the following operations:<br />
<br />
; ADC correction: corrects for the uneven size of the ADC bins (see [[ADC correction]]).<br />
; demodulation: this is performed around a variable level which is determined from the valid input data (using a validity flag from a previous version of the processing), and the data are converted to engineering units (V) using known conversion coefficients.<br />
; despiking: the redundancy within a ring is used to determine where glitches occur. Once identified, the glitches are fitted with templates. A glitch flag is produced that identifies the strongest part of the glitches, and a timeline of glitch tails. produced from the template fits, is subtracted from the demodulated timeline. Finally, the flagged regions are replaced with data from an average over the pointing period in order to not leave holes in the timeline that would perturb the usage of Fourier methods on them<br />
; dark template removal: the two dark bolometers are demodulated and despiked as above; the resulting timelines are then smoothed and used as an indicator of the overall temperature variations of the bolometer plate. Where the variations are consistent with each other, they are combined and removed from the bolometer signal timelines using appropriate coupling coefficients. The few percent of the data where they are not consistent are flagged as not valid on the timelines.<br />
; conversion to absorbed power: the timeline is converted to watts of absorbed power using the bolometer function. This includes a non-linearity correction; removal of the 4K cooler lines: the electromagnetic interference of the 4K cooler with the bolometer readout wires induces some sharp lines in the signal power spectra at frequencies of the 4K cooler's fundamental and its multiples, folded by the signal modulations. Fourier coefficients of the relevant lines are determined on a per-ring basis, and then removed from the data. The quality of the removal depends on the bolometer.<br />
; deconvolution by the time transfer function: this is done to correct for the non-instantaneous time response of the bolometers. The function itself is modeled using up to 8 time constants which are adjusted primarily on the planet data and also from comparisons of the northward and southward scans of the Galactic Plane. It is then removed using Fourier techniques.<br />
; jump correction: corrects some pretty rare jumps in the signal baseline (there are on average ~ 0.3 jumps per bolometer per pointing period). The jumps are detected and characterised on smoothed TOIs, and corrected by adding a constant to part of the signal timeline. The origin of the jumps is not known.<br />
<br />
The results of this processing are a timeline of signal (in absorbed watts) and a ''valid data'' flag timeline for each of the 50 valid bolometers which are processed, out of the 52 HFI bolometers; these timelines contain the full sky signal, i.e., including the solar and orbital dipoles, the Zodiacal light, and contributions from the Far-Side lobes. The dipoles are necessary for the flux calibration and are removed at the mapmaking stage. The remaining two bolometers (143-8 and 545-3) show semi-random jumps in the signal level, typically jumping over 2-5 different ''pseudo-baseline'' levels, a behavior known as ''Random Telegraphic Signal'', so that these are commonly called the RTS bolometers. Finally, ring-level statistics of different types (mean, median, rms, kurtosis, etc.) are determined on a per-ring basis for all timelines, and a selection based on these statistics is used to discard anomalous rings, which are recorded in a ring-level flag for each valid bolometer timeline (see the [[TOI_processing#Discarded_rings | Discarded rings]] section). <br />
<br />
Throughout this processing, some planet signals are masked in the timeline in order to avoid ringing effects in the processing. It concerns only Jupiter at 100 and 143 GHz, Jupiter and Saturn at 217 GHz, Jupiter, Saturn and Mars at 353, 545 and 857 GHz (thanks to various improvements in the despiking and in the transfer functions it is no longer necessary to flag these three planets in the CMB channels as was done in Release 1). Since they move on the sky, the portion of the sky masked during one survey is observed during another one, and no hole is left in the final map. In parallel, the planet data are processed in a similar way, but with different parameters for the despiking step. These results are processed separately to determine the beam shapes and the focal plane geometry.<br />
<br />
Next, the TOIs are calibrated in astrophysical units using the results of the calibration pipeline (see the [[Map-making | Map-making and calibration]] section) and the best estimate of the zero-point offsets (a constant level for each bolometer). These values are given in the RIMO. Also, the solar and earth-motion dipole signals are computed and removed. <br />
<br />
These TOIs are accompanied by several flags that are described below. The most important one is the ''Total'' flag, which identifies all the samples that were discarded by the DPC mapmaking, ad described in [[TOI processing | HFI TOI processing]]. This flag includes the portion beyond 72 min for the rings that are longer, which is not used because of the slight drift of the satellite pointing direction (spin axis) during these long acquisition periods.<br />
<br />
At this point the TOIs still contain the low frequency (1/f) noise which should be removed before projection onto a map. That cleaning step is called "destriping" "baseline removal". The HFI-DPC does its destriping at ring-level, meaning that a constant is added to the signal of each ring in order to minimise the difference at the ring crossings, where the signal should be the same for all detectors (with the necessary precautions as described in [[Map-making | Map-making and calibration]] section); should the user want to use the DPC's offsets, they are provided separately (see [[Timelines#ROI_files | ROI files]] below). Maps produced from these TOIs, and after subtraction of the DPC's destriping offsets, are not identical to the maps delivered. This is discussed in Section A.2 by <span style="color:Red">Planck-2015-VII ref</span>.<br />
<br />
The pointing (see common [[Detector_pointing | Detector Pointing]] section for details) is determined from the AHF produced by MOC, which gives the direction and orientation of the LOS of a fiducial position in the focal plane at frequencies of 8Hz during stable pointing and 4 Hz during maneuvers. This is interpolated to the timestamps of data samples, corrected for the wobble and other time-dependent offsets determined from the observed positions of a large number of sources around the sky, and finally converted to the LOS of each detector using the quaternions in the IMO.<br />
<br />
=== LFI processing ===<br />
The input TOIs are in ADUs representing the voltage signal at the output of the electronics (see [[LFI design, qualification, and performance#Radiometer Chain Assembly (RCA) | Radiometer Chain Assembly (RCA)]] for details). The processing applied to remove instrumental effects and to calibrate them is described in detail in the [[TOI processing | LFI TOI processing]] section, and in {{PlanckPapers|planck2014-a03||Planck-2015-A03}} we give a very brief summary here for convenience. That pipeline performs the following operations:<br />
; ADC correction: due to ADC non-linearity under certain condition, this instrumental effect is removed by applying well know templates directly to the diode signal.<br />
; Electronics Spikes: caused by the interaction between the electronics clock and the scientific data lines. The<br />
signal is detected in all the LFI radiometers' time-domain outputs as a 1s square wave with a rising edge near 0.5s <br />
and a falling edge near 0.75s synchronous with the on-board time signal. In the frequency domain it appears as a spike signal at multiples of 1 Hz. The 44 GHz channels are the only LFI outputs significantly affected by this effect. Consequently the spike signal is removed from the data only in these channels.<br />
; Demodulation: each LFI diode switches at 4096 Hz between the sky and the 4K reference load. The data acquired in this way is dominated by 1\f noise that is highly correlated between the two streams; differencing those streams results in a strong reduction of 1\f noise. The procedure applied is described in [[TOI processing | LFI TOI processing]] taking into account that the gain modulation factor R was computed on timestreams with the Galaxy and point sources masked to avoid strong sky signals.<br />
; Diode combination: two detector diodes provide the output for each LFI receiver channel. To minimize the impact of imperfect isolation of the data stream of each diode, we perform a weighted average of the time-ordered data from the two diodes of each receiver. The procedure applied is detailed in [[TOI processing | LFI TOI processing]]; the weights used are kept fixed for the entire mission.<br />
; Scientific Calibration: calibrate the timelines to physical units K<sub>CMB</sub>, fitting the total CMB dipole convolved with the 4pi beam representation, without taking into account the signature due to Galactic straylight;<br />
; Gain regularization: the calibration constants computed using the model of the dipole signal suffer from large uncertainties when the Planck spacecraft is badly aligned with the dipole axis. To reduce the noise, we apply an adaptive smoothing algorithm<br />
that is also designed to preserve the discontinuities caused by abrupt changes in the working configuration of the radiometers<br />
(e.g., sudden temperature changes in the focal plane).<br />
; Removal of solar and orbital dipole signal: the combined solar and orbital dipole is convolved with the 4pi beam representation of each radiometer and the removed from its timeline.<br />
; Removal of Galactic Straylight: the light incident on the focal plane without reflecting on the primary mirror (straylight) is a major source of systematic effects, especially when the Galactic plane intersects the direction of the main spillover. This effect is corrected by removing the estimated straylight signal from the timelines. This signal is computed as the convolution of Galaxy simulation with the beam sidelobes, see details in [[TOI processing | LFI TOI processing]].<br />
<br />
At this point the timelines are used for the production of the maps.<br />
<br />
The pointing (see common [[Detector_pointing | Detector Pointing]] section for details) is determined from the AHF produced by the MOC, which gives the direction and orientation of the LOS of a fiducial position in the focal plane at frequencies of 8Hz during stable pointing and 4 Hz during maneuvers. This is interpolated to the timestamps of data samples, corrected for the wobble and other time-dependent offsets determined from the observed positions of a large number of sources around the sky and temperature sensor, and finally converted to the LOS of each detector.<br />
<br />
==File Names==<br />
<br />
The file names are of the form:<br />
<br />
''{H,L}FI_TOI_{fff}-{SCI,PTG,TAI,OFF}_R2.nn_ODxxxx.fits''<br />
<br />
where<br />
* ''fff'' denotes the frequency<br />
* SCI denote signal TOIs<br />
* PTG denote pointing TOIs<br />
* TAI denote OBT-MJD correlation TOI<br />
* OFF denote Baseline TOI<br />
* R2.nn is the version, and<br />
* ODxxxx indicates the OD.<br />
<br />
<br />
At the present time, HFI is providing signal TOIs for all the SWB (non-polarised) bolometers and for the PSB (polarised) bolometers at 353GHz only. The reasons for this are detailed in [###REF###]. On the other hand, the pointing TOIs are available for all bolometers. LFI is providing all signal TOI.<br />
<br />
==FITS file structure==<br />
<br />
All FITS files begin with a primary extension containing no data and a minimal header, which is followed by one or more ''BINTABLE'' extensions with data, and with a description of the data in the header keywords. In what follows will usually ignore the primary extension, and count only the extensions containing data.<br />
<br />
===TOI files===<br />
<br />
The signal FITS files contain N ,'BINTABLE', data extensions, where N is the number of detectors in that frequency channel. The first extension contains the OBT and its flags, called the ''global'' flags since they apply to all detectors, which is followed by one extension for each detector, containing the signal and its ''local'' flag. The flags columns are written as ''byte'' in which each of the 8 bits (max) encodes one flag timeline. The meaning of each bit is given in the header comments and is subject to change.<br />
For the global flag they include:<br />
* HFI<br />
** Unstable pointing: 1= pointing is not stable (e.g., during repointing maneuvers)<br />
** Dark correlation: 1 = darks are uncorrelated and data are flagged<br />
** First/Second half ring: which samples are in which half (only covers the stable pointing part of the ring)<br />
** HCM: in HCM mode (unstable pointing)<br />
** and more<br />
<br />
* LFI<br />
** Bit 0, unstable pointing: 1= pointing is not stable<br />
** Bit 1, time correlation quality: 1= outside specification<br />
** Bit 2, special observation: 1= special observation like deep scan<br />
<br />
And for the local flag they include<br />
<br />
* HFI<br />
** Total Flag: a combination of the various flags that is the one finally used in the map-making (all samples with Total Flag different from zero should not be used)<br />
** Data not valid: glitched samples<br />
** Despike Common: (for PSBs only) glitch on current or other of PSB pair<br />
** StrongSignal: on Galactic Plane<br />
** Strong Source: on point source<br />
** other<br />
<br />
* LFI<br />
** Bit 0, Data not valid: 1= Science sample not valid<br />
** Bit 2: Planet crossing: 1= Science Sample containing planet<br />
** Bit 3: Moving objects: 1= minor Solar System object (not yet used)<br />
** Bit 4: Gap: 1= this sample was artificially included due to gap in the data<br />
<br />
<br />
<br />
{| border="1" cellpadding="3" cellspacing="0" align="center" style="text-align:left" width=800px<br />
|+ '''TOI file data structure'''<br />
<br />
|- bgcolor="ffdead" <br />
!colspan="5" | 1. EXTNAME = 'OBT' : Data columns<br />
|- bgcolor="ffdead" <br />
! Column Name || Data Type || Units || Description || Comment<br />
|-<br />
|OBT || Int*8 || 2<sup>-16</sup> sec || On-board time ||<br />
|-<br />
|FLAG || Byte || none || the various bit-level flags ||<br />
<br />
|- bgcolor="ffdead" <br />
! Keyword || Data Type || Value || Description || Comment<br />
|-<br />
|OD || Int || || OD covered (as in filename) ||<br />
|-<br />
|BEGIDX || Int || || first sample index of given OD || Only HFI<br />
|-<br />
|ENDIDX || Int || || last sample index of given OD || Only HFI<br />
|-<br />
|BEGRING || Int || || first ring in given OD || Only HFI<br />
|-<br />
|ENDRING || Int || || last ring in given OD || Only HFI<br />
|-<br />
|TIMEZERO || String || 1958-01-01z00:00 || Origin of OBT || Only HFI<br />
|-<br />
|TIMEZERO || Float || 106744000000000. || Origin of OBT || Only LFI<br />
<br />
|- bgcolor="ffdead" <br />
!colspan="5" | n. EXTNAME = ''DETNAME'' : Data columns<br />
<br />
|- bgcolor="ffdead" <br />
! Column Name || Data Type || Units || Description || Comment<br />
|-<br />
|SIGNAL || Real*4 || K<sub>cmb</sub> or MJy/sr || Value of signal || Comment<br />
|-<br />
|FLAG || Byte || none || the various bit-level flags ||<br />
|- bgcolor="ffdead" <br />
<br />
! Keyword || Data Type || Value || Description || Comment<br />
|-<br />
|UNIT || String || || Units of signal || Only HFI, LFI always K<sub>cmb</sub><br />
|-<br />
|DESTRIPE || 1/0 || || whether timeline is destriped || Only HFI<br />
|-<br />
|OD || Int || || OD covered (as in filename) ||<br />
|-<br />
|BEGIDX || Int || || first sample index of given OD || Only HFI<br />
|-<br />
|ENDIDX || Int || || last sample index of given OD || Only HFI<br />
|-<br />
|BEGRING || Int || || first ring in given OD || Only HFI<br />
|-<br />
|ENDRING || Int || || last ring in given OD || Only HFI<br />
|}<br />
<br />
<br />
The pointing files have a similar structure, except that ''DETNAME'' extensions contain 3 columns of Real*8 with the phi, theta, and psi Galactic spherical coordinates of each sample in radians, as shown in the table below. There is no local flag for the coordinates.<br />
<br />
{| border="1" cellpadding="3" cellspacing="0" align="center" style="text-align:left" width=800px<br />
|+ '''Pointing TOI file DETNAME extension structure'''<br />
<br />
|- bgcolor="ffdead" <br />
!colspan="4" | n. EXTNAME = ''DETNAME'' : Data columns<br />
<br />
|- bgcolor="ffdead" <br />
! Column Name || Data Type || Units || Description<br />
|-<br />
|PHI || Real*8 || radian || longitude<br />
|-<br />
|THETA || Real*8 || radian || colatitude<br />
|-<br />
|PSI || Real*8 || radian || roll angle<br />
|}<br />
<br />
===HFI ROI files===<br />
<br />
The files provided by HFI are<br />
* ''HFI_ROI_GlobalParams_RelNum_full.fits''<br />
* ''HFI_ROI_DestripeOffsets_RelNum_full.fits''<br />
which are described below.<br />
<br />
;Global parameters: this ROI file contains a single ''BINTABLE'' extension with 3 columns that give, for each ring, the index number of the first sample, the ESA pointing ID of the ring, and the ring start time. All three are encoded as Int*8, and the time is given in units of 2<sup>-16</sup> sec from ''TIMEZERO'', 1958-01-01z00:00, as in the TOI files. Rings are numbered from 240 to 27005, as given in the ''BEGRING'' and ''ENDRING'' keywords<br />
<br />
; Destriping offsets: this ROI file contains a single ''BINTABLE'' extension with 3 columns that give, for each ring, the offsets to subtract from each bolometer signal timeline or vector. There are three offsets available for each bolometer: full-ring, first half-ring, and second half-ring, for building the full-ring or the two half-ring maps, respectively. The offsets must be subtracted from Index(N) to Index(N+1)-1 of the corresponding signal timeline, where N is the ring number, and the indices are given in the Global parameters file. The offsets are given in the same units as the signal vectors, that is K<sub>cmb</sub> for the 100-353 GHz channels, and MJy/sr for the 545 and 857 GHz channels. All values are encoded as Real*4. The rings for which the offsets are set to 0.000 are [[TOI_processing#Discarded_rings | ''badrings'' ]] which are rejected in the mapmaking process. These rings are also flagged by the ''TotalFlag'', as are the portions of rings longer than ~72.5 min, where the drift in the satellite's spin axis becomes important.<br />
<br />
===TAI TOI files===<br />
<br />
The TAI TOI files contains one extension with two column, the first is the OBT value (exactly the same reported in the SCI TOI), the second the corresponding Modified Julian day. Note that Leap second where not added.<br />
<br />
{| border="1" cellpadding="3" cellspacing="0" align="center" style="text-align:left" width=800px<br />
|+ '''Time TAI TOI file data structure'''<br />
<br />
|- bgcolor="ffdead" <br />
!colspan="5" | 1. EXTNAME = 'OBT-MJD' : Data columns<br />
|- bgcolor="ffdead" <br />
! Column Name || Data Type || Units || Description || Comment<br />
|-<br />
|OBT || Int*8 || 2<sup>-16</sup> sec || On-board time ||<br />
|-<br />
|MJD || Real*8 || day || Modified Julian day ||<br />
|}<br />
<br />
===LFI OFF TOI files===<br />
The OFF (baseline) TOI files adopt the same file structure of the Science TOI files. Note that in case of OFF timelines related to the half-ring, and addition column in included in the OBT extension to define for each sample if it belong to half-ring 1 or half-ring2.<br />
<br />
===LFI HouseKeeping files===<br />
House keeping timelines are:<br />
* LFI_TOI_DAE-FAST-HK_R2.nn_ODxxxx.fits<br />
* LFI_TOI_DAE-SlowConfiguration-HK_R2.nn_ODxxxx.fits<br />
* LFI_TOI_DAE-SlowCurrent-HK_R2.nn_ODxxxx.fits<br />
* LFI_TOI_DAE-SlowPhaseSwitch-HK_R2.nn_ODxxxx.fits<br />
* LFI_TOI_DAE-SlowVoltage-HK_R2.nn_ODxxxx.fits<br />
* LFI_TOI_REBA-HK_R2.nn_ODxxxx.fits<br />
* SCS_TOI_EssentialASW-HK_R2.nn_ODxxxx.fits<br />
* SCS_TOI_NonEssentialASW-HK_R2.nn_ODxxxx.fits<br />
<br />
Each file contains two extension, the first is the OBT (value are sampled at 1 or 10 seconds), the latter contain a variable number of column = 2* number of HouseKeeping stored. Each Housekeeping is accompanied by its flag (normally 0 is NOT 0 the value was considerate invalid or Out Of Limit). The Housekeeping name are the once defined in the LFI Instrnument Operation Manual.<br />
<br />
<br />
<span style="color:red"> TBW: Note on half-ring offsets, which differ by 1-2% from full ring offsets</span> <br />
<br />
== References ==<br />
<br />
<References /><br />
<br />
[[Category:Mission products|001]]</div>
Xdupac
https://wiki.cosmos.esa.int/planckpla2015/index.php?title=HFI/LFI_joint_data_processing&diff=11416
HFI/LFI joint data processing
2015-02-05T10:33:14Z
<p>Xdupac: </p>
<hr />
<div>The HFI / LFI common processing uses as basic input the maps at the nine frequencies covered by the two instruments. <br />
<br />
The goal is to obtain various catalogues, identify the different astrophysical components whose superposition leads to the observed sky, and provide a statistical characterisation of the CMB, in particular through a likelihood code (of a particular theoretical <math>C(\ell)</math> given Planck data).<br />
<br />
<br />
[[Category:HFI/LFI joint data processing|000]]</div>
Xdupac
https://wiki.cosmos.esa.int/planckpla2015/index.php?title=HFI-Validation&diff=11413
HFI-Validation
2015-02-05T10:28:23Z
<p>Xdupac: /* Generic approach to systematics */</p>
<hr />
<div>{{DISPLAYTITLE:Internal overall validation}}<br />
<br />
The HFI validation is mostly modular. That is, each part of the pipeline, be it timeline processing, map-making, or any other, validates the results of its work at each step of the processing, looking specifically for known issues. In addition, we do additional validation with an eye towards overall system integrity by looking at generic differences between sets of maps, in which most problems will become apparent, whether known or not. Both these are described below. <br />
<br />
==Expected systematics and tests (bottom-up approach)==<br />
<br />
Like all experiments, Planck/HFI had a number of "issues" which it needed to track and verify were not compromising the data. While these are discussed in appropriate sections, here we gather them together to give brief summaries of the issues and refer the reader to the appropriate section for more details. <br />
<br />
* Cosmic Rays - Unprotected by the atmosphere and more sensitive than previous bolometric experiments, HFI saw many more cosmic ray hits than previous experiments. These were detected, the worst parts of the data flagged as unusable, and "tails" were modeled and removed. This is described in [[TOI_processing#Glitch_statistics|the section on glitch statistics]]<!-- and in [[#Cosmic_rays|the section on cosmic rays]],--> as well as in {{PlanckPapers|planck2013-p03e|1|the 2013 HFI Cosmic Ray Removal paper}}.<br />
* Elephants - Cosmic rays also hit the HFI 100 mK stage and cause the temperature to vary, inducing small temperature and thus noise variations in the detectors. These are removed with the rest of the thermal fluctuations, described directly below. <br />
* Thermal Fluctuations - HFI is an extremely stable instrument, but there are small thermal fluctuations. These are discussed in [[TOI_processing#Thermal_template_for_decorrelation|the timeline processing section on thermal decorrelation]]<!-- and in [[#1.6K_and_4K_stage_fluctuations|the section on 1.6 K and 4 K thermal fluctuations]]-->.<br />
* Random Telegraphic Signal (RTS) or Popcorn Noise - Some channels were occasionally affected by what seems to be a baseline which abruptly changes between two levels, which has been variously called popcorn noise or random telegraphic signal. These data are usually flagged. This is described in [[TOI_processing#Noise_stationarity|the section on noise stationarity]]<!-- and [[#RTS_noise|the section on Random Telegraphic Signal Noise]]-->.<br />
* Jumps - Similar to but distinct from popcorn noise, small jumps were occasionally found in the data streams. These data are usually corrected. This is described in [[TOI_processing#jump_correction|the section on jump corrections]]. <br />
* 4 K Cooler-Induced EM Noise - The 4 K cooler induced noise in the detectors with very specific frequency signatures, which is filtered. This is described in {{PlanckPapers|planck2013-p03|1|the 2013 HFI DPC Paper}}<!--, [[#4K_lines_Residuals|the section below on 4 K line residuals]]-->, and their stability is discussed in [[TOI_processing#4K_cooler_lines_variability|the section on 4 K cooler line stability]].<br />
* Compression - On-board compression is used to overcome our telemetry bandwidth limitations. This is explained in {{PlanckPapers|planck2011-1-5}}. <br />
* Noise Correlations - Correlations in noise between detectors seems to be negligible but for two polarization sensitive detectors in the same horn. This is discussed in {{PlanckPapers|planck2013-p03e|1|the 2013 HFI Cosmic Ray Removal paper}}.<br />
* Pointing - The final pointing reconstruction for Planck is near the arcsecond level. This is discussed in {{PlanckPapers|planck2013-p03|1|the 2013 HFI DPC Paper}}.<br />
* Focal Plane Geometry - The relative positions of different horns in the focal plane is reconstructed using planets. This is also discussed in {{PlanckPapers|planck2013-p03|1|the 2013 HFI DPC paper}}. <br />
* Main Beam - The main beams for HFI are discussed in the {{PlanckPapers|planck2013-p03d|1|2013 Beams and Transfer function paper}}. <br />
* Ruze Envelope - Random imperfections or dust on the mirrors can increase the size of the beam a bit. This is discussed in {{PlanckPapers|planck2013-p03d|1|the 2013 Beams and Transfer function paper}}.<br />
* Dimpling - The mirror support structure causes a pattern of small imperfections in the beams, which cause small sidelobe responses outside the main beam. This is discussed in {{PlanckPapers|planck2013-p03d|1|the 2013 Beams and Transfer function paper}}.<br />
* Far Sidelobes - Small amounts of light can sometimes hit the detectors from just above the primary or secondary mirrors, or even from reflecting off the baffles. While small, when the Galactic center is in the right position, this can be detected in the highest frequency channels, so this is removed from the data. This is discussed in {{PlanckPapers|planck2013-p03d|1|the 2013 Beams and Transfer function paper}} and, non-intuitively, {{PlanckPapers|planck2013-pip88|1|the 2013 Zodiacal emission paper}}. <br />
* Planet Fluxes - Comparing the known fluxes of planets with the calibration on the CMB dipole is a useful check of calibration for the CMB channels, and is the primary calibration source for the submillimeter channels. This is done in {{PlanckPapers|planck2013-p03b|1|the 2013 Map-Making and Calibration Paper}}. <br />
* Point Source Fluxes - As with planet fluxes, we also compare fluxes of known, bright point sources with the CMB dipole calibration. This is done in {{PlanckPapers|planck2013-p03b|1|the 2013 Map-Making and Calibration paper}}. <br />
* Time Constants - The HFI bolometers do not react instantaneously to light; there are small time constants, discussed in {{PlanckPapers|planck2013-p03d|1|the 2013 Beams and Transfer function paper}}. <br />
* ADC Correction - The HFI Analog-to-Digital Converters are not perfect, and are not used perfectly. While this is an on-going effort, their effects on the calibration are discussed in {{PlanckPapers|planck2013-p03c|1|the 2013 Map-Making and Calibration paper}}.<br />
<!--* Gain changes with Temperature Changes--><br />
<!--* Optical Cross-Talk - This is negligible, as noted in [[#Optical_Cross-Talk|the optical cross-talk note]]. --><br />
* Bandpass - The transmission curves, or "bandpass" has shown up in a number of places. This is discussed in {{PlanckPapers|planck2013-p03d|1|the 2013 spectral response paper}}. <br />
<!--* Saturation - While this is mostly an issue only for Jupiter observations, it should be remembered that the HFI detectors cannot observe arbitrarily bright objects. This is discussed in [[#Saturation|the section below on saturation]].--><br />
<br />
<!---==Generic approach to systematics==<br />
<br />
<font style="color:red;font-size:300%">This section is Under (Re-)Construction</font><br />
<br />
Some (null) tests done at the map level are described in the HFI map making paper (REf).<br />
<br />
Some further tests will be described in the "CMB power spectra and liklihood paper".<br />
<br />
Finally detailed End-to-end simulations (from lowest level instrument behaviour to maps) are still ongoing for a detailed characterisation, which will accompany the 100-217GHz polarisation maps when they will be made available, probably before the summer 2015.---><br />
<br />
==References==<br />
<br />
<References /><br />
<br />
<br />
<br />
[[Category:HFI data processing|006]]</div>
Xdupac
https://wiki.cosmos.esa.int/planckpla2015/index.php?title=Map-making&diff=11411
Map-making
2015-02-05T10:27:20Z
<p>Xdupac: /* Map validation */</p>
<hr />
<div>{{DISPLAYTITLE:Map-making and photometric calibration}}<br />
== Introduction ==<br />
<br />
This page will give an overview of the map-making and photometric calibration procedures used by the HFI DPC to build detector and frequency maps for the 2015 data release. <br />
They are described in <span style="color:Red">Planck-2015-VIII ref</span>.<br />
These have common elements with the tools used for the 2013 release that are described in {{PlanckPapers|planck2013-p03}} and {{PlanckPapers|planck2013-p03b}}. <br />
<br />
To build HFI maps, we use the destriping approximation, in which noise is assumed to decompose into two components : white noise plus low frequency drifts. Using the sky redundancy, the low frequency drifts are modelled as one constant, or offset, per pointing period. To speed up the ulterior processing we first build intermediate products, by taking advantage of redundancies : we average signal and detector orientation on healpix pixels visited during <br />
each fixed pointing period, which we call hereafter 'ring'. Detector's pointing are corrected for slow drifts and aberration (displacement on the sky indouced by the satellite's motion). This intermediate product is called HPR for healpix pixel ring. They have been constructed using the same map resolution as the final HFI products (corresponding to <math>N_{\mathrm side}</math>=2048). <br />
This new dataset is used as input in the following steps.<br />
<br />
== Photometric calibration ==<br />
<br />
=== Dipole calibration (100 to 353 GHz) ===<br />
<br />
For the 2015 data release, the HFI CMB channels were calibrated using the orbital dipole modulation. This time-variable anisotropy results from the motion of the spacecraft in the solar system, which is precisely measured. Thus it provides an absolute calibrator for orbital CMB missions. Its measurement is now used to calibrate HFI data thanks to the improvements in the timne stability of the data <br />
brought by the ADC non-linearities corrections and a better control for the detectors time response. <br />
<br />
Residual time response slow components are modeled as a dipole shifted by 90 degrees in phase, whose amplitude is fitted bolometer per bolometer. To mitigate residual systematics, we perform a simultaneous fit of the detectors gains on the orbital dipole. This amounts to solve the non-linear equation : <br />
<math> \displaystyle{d\ =\ g_i.(S+D) + O_i + n}<br />
\label{nlequat}</math><br />
<br />
where d is s the detector measurement, D the total dipole component, n the (white) noise, and both S the sky signal, g the detector gain, O the offset (for ring no i) are the unknowns to be determined. <br />
This is done by linearizing it to look for gains and sky variations, and iterating by updating the approximate sky and gains. <br />
<br />
<br />
=== Higher frequency calibration (545 and 857 GHz) ===<br />
<br />
We therefore the sub-mm channels' calibration for the 2015 Planck data release from the comparison of measurements of the Neptune and Uranus fluxes (with aperture photometry) with their expectations from the Moreno et al model of their atmospheres' emission. This procedure is justified, since for both planets, at the lower frequencies (100-353 Ghz), the fluxes we recover are in agreement within ~ +/-5\% with what is expected from the planet spectral model, and the HFI detector's band-passes.<br />
<br />
=== Zero levels === <br />
We determined zero-level for the released maps in selected regions of the sky where dust emissions are low and well correlated with HI. We may thus estimate and subtract dust emissions using the HI template, and CMB from a Planck component-separated template. The remaining astrophysical zero level is that of CIB. By imposing that the level we find is equal to that of the CIB model of Bethermin et al, we set the zero level of our maps.<br />
<br />
<br />
== Building of maps == <br />
<br />
Using the photometric calibration parameters, we build maps in two steps : <br />
<br />
* we determine the destriping offsets using the full mission data for all detectors of a given frequency<br />
* we build the maps, using these offsets, by inverting the photometric equation :<br />
<br />
<math> \displaystyle{d_i = g(I^p+\eta [Q^p cos(2\psi_i) + U^p sin(2\psi_i)]) + n}<br />
\label{photeq}</math><br />
where d is the destriped and calibrated signal at the HPR level. Detector's data are combined with an inverse noise weights derived from each detector's NEP. Q and U maps are build whenever possible. We propagate the white noise by building the 3x3 (or 1x1 if only I is reconstructed) covariance matrices in each pixel. <br />
At each frequency we build maps combining all detectors and independent detector sets. <br />
We use the offsets build for the full mission for building maps for each scan survey, year (sombineation of surveys 1 and 2 or 3 and 4 respectively) and for the full, nominal mission duration and its two halves. <br />
We also build maps from the two independent halves of each rings. Altogether, more than 8000 maps are built at each release. <br />
<br />
HPR and Maps are built in galactic coordinates.<br />
<br />
== Noise properties ==<br />
<br />
Map noise properties can be evaluated using several methods, thanks to the high level of observation redundancies. <br />
We can use the maps built from the difference between the first and second half of each rings, or compare individual sky scans, years, half-mission or independent detector sets with each other. <br />
Some of these tests are described in <span style="color:Red">Planck-2015-VIII ref</span>.<br />
<br />
Low resolution (nside = 8, 16) pixel-to-pixel noise covariance matrices are build using an analytic approach from the measured noise power spectra.<br />
<br />
== Zodiacal light correction ==<br />
<br />
At the highest Planck frequencies, zodiacal light emission is visible in a survey difference map:<br />
<br />
[[File:Z857SurveyJackknifeWiZodi.png|500px|thumb|center|2013 Release 857 GHz Survey 2 - Survey 1 Difference]]<br />
<br />
This map is a difference between the 857 GHz Survey 2 map and the 857 GHz Survey 1 map. This difference effectively removes Galactic and other emissions which originate far from Planck. As the Solar elongation is different for measurements of the same point on the sky for the two surveys, we see zodiacal light emission, while all emission from further sources is removed. The zodiacal light emission follows the Ecliptic plane, which starts at the lower left of the image, then crosses the center of the plot towards the upper right. Note that the "arcs" at the top and bottom of the image are images of the Galactic center in the Far Sidelobes, which are discussed in the section below. Similar plots for other HFI frequencies, for maps both before and after removal, are shown [[beforeAndAfterSurveyDifferences|here]].<br />
<br />
For the 2015 Planck release, zodiacal light emission is removed from all HFI channels. The general procedure is described in {{PlanckPapers|planck2013-p03}}, but a synopsis of the procedure is as follows:<br />
* During each survey, a large fraction of the sky has observations which all fall within a week of each other. That is, during a single survey, most pixels are observed during a short, well-defined period. The contribution from zodiacal light emission to the total brightness seen, then, is well defined. <br />
* We use the the COBE model of the zodiacal light emission to make predictions for this zodiacal light emission for those pixels observed over a span of one week or less. The templates from the COBE model are shown [[COBEZodiModelTemplates|here]].<br />
* We fit the survey difference maps with these model templates to estimate the emissivity of each zodi component at the Planck wavelengths. The results of these fits at each frequency are given in <span style="color:red">Planck-2015-VIII</span>. <br />
* We reconstruct each ring of the the full mission using the combination of the COBE geometric model with the emissivities determined above. <br />
* We remove the reconstruction above from each ring of data. <br />
* We then make maps as described previously in this section.<br />
<br />
== Far SideLobes (FSL)==<br />
<br />
Contrary to the 2013 Planck release, Far Sidelobes were not removed from the HFI data for the 2015 Planck release. <br />
The change of the gain due to neglect of the far sidelobes is calculated by fitting the dipole to full timeline simulations of the dipole convolved by the FSL. The correction factors applied to the data are 0.09 % at 100 GHz, 0.05 % at 143 GHz, 0.04 % at 217 GHz and negligible at 353 GHz. Corrections were not made at 545 and 857 GHz <span style="color:red">(see Planck-2015-VIII for details)</span>.<br />
<br />
== CO maps ==<br />
<br />
Carbon monoxide rotational transition line emission is present in all HFI bands but for the 143 GHz<br />
channel. It is especially significant in the 100, 217 and 353 GHz channels (due to the 115<br />
(1-0), 230 (2-1) and 345 GHz (3-2) CO transitions). This emission comes essentially from<br />
the Galactic interstellar medium and is mainly located at low and intermediate Galactic<br />
latitudes. Three approaches (summarised below) have been used to extract CO velocity<br />
integrated emission maps from HFI maps and to generate the CO products. See<br />
Planck-2013-XIII and Planck-2015-X for a full description.<br />
<br />
*Type 1 product: it is based on a single channel approach using the fact that each CO<br />
line has a slightly different transmission in each bolometer at a given frequency channel.<br />
From this, the J=1-0, J=2-1 and J=3-2 CO lines can be extracted independently. As this<br />
approach is based on individual bolometer maps of a single channel, the resulting<br />
Signal-to-Noise ratio (SNR) is relatively low. The benefit, however, is that these maps do<br />
not suffer from contamination from other HFI channels (as is the case for the other<br />
approaches) and are more reliable, especially in the Galactic plane. <br />
<br />
*Type 2 product: this product is obtained using a multi-frequency approach. Three<br />
frequency channel maps are combined to extract the J=1-0 (using the 100, 143 and 353<br />
GHz channels) and J=2-1 (using the 143, 217 and 353 GHz channels) CO maps. As<br />
frequency maps are combined, the spectral behaviour of other foregrounds influences<br />
the result. The two Type 2 CO maps produced in this way have a higher SNR than the<br />
Type 1 maps at the cost of a larger residual contamination from other diffuse<br />
foregrounds.<br />
<br />
* Type 3 product: no Type 3 product (as defined in 2013) has been produced for the<br />
2015 release. Instead, it is superseded by a high-resolution CO(2-1) map (FWHM=7.5<br />
arcmin) produced by the Commander component separation pipeline. Note that low<br />
resolution (FWHM=1 deg) CO maps of the three lines have also been produced using<br />
Commander. See [le lien vers la section avant-plans de Commander] for a complete<br />
description.<br />
<br />
The 2015 Type 1 and Type 2 CO maps have been produced using the same procedure as<br />
for the 2013 results. Very similar to their 2013 counterparts, the 2015 maps benefit from<br />
an increased SNR due to the use of the full, rather than nominal, mission data. <br />
Characteristics of the released maps are the following. We provide Healpix maps with<br />
Nside=2048. For one transition, the CO velocity-integrated line signal map is given in<br />
K_RJ.km/s units. A conversion factor from this unit to the native unit of HFI maps (K_CMB)<br />
is provided in the header of the data files and in the RIMO. Four maps are given per<br />
transition and per type:<br />
* The signal map<br />
* The standard deviation map (same unit as the signal),<br />
* A null test noise map (same unit as the signal) with similar statistical properties. It is<br />
made out of half the difference of half-ring maps.<br />
* A mask map (0B or 1B) giving the regions (1B) where the CO measurement is not<br />
reliable because of some severe identified foreground contamination. <br />
All products of a given type belong to a single file. Type 1 products have the native HFI<br />
resolution i.e. approximately 10, 5 and 5 arcminutes for the CO 1-0, 2-1, 3-2 transitions<br />
respectively. Type 2 products have a 15 arcminute resolution.<br />
We refer the reader to [le lien vers la section avant-plans de Commander] for a<br />
description and characteristics of the Commander CO products.<br />
<br />
== Map validation ==<br />
<br />
Several validations of HFI maps are described in <span style="color:Red">Planck-2015-VII ref</span> and in <span style="color:Red">Planck-2015-VIII ref</span>. <br />
<br />
Further checks are presented in the likelihood, parameters, component separation, and Commander papers.<br />
<br />
== References ==<br />
<References /><br />
<br />
<br />
[[Category:HFI data processing|004]]</div>
Xdupac
https://wiki.cosmos.esa.int/planckpla2015/index.php?title=Map-making&diff=11410
Map-making
2015-02-05T10:26:36Z
<p>Xdupac: /* Noise properties */</p>
<hr />
<div>{{DISPLAYTITLE:Map-making and photometric calibration}}<br />
== Introduction ==<br />
<br />
This page will give an overview of the map-making and photometric calibration procedures used by the HFI DPC to build detector and frequency maps for the 2015 data release. <br />
They are described in <span style="color:Red">Planck-2015-VIII ref</span>.<br />
These have common elements with the tools used for the 2013 release that are described in {{PlanckPapers|planck2013-p03}} and {{PlanckPapers|planck2013-p03b}}. <br />
<br />
To build HFI maps, we use the destriping approximation, in which noise is assumed to decompose into two components : white noise plus low frequency drifts. Using the sky redundancy, the low frequency drifts are modelled as one constant, or offset, per pointing period. To speed up the ulterior processing we first build intermediate products, by taking advantage of redundancies : we average signal and detector orientation on healpix pixels visited during <br />
each fixed pointing period, which we call hereafter 'ring'. Detector's pointing are corrected for slow drifts and aberration (displacement on the sky indouced by the satellite's motion). This intermediate product is called HPR for healpix pixel ring. They have been constructed using the same map resolution as the final HFI products (corresponding to <math>N_{\mathrm side}</math>=2048). <br />
This new dataset is used as input in the following steps.<br />
<br />
== Photometric calibration ==<br />
<br />
=== Dipole calibration (100 to 353 GHz) ===<br />
<br />
For the 2015 data release, the HFI CMB channels were calibrated using the orbital dipole modulation. This time-variable anisotropy results from the motion of the spacecraft in the solar system, which is precisely measured. Thus it provides an absolute calibrator for orbital CMB missions. Its measurement is now used to calibrate HFI data thanks to the improvements in the timne stability of the data <br />
brought by the ADC non-linearities corrections and a better control for the detectors time response. <br />
<br />
Residual time response slow components are modeled as a dipole shifted by 90 degrees in phase, whose amplitude is fitted bolometer per bolometer. To mitigate residual systematics, we perform a simultaneous fit of the detectors gains on the orbital dipole. This amounts to solve the non-linear equation : <br />
<math> \displaystyle{d\ =\ g_i.(S+D) + O_i + n}<br />
\label{nlequat}</math><br />
<br />
where d is s the detector measurement, D the total dipole component, n the (white) noise, and both S the sky signal, g the detector gain, O the offset (for ring no i) are the unknowns to be determined. <br />
This is done by linearizing it to look for gains and sky variations, and iterating by updating the approximate sky and gains. <br />
<br />
<br />
=== Higher frequency calibration (545 and 857 GHz) ===<br />
<br />
We therefore the sub-mm channels' calibration for the 2015 Planck data release from the comparison of measurements of the Neptune and Uranus fluxes (with aperture photometry) with their expectations from the Moreno et al model of their atmospheres' emission. This procedure is justified, since for both planets, at the lower frequencies (100-353 Ghz), the fluxes we recover are in agreement within ~ +/-5\% with what is expected from the planet spectral model, and the HFI detector's band-passes.<br />
<br />
=== Zero levels === <br />
We determined zero-level for the released maps in selected regions of the sky where dust emissions are low and well correlated with HI. We may thus estimate and subtract dust emissions using the HI template, and CMB from a Planck component-separated template. The remaining astrophysical zero level is that of CIB. By imposing that the level we find is equal to that of the CIB model of Bethermin et al, we set the zero level of our maps.<br />
<br />
<br />
== Building of maps == <br />
<br />
Using the photometric calibration parameters, we build maps in two steps : <br />
<br />
* we determine the destriping offsets using the full mission data for all detectors of a given frequency<br />
* we build the maps, using these offsets, by inverting the photometric equation :<br />
<br />
<math> \displaystyle{d_i = g(I^p+\eta [Q^p cos(2\psi_i) + U^p sin(2\psi_i)]) + n}<br />
\label{photeq}</math><br />
where d is the destriped and calibrated signal at the HPR level. Detector's data are combined with an inverse noise weights derived from each detector's NEP. Q and U maps are build whenever possible. We propagate the white noise by building the 3x3 (or 1x1 if only I is reconstructed) covariance matrices in each pixel. <br />
At each frequency we build maps combining all detectors and independent detector sets. <br />
We use the offsets build for the full mission for building maps for each scan survey, year (sombineation of surveys 1 and 2 or 3 and 4 respectively) and for the full, nominal mission duration and its two halves. <br />
We also build maps from the two independent halves of each rings. Altogether, more than 8000 maps are built at each release. <br />
<br />
HPR and Maps are built in galactic coordinates.<br />
<br />
== Noise properties ==<br />
<br />
Map noise properties can be evaluated using several methods, thanks to the high level of observation redundancies. <br />
We can use the maps built from the difference between the first and second half of each rings, or compare individual sky scans, years, half-mission or independent detector sets with each other. <br />
Some of these tests are described in <span style="color:Red">Planck-2015-VIII ref</span>.<br />
<br />
Low resolution (nside = 8, 16) pixel-to-pixel noise covariance matrices are build using an analytic approach from the measured noise power spectra.<br />
<br />
== Zodiacal light correction ==<br />
<br />
At the highest Planck frequencies, zodiacal light emission is visible in a survey difference map:<br />
<br />
[[File:Z857SurveyJackknifeWiZodi.png|500px|thumb|center|2013 Release 857 GHz Survey 2 - Survey 1 Difference]]<br />
<br />
This map is a difference between the 857 GHz Survey 2 map and the 857 GHz Survey 1 map. This difference effectively removes Galactic and other emissions which originate far from Planck. As the Solar elongation is different for measurements of the same point on the sky for the two surveys, we see zodiacal light emission, while all emission from further sources is removed. The zodiacal light emission follows the Ecliptic plane, which starts at the lower left of the image, then crosses the center of the plot towards the upper right. Note that the "arcs" at the top and bottom of the image are images of the Galactic center in the Far Sidelobes, which are discussed in the section below. Similar plots for other HFI frequencies, for maps both before and after removal, are shown [[beforeAndAfterSurveyDifferences|here]].<br />
<br />
For the 2015 Planck release, zodiacal light emission is removed from all HFI channels. The general procedure is described in {{PlanckPapers|planck2013-p03}}, but a synopsis of the procedure is as follows:<br />
* During each survey, a large fraction of the sky has observations which all fall within a week of each other. That is, during a single survey, most pixels are observed during a short, well-defined period. The contribution from zodiacal light emission to the total brightness seen, then, is well defined. <br />
* We use the the COBE model of the zodiacal light emission to make predictions for this zodiacal light emission for those pixels observed over a span of one week or less. The templates from the COBE model are shown [[COBEZodiModelTemplates|here]].<br />
* We fit the survey difference maps with these model templates to estimate the emissivity of each zodi component at the Planck wavelengths. The results of these fits at each frequency are given in <span style="color:red">Planck-2015-VIII</span>. <br />
* We reconstruct each ring of the the full mission using the combination of the COBE geometric model with the emissivities determined above. <br />
* We remove the reconstruction above from each ring of data. <br />
* We then make maps as described previously in this section.<br />
<br />
== Far SideLobes (FSL)==<br />
<br />
Contrary to the 2013 Planck release, Far Sidelobes were not removed from the HFI data for the 2015 Planck release. <br />
The change of the gain due to neglect of the far sidelobes is calculated by fitting the dipole to full timeline simulations of the dipole convolved by the FSL. The correction factors applied to the data are 0.09 % at 100 GHz, 0.05 % at 143 GHz, 0.04 % at 217 GHz and negligible at 353 GHz. Corrections were not made at 545 and 857 GHz <span style="color:red">(see Planck-2015-VIII for details)</span>.<br />
<br />
== CO maps ==<br />
<br />
Carbon monoxide rotational transition line emission is present in all HFI bands but for the 143 GHz<br />
channel. It is especially significant in the 100, 217 and 353 GHz channels (due to the 115<br />
(1-0), 230 (2-1) and 345 GHz (3-2) CO transitions). This emission comes essentially from<br />
the Galactic interstellar medium and is mainly located at low and intermediate Galactic<br />
latitudes. Three approaches (summarised below) have been used to extract CO velocity<br />
integrated emission maps from HFI maps and to generate the CO products. See<br />
Planck-2013-XIII and Planck-2015-X for a full description.<br />
<br />
*Type 1 product: it is based on a single channel approach using the fact that each CO<br />
line has a slightly different transmission in each bolometer at a given frequency channel.<br />
From this, the J=1-0, J=2-1 and J=3-2 CO lines can be extracted independently. As this<br />
approach is based on individual bolometer maps of a single channel, the resulting<br />
Signal-to-Noise ratio (SNR) is relatively low. The benefit, however, is that these maps do<br />
not suffer from contamination from other HFI channels (as is the case for the other<br />
approaches) and are more reliable, especially in the Galactic plane. <br />
<br />
*Type 2 product: this product is obtained using a multi-frequency approach. Three<br />
frequency channel maps are combined to extract the J=1-0 (using the 100, 143 and 353<br />
GHz channels) and J=2-1 (using the 143, 217 and 353 GHz channels) CO maps. As<br />
frequency maps are combined, the spectral behaviour of other foregrounds influences<br />
the result. The two Type 2 CO maps produced in this way have a higher SNR than the<br />
Type 1 maps at the cost of a larger residual contamination from other diffuse<br />
foregrounds.<br />
<br />
* Type 3 product: no Type 3 product (as defined in 2013) has been produced for the<br />
2015 release. Instead, it is superseded by a high-resolution CO(2-1) map (FWHM=7.5<br />
arcmin) produced by the Commander component separation pipeline. Note that low<br />
resolution (FWHM=1 deg) CO maps of the three lines have also been produced using<br />
Commander. See [le lien vers la section avant-plans de Commander] for a complete<br />
description.<br />
<br />
The 2015 Type 1 and Type 2 CO maps have been produced using the same procedure as<br />
for the 2013 results. Very similar to their 2013 counterparts, the 2015 maps benefit from<br />
an increased SNR due to the use of the full, rather than nominal, mission data. <br />
Characteristics of the released maps are the following. We provide Healpix maps with<br />
Nside=2048. For one transition, the CO velocity-integrated line signal map is given in<br />
K_RJ.km/s units. A conversion factor from this unit to the native unit of HFI maps (K_CMB)<br />
is provided in the header of the data files and in the RIMO. Four maps are given per<br />
transition and per type:<br />
* The signal map<br />
* The standard deviation map (same unit as the signal),<br />
* A null test noise map (same unit as the signal) with similar statistical properties. It is<br />
made out of half the difference of half-ring maps.<br />
* A mask map (0B or 1B) giving the regions (1B) where the CO measurement is not<br />
reliable because of some severe identified foreground contamination. <br />
All products of a given type belong to a single file. Type 1 products have the native HFI<br />
resolution i.e. approximately 10, 5 and 5 arcminutes for the CO 1-0, 2-1, 3-2 transitions<br />
respectively. Type 2 products have a 15 arcminute resolution.<br />
We refer the reader to [le lien vers la section avant-plans de Commander] for a<br />
description and characteristics of the Commander CO products.<br />
<br />
== Map validation ==<br />
<br />
Several validations of HFI maps are described in <span style="color:Red">Planck-2015-VII ref</span> and in <span style="color:Red">Planck-2015-VIII ref</span>. <br />
<br />
Further checks are presented in the <span style="color:Red"> likelihood, params, comsep and commander papers refs </span>.<br />
<br />
== References ==<br />
<References /><br />
<br />
<br />
[[Category:HFI data processing|004]]</div>
Xdupac
https://wiki.cosmos.esa.int/planckpla2015/index.php?title=Product_Table_for_PLAv2&diff=11409
Product Table for PLAv2
2015-02-05T10:24:05Z
<p>Xdupac: /* Other products */</p>
<hr />
<div>{{DISPLAYTITLE:Products table for PLAv2}}<br />
==Product categories==<br />
*New products for this release that I believe have been confirmed appear in <span style="color:Blue">blue font</span>, products that are still TBC in <span style="color:Red">red font</span> (if it is one entire category of products I will just use color in the products category name, e.g. <span style="color:Blue">1 year maps</span>). Please check this in the tables and let me know whether there are any errors.<br />
*The Obs column contains links to notes at the end of each table. Please check the notes and let me know your feedback.<br />
*More general comments appear at the end of the numbered notes.<br />
<br />
I suggest you use the [[Talk:Product_Table_for_PLAv2|discussion page associated with this page]] to provide your feedback or make any comments relate to the list of products. The discussion page has the same structures in terms of sections as this page. Please try to write your comments/feedback in the appropriate section. I would also ask you to put your initials in the comments you write so that I can more easily get back to you to try to clarify any questions. Yes, it is true I can find out who wrote what in the history page but it makes my life easier if you associate your name to the comments you provide.<br />
<br />
The '''Description''' column will be used to add a one line description of the product that will appear in the archive as a tooltip associated with the product to allow a quick identification by users.<br />
===Time Series===<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=1050px<br />
|+ '''FITS filenames'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" rowspan="9" | <span style="color:Blue">Detector timeseries</span><br />
|rowspan="3" align="center" | LFI <br />
| LFI_TOI_030-SCI_R2.xx_ODXXXX.fits<br />
| <br />
| <br />
|00 <br />
| 10-09-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| LFI_TOI_044-SCI_R2.xx_ODXXXX.fits<br />
| <br />
| <br />
| 00<br />
| 10-09-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| LFI_TOI_070-SCI_R2.xx_ODXXXX.fits<br />
| <br />
| <br />
| 00<br />
| 10-09-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
|rowspan="6" align="center" | HFI <br />
| HFI_TOI_100-SCI_R2.xx_ODXXXX.fits<br />
| Only PSB: not for Feb. 2015 release<br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
|<br />
|-<br />
| HFI_TOI_143-SCI_R2.xx_ODXXXX.fits<br />
| without PSBs<br />
| <br />
| 00<br />
| 20/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_TOI_217-SCI_R2.xx_ODXXXX.fits<br />
| without PSBs<br />
| <br />
| 00<br />
| 20/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_TOI_353-SCI_R2.xx_ODXXXX.fits<br />
| with PSBs<br />
| <br />
| 00<br />
| 19/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_TOI_545-SCI_R2.xx_ODXXXX.fits<br />
| <br />
| <br />
| 00<br />
| 23/01/2015<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_TOI_857-SCI_R2.xx_ODXXXX.fits<br />
| <br />
| <br />
| 00<br />
| 23/01/2015<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="7" | <span style="color:Blue">Offsets</span><br />
| rowspan="6" align="center"| LFI <br />
| LFI_TOI_030-OFF_R2.xx_ODXXXX-full.fits<br />
| <br />
| <br />
| 00<br />
| 19-09-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_TOI_044-OFF_R2.xx_ODXXXX-full.fits<br />
| <br />
| <br />
| 00<br />
| 19-09-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_TOI_070-OFF_R2.xx_ODXXXX-full.fits<br />
| <br />
| <br />
|00<br />
| 19-09-2014 <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_TOI_030-OFF_R2.xx_ODXXXX-full-ringhalf.fits<br />
| <br />
| <br />
| 00<br />
| 11-11-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_TOI_044-OFF_R2.xx_ODXXXX-full-ringhalf.fits<br />
| <br />
| <br />
| 00<br />
| 11-11-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_TOI_070-OFF_R2.xx_ODXXXX-full-ringhalf.fits<br />
| <br />
| <br />
| 00<br />
| 11-11-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
|align="center"| HFI <br />
| HFI_TOI_AllFreqs-OFF_R2.xx.fits<br />
|<br />
|<br />
|00<br />
|13/01/2015<br />
|style="background-color: green;" |<br />
|style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan=9| <span style="color:Blue">Pointing</span><br />
| align="center" rowspan="3"| LFI <br />
| LFI_TOI_030-PTG_R2.xx_ODXXXX.fits <br />
|<br />
| <br />
|00 <br />
|18-07-2014 <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_TOI_044-PTG_R2.xx_ODXXXX.fits <br />
|<br />
| <br />
| 00 <br />
| 18-07-2014 <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_TOI_070-PTG_R2.xx_ODXXXX.fits <br />
|<br />
| <br />
| 00 <br />
| 18-07-2014 <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| rowspan=6 align="center"| HFI <br />
| HFI_TOI_100-PTG_R2.xx_ODXXXX.fits <br />
|<br />
| <br />
| 01 <br />
| 26-08-2014 <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_TOI_143-PTG_R2.xx_ODXXXX.fits <br />
|<br />
| <br />
| 01 <br />
| 26-08-2014 <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_TOI_217-PTG_R2.xx_ODXXXX.fits <br />
|<br />
| <br />
| 01 <br />
| 26-08-2014 <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_TOI_353-PTG_R2.xx_ODXXXX.fits <br />
|<br />
| <br />
| 01 <br />
| 26-08-2014 <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_TOI_545-PTG_R2.xx_ODXXXX.fits <br />
|<br />
| <br />
| 01 <br />
| 26-08-2014 <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_TOI_857-PTG_R2.xx_ODXXXX.fits <br />
|<br />
| <br />
| 01 <br />
| 26-08-2014 <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="4"| <span style="color:Blue">Time stamps</span><br />
| align="center" rowspan="3"| LFI <br />
| LFI_TOI_030-TAI_R2.xx_ODXXXX.fits <br />
|<br />
| <br />
|00 <br />
| 20-09-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_TOI_044-TAI_R2.xx_ODXXXX.fits <br />
|<br />
| <br />
| 00 <br />
| 20-09-2014 <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_TOI_070-TAI_R2.xx_ODXXXX.fits <br />
|<br />
| <br />
| 00<br />
| 20-09-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| align="center"| HFI <br />
| HFI_TOI_AllFreqs-TAI_R2.xx_ODXXXX.fits <br />
|<br />
| <br />
| 00<br />
| 20-09-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan=8| <span style="color:Blue">HK</span> <br />
|align="center" rowspan="8"| LFI <br />
| LFI_TOI_DAE-FAST-HK_R2.XX_ODXXX.fits<br />
| <br />
| <br />
|00 <br />
|14-08-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| LFI_TOI_DAE-SlowConfiguration-HK_R2.XX_ODXXXX.fits<br />
| <br />
| <br />
|00 <br />
|14-08-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| LFI_TOI_DAE-SlowCurrent-HK_R2.XX_ODXXXX.fits<br />
| <br />
| <br />
|00 <br />
|14-08-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| LFI_TOI_DAE-SlowPhaseSwitch-HK_R2.XX_ODXXXX.fits<br />
| <br />
| <br />
|00 <br />
|14-08-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" | <br />
| <br />
|<br />
|-<br />
| LFI_TOI_DAE-SlowVoltage-HK_R2.XX_ODXXXX.fits<br />
| <br />
| <br />
|00 <br />
|14-08-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" | <br />
| <br />
|<br />
|-<br />
| LFI_TOI_REBA-HK_R2.XX_ODXXXX.fits<br />
| <br />
| <br />
|00 <br />
|14-08-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" | <br />
| <br />
|<br />
|-<br />
| SCS_TOI_EssentialASW(R)-HK_R2.XX_ODXXXX.fits<br />
| <br />
| <br />
|00 <br />
|14-08-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" | <br />
| <br />
| <br />
|-<br />
| SCS_TOI_NonEssentialASW(R)-HK_R2.XX_ODXXXX.fits<br />
| <br />
| <br />
|00 <br />
|14-08-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" | <br />
| <br />
| <br />
|-<br />
|}<br />
<br />
===Maps===<br />
====Sky Maps====<br />
=====All detectors=====<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=1050px<br />
|+ '''All Detectors'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" rowspan="56" | Survey maps<br />
| rowspan="32" align="center"| LFI<br />
| LFI_SkyMap_030_1024_R2.xx_survey-1.fits<br />
| <br />
| <br />
| 01<br />
| 26/01/2015<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_030_1024_R2.xx_survey-2.fits<br />
| <br />
| <br />
| 01<br />
| <br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_030_1024_R2.xx_survey-3.fits<br />
| <br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_030_1024_R2.xx_survey-4.fits<br />
| <br />
| <br />
|01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_030_1024_R2.xx_survey-5.fits<br />
| <br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_030_1024_R2.xx_survey-6.fits<br />
| <br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_030_1024_R2.xx_survey-7.fits<br />
| <br />
|<br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_030_1024_R2.xx_survey-8.fits<br />
| <br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_survey-1.fits<br />
| <br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_survey-2.fits<br />
| <br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_survey-3.fits<br />
| <br />
|<br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_survey-4.fits<br />
|<br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_survey-5.fits<br />
| <br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_survey-6.fits<br />
| <br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_survey-7.fits<br />
| <br />
|<br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_survey-8.fits<br />
| <br />
|<br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_survey-1.fits<br />
|<br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_survey-2.fits<br />
| <br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_survey-3.fits<br />
| <br />
| <br />
|01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_survey-4.fits<br />
| <br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_survey-5.fits<br />
| <br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_survey-6.fits<br />
| <br />
|<br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_survey-7.fits<br />
| <br />
|<br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_survey-8.fits<br />
| <br />
|<br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_2048_R2.xx_survey-1.fits<br />
| <br />
|<br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_2048_R2.xx_survey-2.fits<br />
| <br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_2048_R2.xx_survey-3.fits<br />
| <br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_2048_R2.xx_survey-4.fits<br />
| <br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_2048_R2.xx_survey-5.fits<br />
| <br />
|<br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_2048_R2.xx_survey-6.fits<br />
|<br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_2048_R2.xx_survey-7.fits<br />
| <br />
| <br />
| 01<br />
|<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_2048_R2.xx_survey-8.fits<br />
| <br />
| <br />
| 01<br />
|<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| rowspan="24" align="center"| HFI<br />
| HFI_SkyMap_100_2048_R2.xx_survey-1.fits<br />
| <br />
|<br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_100_2048_R2.xx_survey-2.fits<br />
| <br />
|<br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_100_2048_R2.xx_survey-3.fits<br />
| <br />
|<br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_100_2048_R2.xx_survey-4.fits<br />
| <br />
| <br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_143_2048_R2.xx_survey-1.fits<br />
| <br />
| <br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_143_2048_R2.xx_survey-2.fits<br />
|<br />
| <br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_143_2048_R2.xx_survey-3.fits<br />
| <br />
| <br />
|00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_143_2048_R2.xx_survey-4.fits<br />
| <br />
|<br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_217_2048_R2.xx_survey-1.fits<br />
| <br />
| <br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_217_2048_R2.xx_survey-2.fits<br />
| <br />
| <br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_217_2048_R2.xx_survey-3.fits<br />
| <br />
|<br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_217_2048_R2.xx_survey-4.fits<br />
| <br />
|<br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_353_2048_R2.xx_survey-1.fits<br />
| <br />
| <br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_353_2048_R2.xx_survey-2.fits<br />
| <br />
|<br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_353_2048_R2.xx_survey-3.fits<br />
| <br />
| <br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_353_2048_R2.xx_survey-4.fits<br />
| <br />
| <br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_545_2048_R2.xx_survey-1.fits<br />
| <br />
| <br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_545_2048_R2.xx_survey-2.fits<br />
| <br />
|<br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_545_2048_R2.xx_survey-3.fits<br />
| <br />
| <br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_545_2048_R2.xx_survey-4.fits<br />
| <br />
| <br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_857_2048_R2.xx_survey-1.fits<br />
| <br />
| <br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_857_2048_R2.xx_survey-2.fits<br />
|<br />
| <br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_857_2048_R2.xx_survey-3.fits<br />
| <br />
| <br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_857_2048_R2.xx_survey-4.fits<br />
| <br />
| <br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="28" | <span style="color:Blue">1 year maps</span> <br />
1 year = 2 surveys<br />
<br />
y1=s1+s2<br />
<br />
y2=s3+s4<br />
<br />
y3=s5+s6<br />
<br />
y4=s7+s8<br />
| rowspan="16" align="center" | LFI<br />
| LFI_SkyMap_030_1024_R2.xx_year-1.fits<br />
| <br />
|<br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_030_1024_R2.xx_year-2.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_030_1024_R2.xx_year-3.fits<br />
| <br />
|<br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_030_1024_R2.xx_year-4.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_year-1.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_year-2.fits<br />
| <br />
| <br />
|00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_year-3.fits<br />
| <br />
|<br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_year-4.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_year-1.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_year-2.fits<br />
| <br />
|<br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_year-3.fits<br />
| <br />
|<br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_year-4.fits<br />
| <br />
| <br />
|00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_2048_R2.xx_year-1.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_2048_R2.xx_year-2.fits<br />
| <br />
|<br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_2048_R2.xx_year-3.fits<br />
| <br />
|<br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_2048_R2.xx_year-4.fits<br />
| <br />
| <br />
|00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| rowspan="12" align="center" | HFI<br />
| HFI_SkyMap_100_2048_R2.xx_year-1.fits<br />
| <br />
| <br />
| 00 <br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_100_2048_R2.xx_year-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_143_2048_R2.xx_year-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_143_2048_R2.xx_year-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_217_2048_R2.xx_year-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_217_2048_R2.xx_year-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_353_2048_R2.xx_year-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_353_2048_R2.xx_year-2.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_545_2048_R2.xx_year-1.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_545_2048_R2.xx_year-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_857_2048_R2.xx_year-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_857_2048_R2.xx_year-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="12" | <span style="color:Blue">Half mission maps</span><br />
| rowspan="12" align="center"| HFI<br />
| HFI_SkyMap_100_2048_R2.xx_halfmission-1.fits<br />
| <br />
| <br />
| 00 <br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_100_2048_R2.xx_halfmission-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_143_2048_R2.xx_halfmission-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_143_2048_R2.xx_halfmission-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_217_2048_R2.xx_halfmission-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_217_2048_R2.xx_halfmission-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_353_2048_R2.xx_halfmission-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_353_2048_R2.xx_halfmission-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_545_2048_R2.xx_halfmission-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_545_2048_R2.xx_halfmission-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_857_2048_R2.xx_halfmission-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_857_2048_R2.xx_halfmission-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="12" | <span style="color:Blue">Multi year maps</span><br />
| rowspan="12" align="center"| LFI<br />
| LFI_SkyMap_030_1024_R2.xx_year-1-2.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_030_1024_R2.xx_year-1-3.fits<br />
| <br />
| <br />
| 00<br />
| 21/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_030_1024_R2.xx_year-2-4.fits<br />
| <br />
| <br />
| 00<br />
| 21/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_030_1024_R2.xx_year-3-4.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_year-1-2.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_year-1-3.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_year-2-4.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_year-3-4.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_year-1-2.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_year-1-3.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_year-2-4.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_year-3-4.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="20" | Half-ring maps <br />
| rowspan="8" align="center" | LFI <br />
| LFI_SkyMap_030_1024_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
|00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_030_1024_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| rowspan="12" align="center" | HFI <br />
| HFI_SkyMap_100_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_100_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_143_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_143_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_217_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_217_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_353_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_353_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_545_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_545_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_857_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_857_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="10" | Frequency Maps <br />
| rowspan="4" align="center" | LFI <br />
| LFI_SkyMap_030_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| rowspan="6" align="center" | HFI <br />
| HFI_SkyMap_100_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_143_2048_R2.xx_full.fits<br />
| <br />
|<br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_217_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_353_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_545_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_857_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" | Zodi correction maps <br />
| align="center" | HFI <br />
| HFI_CorrMap_<Freq>-Zodi_2048_R2.xx_<Coverage>.fits<br />
| <br />
| <br />
| 00<br />
| 16/12/2014<br />
| style="background-color: green;" |<br />
|style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
|}<br />
<br />
=====Detector maps=====<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=950px<br />
|+ '''HFI detector maps/LFI radiometer maps'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" rowspan="40" | <span style="color:Blue">Full mission</span><br />
| rowspan="22" align="center" | LFI<br />
| LFI_SkyMap_030-27M_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_030-27S_1024_R2.xx_full.fits<br />
| <br />
| <br />
|00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_030-28M_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_030-28S_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_044-24M_1024_R2.xx_full.fits<br />
| <br />
|<br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_044-24S_1024_R2.xx_full.fits<br />
| <br />
|<br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_044-25M_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_044-25S_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_044-26M_1024_R2.xx_full.fits<br />
| <br />
|<br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_044-26S_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_070-18M_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_070-18S_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_070-19M_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_070-19S_1024_R2.xx_full.fits<br />
|<br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_070-20M_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_070-20S_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_070-21M_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_070-21S_1024_R2.xx_full.fits<br />
| <br />
| <br />
|00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_070-22M_1024_R2.xx_full.fits<br />
| <br />
|<br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_070-22S_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_070-23M_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_070-23S_1024_R2.xx_full.fits<br />
| <br />
| <br />
|00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| rowspan="18" align="center" | HFI<br />
| HFI_SkyMap_143-5_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_143-6_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_143-7_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_217-1_2048_R2.xx_full.fits<br />
| <br />
|<br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_217-2_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_217-3_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
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| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
|style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_217-4_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
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| [[#note8|[8]]][[#note9|[9]]]<br />
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| HFI_SkyMap_217-4_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
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|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
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| [[#note8|[8]]][[#note9|[9]]]<br />
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| HFI_SkyMap_353-1_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_353-1_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
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| HFI_SkyMap_353-2_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
|00<br />
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| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
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| [[#note8|[8]]][[#note9|[9]]]<br />
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| HFI_SkyMap_353-2_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
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| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_353-7_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
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|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
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| [[#note8|[8]]][[#note9|[9]]]<br />
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| HFI_SkyMap_353-7_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
|<br />
| 00<br />
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| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_353-8_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
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| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_353-8_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
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| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
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| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_545-1_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
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| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
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| HFI_SkyMap_545-1_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
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|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
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| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_545-2_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
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| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
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| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_545-2_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
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| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
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| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_545-4_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
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| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_545-4_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_857-1_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
|00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_857-1_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_857-2_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_857-2_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_857-3_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
|00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_857-3_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_857-4_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_857-4_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|}<br />
<br />
=====Detector set maps=====<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=1050px<br />
|+ '''Detector set maps'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" rowspan="16" | <span style="color:Blue">Full mission</span><br />
| rowspan="8" align="center" | LFI<br />
| LFI_SkyMap_044-24_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| [[#note12|[12]]]<br />
|-<br />
| LFI_SkyMap_044-25-26_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| [[#note12|[12]]]<br />
|-<br />
| LFI_SkyMap_070-18-23_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note12|[12]]]<br />
|-<br />
| LFI_SkyMap_070-19-22_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note12|[12]]]<br />
|-<br />
| LFI_SkyMap_070-20-21_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note12|[12]]]<br />
|-<br />
| LFI_SkyMap_070-18-23_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note12|[12]]]<br />
|-<br />
| LFI_SkyMap_070-19-22_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note12|[12]]]<br />
|-<br />
| LFI_SkyMap_070-20-21_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note12|[12]]]<br />
|-<br />
| rowspan="8" align="center" | HFI<br />
| HFI_SkyMap_100-ds1_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_100-ds2_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_143-ds1_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_143-ds2_2048_R2.xx_full.fits<br />
| <br />
| <br />
|00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_217-ds1_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_217-ds2_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_353-ds1_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_353-ds2_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="26" | <span style="color:Blue">Half rings</span><br />
| rowspan="10" align="center" | LFI<br />
| LFI_SkyMap_044-24_1024_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044-24_1024_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044-25-26_1024_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044-25-26_1024_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070-18-23_1024_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
|00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070-18-23_1024_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070-19-22_1024_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070-19-22_1024_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070-20-21_1024_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070-20-21_1024_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| rowspan="16" align="center" | HFI<br />
| HFI_SkyMap_100-ds1_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
|<br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_100-ds1_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_100-ds2_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_100-ds2_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_143-ds1_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_143-ds1_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
|style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_143-ds2_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_143-ds2_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_217-ds1_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
|00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
|| HFI_SkyMap_217-ds1_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
|00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_217-ds2_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_217-ds2_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_353-ds1_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_353-ds1_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_353-ds2_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_353-ds2_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|}<br />
<br />
=====Low resolution maps=====<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=950px<br />
|+ '''Low resolution maps (with noise cov. mat.)'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" rowspan="2"|Low resolution maps (with noise cov. mat.)<br />
| align="center" | LFI<br />
| LFI_SkyMap_fff_0016_R2.xx_full.fits<br />
| <br />
| <br />
|00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| align="center" | HFI <br />
| HFI_SkyMap_fff_0016_R2.xx_full.fits<br />
| Not for PR2<br />
| <br />
| 01<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|}<br />
<br />
=====Correction maps=====<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=1300px<br />
|+ '''Correction maps'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" rowspan="1"| <span style="color:Red">A correction maps</span><br />
| rowspan="10" align="center" | LFI<br />
| <strike>LFI_CorrMap_030-ACorr_NSNS_R2.xx_full.fits</strike><br />
| <br />
| <br />
| <br />
| <br />
|<br />
| <br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="9"| <span style="color:Blue">Band pass correction<br>maps</span><br />
| LFI_CorrMap_030-BPassCorr_0256_R2.xx_full.fits<br />
| <br />
| <br />
|00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_CorrMap_044-BPassCorr_0256_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
| LFI_CorrMap_070-BPassCorr_0256_R2.xx_full.fits<br />
| <br />
| <br />
|00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_CorrMap_030-BPassCorr_0128_R2.xx_full.fits<br />
| <br />
| <br />
|00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_CorrMap_044-BPassCorr_0128_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
| LFI_CorrMap_070-BPassCorr_0128_R2.xx_full.fits<br />
| <br />
| <br />
|00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_CorrMap_030-BPassCorr_0064_R2.xx_full.fits<br />
| <br />
| <br />
|00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_CorrMap_044-BPassCorr_0064_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
| LFI_CorrMap_070-BPassCorr_0064_R2.xx_full.fits<br />
| <br />
| <br />
|00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="12"| <span style="color:Blue">Dust correction<br>maps</span><br />
| rowspan="12" align="center" |HFI <br />
| HFI_CorrMap 353 GHz leakage global fits maps<br />
| <br />
| <br />
| 00<br />
| 09/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| <strike>HFI_CorrMap_100-dustleak-ground_2048_R2.xx_full.fits</strike><br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
|<br />
|-<br />
| <strike>HFI_CorrMap_353-dustleak-diff_2048_R2.xx_full.fits</strike><br />
| <br />
| <br />
| <br />
| <br />
|<br />
| <br />
| <br />
| <br />
|-<br />
| HFI_CorrMap_353-dustleak-ground_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
|24/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| <strike>HFI_CorrMap_353_dustleak-diff_2048_R2.xx_year-1.fits</strike><br />
| <br />
| <br />
| <br />
|<br />
| <br />
| <br />
| <br />
| <br />
|-<br />
| <strike>HFI_CorrMap_353_dustleak-diff_2048_R2.xx_year-2.fits</strike><br />
| <br />
| <br />
| <br />
| <br />
|<br />
| <br />
| <br />
| <br />
|-<br />
| HFI_CorrMap_353_dustleak-ground_2048_R2.xx_year-1.fits<br />
| <br />
| <br />
| 00<br />
| 24/11/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_CorrMap_353_dustleak-ground_2048_R2.xx_year-2.fits<br />
| <br />
| <br />
| 00<br />
| 24/11/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| <strike>HFI_CorrMap_353-ds1-dustleak-diff_2048_R2.xx_full.fits</strike><br />
| <br />
|<br />
| <br />
| <br />
| <br />
| <br />
| <br />
|<br />
|-<br />
| <strike>HFI_CorrMap_353-ds2-dustleak-diff_2048_R2.xx_full.fits</strike><br />
| <br />
| <br />
| <br />
|<br />
| <br />
| <br />
| <br />
| <br />
|-<br />
| HFI_CorrMap_353-ds1-dustleak-ground_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 24/11/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_CorrMap_353-ds2-dustleak-ground_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 24/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="1"| <span style="color:Blue">CO correction<br>maps</span><br />
| rowspan="1" align="center" | HFI <br />
| <strike>HFI_CorrMap_<freq>-coleak-'''METHOD1'''_2048_R2.xx_full.fits</strike><br />
| <br />
| <br />
| <br />
| <br />
|<br />
| <br />
| <br />
| <br />
|}<br />
<br />
====Covariance matrices====<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=850px<br />
|+ '''Covariance matrices'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" rowspan="4"| Cov. Matrices<br />
| style="text-align:center" rowspan="4"| HFI+LFI<br />
| LFI_NoiseCovMat_030_0016_R2.xx.tgz<br />
| <br />
| <br />
|00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| LFI_NoiseCovMat_044_0016_R2.xx.tgz<br />
| <br />
| <br />
| 00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_NoiseCovMat_070_0016_R2.xx.tgz<br />
| <br />
| <br />
| 00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI covariance matrices<br />
| Not for PR2<br />
| <br />
| 01<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|}<br />
<br />
====CMB maps====<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=1050px<br />
|+ '''CMB Maps'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" rowspan="6" | CMB anisotropy maps<br />
| rowspan="6" align="center" | COM<br />
| COM_CMB_IQU-nilc-field-X_Nside_R2.xx.fits<br />
| <br />
|<br />
|00 <br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_CMB_IQU-sevem-field-X_Nside_R2.xx.fits<br />
| <br />
| <br />
| 00<br />
|09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| COM_CMB_IQU-smica-field-X_Nside_R2.xx.fits<br />
| <br />
| <br />
| 00<br />
|09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_CMB_IQU-commander-field-X_Nside_R2.xx.fits<br />
| <br />
| <br />
| 00<br />
| 09/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| <strike>COM_CMB_IQU-commrul_0256_R2.xx.fits</strike><br />
| <br />
| <br />
| <br />
|<br />
| <br />
| <br />
| <br />
| <br />
|-<br />
| <span style="color:Red"><strike>Other representations</strike></span><br />
| <br />
| <br />
| <br />
|<br />
| <br />
| <br />
| <br />
| <br />
|-<br />
|}<br />
<br />
====Component maps====<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=950px<br />
|+ '''Component Maps'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" rowspan="3" | CO maps<br />
| align="center" rowspan="3"| HFI<br />
| HFI_CompMap_CO-Type1_2048_R2.xx.fits<br />
| <br />
|<br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_CompMap_CO-Type2_2048_R2.xx.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| <strike>HFI_CompMap_CO-Type3_2048_R2.xx.fits</strike><br />
| <br />
| <br />
| <br />
|<br />
| <br />
| <br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="12" | Commander foregrounds<br />
| align="center" rowspan="12"| COM<br />
| COM_CompMap_AME-commander_0256_R2.xx.fits<br />
|<br />
|<br />
| 00<br />
| 11/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| COM_CompMap_CMB-commander_0256_R2.xx.fits<br />
|<br />
|<br />
| 00<br />
| 11/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| COM_CompMap_CO21-commander_2048_R2.xx.fits<br />
|<br />
|<br />
| 00<br />
| 11/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| COM_CompMap_CO-commander_0256_R2.xx.fits<br />
|<br />
|<br />
| 00<br />
| 11/12/2014<br />
| style="background-color: green;" |<br />
|style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_CompMap_dust-commander_0256_R2.xx.fits<br />
|<br />
|<br />
| 00<br />
| 11/12/2014<br />
| style="background-color: green;" |<br />
|style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_CompMap_DustPol-commander_1024_R2.xx.fits<br />
|<br />
|<br />
| 00<br />
| 11/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_CompMap_freefree-commander_0256_R2.xx.fits<br />
|<br />
|<br />
| 00<br />
| 11/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| COM_CompMap_Synchrotron-commander_0256_R2.xx.fits<br />
|<br />
|<br />
| 00<br />
| 11/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| COM_CompMap_SynchrotronPol-commander_0256_R2.xx.fits<br />
|<br />
|<br />
| 00<br />
| 11/12/2014<br />
| style="background-color: green;" |<br />
|style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_CompMap_SZ-commander_0256_R2.xx.fits<br />
|<br />
|<br />
| 00<br />
| 11/12/2014<br />
| style="background-color: green;" |<br />
|style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_CompMap_ThermalDust-commander_2048_R2.xx.fits<br />
|<br />
|<br />
| 00<br />
| 11/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_CompMap_xline-commander_0256_R2.xx.fits<br />
|<br />
|<br />
| 00<br />
| 11/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" | Lensing maps<br />
| align="center" | COM<br />
| COM_CompMap_Lensing_2048_R2.xx.tar + SimMap tars<br />
|<br />
| <br />
|00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
|}<br />
<br />
====Masks====<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=850px<br />
|+ '''Masks'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" rowspan='4'| Masks<br />
| style="text-align:center" | <strike>LFI</strike><br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
|-<br />
| style="text-align:center" | HFI<br />
| HFI_Mask_GalPlane-apo 0 2 5 _2048_R2.xx.fits<br />
|<br />
| <br />
| 00<br />
| 19/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| style="text-align:center" rowspan='2'| COM<br />
| COM_CMB_IQU-common-field-MaskInt_2048_R2.xx.fits<br />
| <br />
|<br />
| 00<br />
| 10/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_CMB_IQU-common-field-MaskPol_1024_R2.xx.fits<br />
| <br />
| <br />
| 00<br />
| 10/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan='2'| Point source masks<br />
| style="text-align:center" rowspan='1'| LFI<br />
| LFI_Mask_PointSrc_2048_R2.xx.fits<br />
| <br />
| <br />
| 00<br />
|27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| style="text-align:center" | HFI<br />
| HFI_Mask_PointSrc_2048_R2.xx.fits<br />
| <br />
| <br />
|00<br />
| 19/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
|}<br />
<br />
===Angular power spectra===<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=1050px<br />
|+ '''Angular power spectra'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" rowspan="2" | CMB angular power spectra<br />
| style="text-align:center" rowspan="2" |COM<br />
| COM_PowerSpect_CMB_R2.xx.fits<br />
|<br />
| <br />
| 00<br />
| 05/02/2015<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| <strike>COM_PowerSpect_CMB_R2.xx.txt</strike><br />
|<br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="1"| <strike>Sky Angular power spectrum</strike><br />
| style="text-align:center" rowspan="4" |<br />
| <strike>LFI_PowerSpect_030_R2.xx.fits</strike><br />
|<br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
| [[#note37|[37]]]<br />
|-<br />
|}<br />
<div id="note37"></div>[37] For this release detector and detector set power spectra will not be provided. Instead the detector and detector set maps will be provided.<br />
<br />
===Characterisation===<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=850px<br />
|+ '''Characterization'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" rowspan="3"| RIMO<br />
| style="text-align:center" | LFI<br />
| LFI_RIMO_R2.xx.fits<br />
| <br />
| <br />
|50<br />
| 16/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| style="text-align:center" | HFI<br />
| HFI_RIMO_R2.xx.fits<br />
| <br />
| <br />
| 00<br />
| 20/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| style="text-align:center" | HFI<br />
| HFI beams RIMO(s)<br />
| <br />
| <br />
| 00<br />
| 05/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
|}<br />
<br />
===Catalogues===<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=850px<br />
|+ '''Catalogues'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" rowspan="9"| PCCS<br />
| style="text-align:center" rowspan="9"| COM<br />
| COM_PCCS_030_R2.xx.fits + excl.<br />
| <br />
| <br />
| 02<br />
|15/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_PCCS_044_R2.xx.fits + excl.<br />
| <br />
| <br />
| 02<br />
|15/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_PCCS_070_R2.xx.fits + excl.<br />
| <br />
| <br />
| 02<br />
| 15/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_PCCS_100_R2.xx.fits<br />
| <br />
| <br />
| 01<br />
| 19/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_PCCS_143_R2.xx.fits<br />
| <br />
| <br />
| 01<br />
| 19/11/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_PCCS_217_R2.xx.fits<br />
| <br />
| <br />
|01<br />
| 19/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_PCCS_353_R2.xx.fits<br />
| <br />
| <br />
| 01<br />
| 19/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_PCCS_545_R2.xx.fits<br />
| <br />
| <br />
| 01<br />
|19/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_PCCS_857_R2.xx.fits<br />
| <br />
| <br />
| 01<br />
|19/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="4"| SZ catalogues<br />
| style="text-align:center" rowspan="4"| COM<br />
| COM_PCCS_SZ-MMF1_R2.xx.fits<br />
| <br />
| <br />
| 08<br />
| 29/01/2015<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_PCCS_SZ-MMF3_R2.xx.fits<br />
| <br />
| <br />
| 08<br />
| 29/01/2015<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
|<br />
|-<br />
| COM_PCCS_SZ-PwS_R2.xx.fits<br />
| <br />
| <br />
| 08<br />
| 29/01/2015<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_PCCS_SZ-union_R2.xx.fits<br />
| <br />
| <br />
| 08<br />
| 03/02/2015<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
|<br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="4"| Other catalogues<br />
| style="text-align:center" rowspan="4"| HFI<br />
| <span style="color:Red"><strike>Dusty source catalogue</strike></span><br />
| <br />
| <br />
|<br />
| <br />
| <br />
| <br />
| <br />
| <br />
|-<br />
| <span style="color:Red"><strike>Radio sources catalogue</strike></span><br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
|-<br />
| <span style="color:Blue">HFI_PCCS_GCC_R2.xx.fits</span><br />
| <br />
| <br />
| 02<br />
| 16/01/2015<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| <span style="color:Blue">High-z catalogue</span><br />
| <br />
| <br />
| <br />
| <br />
|<br />
| <br />
| <br />
| <br />
|-<br />
|}<br />
<br />
===Other products===<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=850px<br />
|+ '''Other products'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" | Cosmological parameters<br />
| style="text-align:center" rowspan="1"| COM<br />
| Cosmological parameter tables<br />
| <br />
| <br />
| 00<br />
| 28/01/2015<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="1"| Codes<br />
| style="text-align:center" rowspan="1"| COM<br />
| Likelihood code<br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
|<br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="11"| Beams<br />
| style="text-align:center" rowspan="5"| <br />
| LFI scanning beams<br />
| <br />
| <br />
| 00<br />
| 21-11-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
| HFI scanning beams<br />
| <br />
| <br />
| 00<br />
| 05/02/2015<br />
| style="background-color: green;" |<br />
| <br />
|<br />
| <br />
|-<br />
| Effective beams 30GHz<br />
| <br />
| <br />
| <br />
| 22-09-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
| Effective beams 44GHz<br />
| <br />
| <br />
| <br />
| 24-09-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
| Effective beams 70GHz<br />
| <br />
| <br />
| <br />
| 24-09-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
| style="text-align:center" rowspan="6"| <br />
| Effective beams 100 GHz<br />
| <br />
| <br />
| <br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
| Effective beams 143 GHz<br />
| <br />
| <br />
| <br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
| Effective beams 217 GHz<br />
| <br />
| <br />
| <br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
| Effective beams 353 GHz<br />
| <br />
| <br />
| <br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
| Effective beams 545 GHz<br />
| <br />
| <br />
| <br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
| Effective beams 857 GGz<br />
| <br />
| <br />
| <br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="2"| 4D maps<br />
| style="text-align:center" rowspan="2"| LFI<br />
| Code<br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
|<br />
| [[#noteA|[A]]]<br />
|-<br />
| map4D_calib_DDX11_LFIXX_gal_nsideXXX_npsiXXXX.fits<br />
| <br />
| <br />
| <br />
| 19/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| [[#noteA|[A]]]<br />
|-<br />
!bgcolor="ffdead" scope="row" | Datesobs<br />
| USPDC<br />
| HFI_DatesObs_<Freq>_2048_R2.xx_surveyX.fits.gz<br />
| <br />
| <br />
| 01<br />
|29/01/2015<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" | YSZ package<br />
| COM<br />
| COM_CompMap_YSZ_R2.nn.fits.tgz<br />
| <br />
| 12 Gb<br />
|00<br />
| 05/02/2015<br />
| <br />
| <br />
| <br />
| <br />
|-<br />
|}<br />
<div id="noteA"></div>[A] '''This is not an official product.'''</div>
Xdupac
https://wiki.cosmos.esa.int/planckpla2015/index.php?title=Product_Table_for_PLAv2&diff=11408
Product Table for PLAv2
2015-02-05T10:14:28Z
<p>Xdupac: /* Other products */</p>
<hr />
<div>{{DISPLAYTITLE:Products table for PLAv2}}<br />
==Product categories==<br />
*New products for this release that I believe have been confirmed appear in <span style="color:Blue">blue font</span>, products that are still TBC in <span style="color:Red">red font</span> (if it is one entire category of products I will just use color in the products category name, e.g. <span style="color:Blue">1 year maps</span>). Please check this in the tables and let me know whether there are any errors.<br />
*The Obs column contains links to notes at the end of each table. Please check the notes and let me know your feedback.<br />
*More general comments appear at the end of the numbered notes.<br />
<br />
I suggest you use the [[Talk:Product_Table_for_PLAv2|discussion page associated with this page]] to provide your feedback or make any comments relate to the list of products. The discussion page has the same structures in terms of sections as this page. Please try to write your comments/feedback in the appropriate section. I would also ask you to put your initials in the comments you write so that I can more easily get back to you to try to clarify any questions. Yes, it is true I can find out who wrote what in the history page but it makes my life easier if you associate your name to the comments you provide.<br />
<br />
The '''Description''' column will be used to add a one line description of the product that will appear in the archive as a tooltip associated with the product to allow a quick identification by users.<br />
===Time Series===<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=1050px<br />
|+ '''FITS filenames'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" rowspan="9" | <span style="color:Blue">Detector timeseries</span><br />
|rowspan="3" align="center" | LFI <br />
| LFI_TOI_030-SCI_R2.xx_ODXXXX.fits<br />
| <br />
| <br />
|00 <br />
| 10-09-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| LFI_TOI_044-SCI_R2.xx_ODXXXX.fits<br />
| <br />
| <br />
| 00<br />
| 10-09-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| LFI_TOI_070-SCI_R2.xx_ODXXXX.fits<br />
| <br />
| <br />
| 00<br />
| 10-09-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
|rowspan="6" align="center" | HFI <br />
| HFI_TOI_100-SCI_R2.xx_ODXXXX.fits<br />
| Only PSB: not for Feb. 2015 release<br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
|<br />
|-<br />
| HFI_TOI_143-SCI_R2.xx_ODXXXX.fits<br />
| without PSBs<br />
| <br />
| 00<br />
| 20/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_TOI_217-SCI_R2.xx_ODXXXX.fits<br />
| without PSBs<br />
| <br />
| 00<br />
| 20/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_TOI_353-SCI_R2.xx_ODXXXX.fits<br />
| with PSBs<br />
| <br />
| 00<br />
| 19/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_TOI_545-SCI_R2.xx_ODXXXX.fits<br />
| <br />
| <br />
| 00<br />
| 23/01/2015<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_TOI_857-SCI_R2.xx_ODXXXX.fits<br />
| <br />
| <br />
| 00<br />
| 23/01/2015<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="7" | <span style="color:Blue">Offsets</span><br />
| rowspan="6" align="center"| LFI <br />
| LFI_TOI_030-OFF_R2.xx_ODXXXX-full.fits<br />
| <br />
| <br />
| 00<br />
| 19-09-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_TOI_044-OFF_R2.xx_ODXXXX-full.fits<br />
| <br />
| <br />
| 00<br />
| 19-09-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_TOI_070-OFF_R2.xx_ODXXXX-full.fits<br />
| <br />
| <br />
|00<br />
| 19-09-2014 <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_TOI_030-OFF_R2.xx_ODXXXX-full-ringhalf.fits<br />
| <br />
| <br />
| 00<br />
| 11-11-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_TOI_044-OFF_R2.xx_ODXXXX-full-ringhalf.fits<br />
| <br />
| <br />
| 00<br />
| 11-11-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_TOI_070-OFF_R2.xx_ODXXXX-full-ringhalf.fits<br />
| <br />
| <br />
| 00<br />
| 11-11-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
|align="center"| HFI <br />
| HFI_TOI_AllFreqs-OFF_R2.xx.fits<br />
|<br />
|<br />
|00<br />
|13/01/2015<br />
|style="background-color: green;" |<br />
|style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan=9| <span style="color:Blue">Pointing</span><br />
| align="center" rowspan="3"| LFI <br />
| LFI_TOI_030-PTG_R2.xx_ODXXXX.fits <br />
|<br />
| <br />
|00 <br />
|18-07-2014 <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_TOI_044-PTG_R2.xx_ODXXXX.fits <br />
|<br />
| <br />
| 00 <br />
| 18-07-2014 <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_TOI_070-PTG_R2.xx_ODXXXX.fits <br />
|<br />
| <br />
| 00 <br />
| 18-07-2014 <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| rowspan=6 align="center"| HFI <br />
| HFI_TOI_100-PTG_R2.xx_ODXXXX.fits <br />
|<br />
| <br />
| 01 <br />
| 26-08-2014 <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_TOI_143-PTG_R2.xx_ODXXXX.fits <br />
|<br />
| <br />
| 01 <br />
| 26-08-2014 <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_TOI_217-PTG_R2.xx_ODXXXX.fits <br />
|<br />
| <br />
| 01 <br />
| 26-08-2014 <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_TOI_353-PTG_R2.xx_ODXXXX.fits <br />
|<br />
| <br />
| 01 <br />
| 26-08-2014 <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_TOI_545-PTG_R2.xx_ODXXXX.fits <br />
|<br />
| <br />
| 01 <br />
| 26-08-2014 <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_TOI_857-PTG_R2.xx_ODXXXX.fits <br />
|<br />
| <br />
| 01 <br />
| 26-08-2014 <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="4"| <span style="color:Blue">Time stamps</span><br />
| align="center" rowspan="3"| LFI <br />
| LFI_TOI_030-TAI_R2.xx_ODXXXX.fits <br />
|<br />
| <br />
|00 <br />
| 20-09-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_TOI_044-TAI_R2.xx_ODXXXX.fits <br />
|<br />
| <br />
| 00 <br />
| 20-09-2014 <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_TOI_070-TAI_R2.xx_ODXXXX.fits <br />
|<br />
| <br />
| 00<br />
| 20-09-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| align="center"| HFI <br />
| HFI_TOI_AllFreqs-TAI_R2.xx_ODXXXX.fits <br />
|<br />
| <br />
| 00<br />
| 20-09-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan=8| <span style="color:Blue">HK</span> <br />
|align="center" rowspan="8"| LFI <br />
| LFI_TOI_DAE-FAST-HK_R2.XX_ODXXX.fits<br />
| <br />
| <br />
|00 <br />
|14-08-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| LFI_TOI_DAE-SlowConfiguration-HK_R2.XX_ODXXXX.fits<br />
| <br />
| <br />
|00 <br />
|14-08-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| LFI_TOI_DAE-SlowCurrent-HK_R2.XX_ODXXXX.fits<br />
| <br />
| <br />
|00 <br />
|14-08-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| LFI_TOI_DAE-SlowPhaseSwitch-HK_R2.XX_ODXXXX.fits<br />
| <br />
| <br />
|00 <br />
|14-08-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" | <br />
| <br />
|<br />
|-<br />
| LFI_TOI_DAE-SlowVoltage-HK_R2.XX_ODXXXX.fits<br />
| <br />
| <br />
|00 <br />
|14-08-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" | <br />
| <br />
|<br />
|-<br />
| LFI_TOI_REBA-HK_R2.XX_ODXXXX.fits<br />
| <br />
| <br />
|00 <br />
|14-08-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" | <br />
| <br />
|<br />
|-<br />
| SCS_TOI_EssentialASW(R)-HK_R2.XX_ODXXXX.fits<br />
| <br />
| <br />
|00 <br />
|14-08-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" | <br />
| <br />
| <br />
|-<br />
| SCS_TOI_NonEssentialASW(R)-HK_R2.XX_ODXXXX.fits<br />
| <br />
| <br />
|00 <br />
|14-08-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" | <br />
| <br />
| <br />
|-<br />
|}<br />
<br />
===Maps===<br />
====Sky Maps====<br />
=====All detectors=====<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=1050px<br />
|+ '''All Detectors'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" rowspan="56" | Survey maps<br />
| rowspan="32" align="center"| LFI<br />
| LFI_SkyMap_030_1024_R2.xx_survey-1.fits<br />
| <br />
| <br />
| 01<br />
| 26/01/2015<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_030_1024_R2.xx_survey-2.fits<br />
| <br />
| <br />
| 01<br />
| <br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_030_1024_R2.xx_survey-3.fits<br />
| <br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_030_1024_R2.xx_survey-4.fits<br />
| <br />
| <br />
|01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_030_1024_R2.xx_survey-5.fits<br />
| <br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_030_1024_R2.xx_survey-6.fits<br />
| <br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_030_1024_R2.xx_survey-7.fits<br />
| <br />
|<br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_030_1024_R2.xx_survey-8.fits<br />
| <br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_survey-1.fits<br />
| <br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_survey-2.fits<br />
| <br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_survey-3.fits<br />
| <br />
|<br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_survey-4.fits<br />
|<br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_survey-5.fits<br />
| <br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_survey-6.fits<br />
| <br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_survey-7.fits<br />
| <br />
|<br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_survey-8.fits<br />
| <br />
|<br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_survey-1.fits<br />
|<br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_survey-2.fits<br />
| <br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_survey-3.fits<br />
| <br />
| <br />
|01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_survey-4.fits<br />
| <br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_survey-5.fits<br />
| <br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_survey-6.fits<br />
| <br />
|<br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_survey-7.fits<br />
| <br />
|<br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_survey-8.fits<br />
| <br />
|<br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_2048_R2.xx_survey-1.fits<br />
| <br />
|<br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_2048_R2.xx_survey-2.fits<br />
| <br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_2048_R2.xx_survey-3.fits<br />
| <br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_2048_R2.xx_survey-4.fits<br />
| <br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_2048_R2.xx_survey-5.fits<br />
| <br />
|<br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_2048_R2.xx_survey-6.fits<br />
|<br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_2048_R2.xx_survey-7.fits<br />
| <br />
| <br />
| 01<br />
|<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_2048_R2.xx_survey-8.fits<br />
| <br />
| <br />
| 01<br />
|<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| rowspan="24" align="center"| HFI<br />
| HFI_SkyMap_100_2048_R2.xx_survey-1.fits<br />
| <br />
|<br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_100_2048_R2.xx_survey-2.fits<br />
| <br />
|<br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_100_2048_R2.xx_survey-3.fits<br />
| <br />
|<br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_100_2048_R2.xx_survey-4.fits<br />
| <br />
| <br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_143_2048_R2.xx_survey-1.fits<br />
| <br />
| <br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_143_2048_R2.xx_survey-2.fits<br />
|<br />
| <br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_143_2048_R2.xx_survey-3.fits<br />
| <br />
| <br />
|00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_143_2048_R2.xx_survey-4.fits<br />
| <br />
|<br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_217_2048_R2.xx_survey-1.fits<br />
| <br />
| <br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_217_2048_R2.xx_survey-2.fits<br />
| <br />
| <br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_217_2048_R2.xx_survey-3.fits<br />
| <br />
|<br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_217_2048_R2.xx_survey-4.fits<br />
| <br />
|<br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_353_2048_R2.xx_survey-1.fits<br />
| <br />
| <br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_353_2048_R2.xx_survey-2.fits<br />
| <br />
|<br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_353_2048_R2.xx_survey-3.fits<br />
| <br />
| <br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_353_2048_R2.xx_survey-4.fits<br />
| <br />
| <br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_545_2048_R2.xx_survey-1.fits<br />
| <br />
| <br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_545_2048_R2.xx_survey-2.fits<br />
| <br />
|<br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_545_2048_R2.xx_survey-3.fits<br />
| <br />
| <br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_545_2048_R2.xx_survey-4.fits<br />
| <br />
| <br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_857_2048_R2.xx_survey-1.fits<br />
| <br />
| <br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_857_2048_R2.xx_survey-2.fits<br />
|<br />
| <br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_857_2048_R2.xx_survey-3.fits<br />
| <br />
| <br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_857_2048_R2.xx_survey-4.fits<br />
| <br />
| <br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="28" | <span style="color:Blue">1 year maps</span> <br />
1 year = 2 surveys<br />
<br />
y1=s1+s2<br />
<br />
y2=s3+s4<br />
<br />
y3=s5+s6<br />
<br />
y4=s7+s8<br />
| rowspan="16" align="center" | LFI<br />
| LFI_SkyMap_030_1024_R2.xx_year-1.fits<br />
| <br />
|<br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_030_1024_R2.xx_year-2.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_030_1024_R2.xx_year-3.fits<br />
| <br />
|<br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_030_1024_R2.xx_year-4.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_year-1.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_year-2.fits<br />
| <br />
| <br />
|00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_year-3.fits<br />
| <br />
|<br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_year-4.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_year-1.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_year-2.fits<br />
| <br />
|<br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_year-3.fits<br />
| <br />
|<br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_year-4.fits<br />
| <br />
| <br />
|00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_2048_R2.xx_year-1.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_2048_R2.xx_year-2.fits<br />
| <br />
|<br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_2048_R2.xx_year-3.fits<br />
| <br />
|<br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_2048_R2.xx_year-4.fits<br />
| <br />
| <br />
|00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| rowspan="12" align="center" | HFI<br />
| HFI_SkyMap_100_2048_R2.xx_year-1.fits<br />
| <br />
| <br />
| 00 <br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_100_2048_R2.xx_year-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_143_2048_R2.xx_year-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_143_2048_R2.xx_year-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_217_2048_R2.xx_year-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_217_2048_R2.xx_year-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_353_2048_R2.xx_year-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_353_2048_R2.xx_year-2.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_545_2048_R2.xx_year-1.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_545_2048_R2.xx_year-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_857_2048_R2.xx_year-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_857_2048_R2.xx_year-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="12" | <span style="color:Blue">Half mission maps</span><br />
| rowspan="12" align="center"| HFI<br />
| HFI_SkyMap_100_2048_R2.xx_halfmission-1.fits<br />
| <br />
| <br />
| 00 <br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_100_2048_R2.xx_halfmission-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_143_2048_R2.xx_halfmission-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_143_2048_R2.xx_halfmission-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_217_2048_R2.xx_halfmission-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_217_2048_R2.xx_halfmission-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_353_2048_R2.xx_halfmission-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_353_2048_R2.xx_halfmission-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_545_2048_R2.xx_halfmission-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_545_2048_R2.xx_halfmission-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_857_2048_R2.xx_halfmission-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_857_2048_R2.xx_halfmission-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="12" | <span style="color:Blue">Multi year maps</span><br />
| rowspan="12" align="center"| LFI<br />
| LFI_SkyMap_030_1024_R2.xx_year-1-2.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_030_1024_R2.xx_year-1-3.fits<br />
| <br />
| <br />
| 00<br />
| 21/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_030_1024_R2.xx_year-2-4.fits<br />
| <br />
| <br />
| 00<br />
| 21/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_030_1024_R2.xx_year-3-4.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_year-1-2.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_year-1-3.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_year-2-4.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_year-3-4.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_year-1-2.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_year-1-3.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_year-2-4.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_year-3-4.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="20" | Half-ring maps <br />
| rowspan="8" align="center" | LFI <br />
| LFI_SkyMap_030_1024_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
|00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_030_1024_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| rowspan="12" align="center" | HFI <br />
| HFI_SkyMap_100_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_100_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_143_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_143_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_217_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_217_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_353_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_353_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_545_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_545_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_857_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_857_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="10" | Frequency Maps <br />
| rowspan="4" align="center" | LFI <br />
| LFI_SkyMap_030_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| rowspan="6" align="center" | HFI <br />
| HFI_SkyMap_100_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_143_2048_R2.xx_full.fits<br />
| <br />
|<br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_217_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_353_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_545_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_857_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" | Zodi correction maps <br />
| align="center" | HFI <br />
| HFI_CorrMap_<Freq>-Zodi_2048_R2.xx_<Coverage>.fits<br />
| <br />
| <br />
| 00<br />
| 16/12/2014<br />
| style="background-color: green;" |<br />
|style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
|}<br />
<br />
=====Detector maps=====<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=950px<br />
|+ '''HFI detector maps/LFI radiometer maps'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" rowspan="40" | <span style="color:Blue">Full mission</span><br />
| rowspan="22" align="center" | LFI<br />
| LFI_SkyMap_030-27M_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_030-27S_1024_R2.xx_full.fits<br />
| <br />
| <br />
|00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_030-28M_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_030-28S_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_044-24M_1024_R2.xx_full.fits<br />
| <br />
|<br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_044-24S_1024_R2.xx_full.fits<br />
| <br />
|<br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_044-25M_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_044-25S_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_044-26M_1024_R2.xx_full.fits<br />
| <br />
|<br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_044-26S_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_070-18M_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_070-18S_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_070-19M_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_070-19S_1024_R2.xx_full.fits<br />
|<br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_070-20M_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_070-20S_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_070-21M_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_070-21S_1024_R2.xx_full.fits<br />
| <br />
| <br />
|00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_070-22M_1024_R2.xx_full.fits<br />
| <br />
|<br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_070-22S_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_070-23M_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_070-23S_1024_R2.xx_full.fits<br />
| <br />
| <br />
|00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| rowspan="18" align="center" | HFI<br />
| HFI_SkyMap_143-5_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_143-6_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_143-7_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_217-1_2048_R2.xx_full.fits<br />
| <br />
|<br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_217-2_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_217-3_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_217-4_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_353-1_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_353-2_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_353-7_2048_R2.xx_full.fits<br />
| <br />
| <br />
|00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_353-8_2048_R2.xx_full.fits<br />
| <br />
|<br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_545-1_2048_R2.xx_full.fits<br />
| <br />
| <br />
|00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_545-2_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_545-4_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_857-1_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_857-2_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_857-3_2048_R2.xx_full.fits<br />
| <br />
|<br />
|00 <br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_857-4_2048_R2.xx_full.fits<br />
| <br />
| <br />
|00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="80" | <span style="color:Blue">Half rings</span><br />
| rowspan="44" align="center" | LFI<br />
| LFI_SkyMap_030-27M_1024_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_030-27M_1024_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_030-27S_1024_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
|00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_030-27S_1024_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
|00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_030-28M_1024_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_030-28M_1024_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_030-28S_1024_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_030-28S_1024_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_044-24M_1024_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
|style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_044-24M_1024_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_044-24S_1024_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_044-24S_1024_R2.xx_full-ringhalf-2.fits<br />
| <br />
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| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_857-4_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_857-4_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|}<br />
<br />
=====Detector set maps=====<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=1050px<br />
|+ '''Detector set maps'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" rowspan="16" | <span style="color:Blue">Full mission</span><br />
| rowspan="8" align="center" | LFI<br />
| LFI_SkyMap_044-24_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| [[#note12|[12]]]<br />
|-<br />
| LFI_SkyMap_044-25-26_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| [[#note12|[12]]]<br />
|-<br />
| LFI_SkyMap_070-18-23_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note12|[12]]]<br />
|-<br />
| LFI_SkyMap_070-19-22_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note12|[12]]]<br />
|-<br />
| LFI_SkyMap_070-20-21_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note12|[12]]]<br />
|-<br />
| LFI_SkyMap_070-18-23_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note12|[12]]]<br />
|-<br />
| LFI_SkyMap_070-19-22_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note12|[12]]]<br />
|-<br />
| LFI_SkyMap_070-20-21_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note12|[12]]]<br />
|-<br />
| rowspan="8" align="center" | HFI<br />
| HFI_SkyMap_100-ds1_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_100-ds2_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_143-ds1_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_143-ds2_2048_R2.xx_full.fits<br />
| <br />
| <br />
|00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_217-ds1_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_217-ds2_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_353-ds1_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_353-ds2_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="26" | <span style="color:Blue">Half rings</span><br />
| rowspan="10" align="center" | LFI<br />
| LFI_SkyMap_044-24_1024_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044-24_1024_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044-25-26_1024_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044-25-26_1024_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070-18-23_1024_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
|00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070-18-23_1024_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070-19-22_1024_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070-19-22_1024_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070-20-21_1024_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070-20-21_1024_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| rowspan="16" align="center" | HFI<br />
| HFI_SkyMap_100-ds1_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
|<br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_100-ds1_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_100-ds2_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_100-ds2_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_143-ds1_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_143-ds1_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
|style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_143-ds2_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_143-ds2_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_217-ds1_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
|00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
|| HFI_SkyMap_217-ds1_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
|00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_217-ds2_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_217-ds2_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_353-ds1_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_353-ds1_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_353-ds2_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_353-ds2_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|}<br />
<br />
=====Low resolution maps=====<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=950px<br />
|+ '''Low resolution maps (with noise cov. mat.)'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" rowspan="2"|Low resolution maps (with noise cov. mat.)<br />
| align="center" | LFI<br />
| LFI_SkyMap_fff_0016_R2.xx_full.fits<br />
| <br />
| <br />
|00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| align="center" | HFI <br />
| HFI_SkyMap_fff_0016_R2.xx_full.fits<br />
| Not for PR2<br />
| <br />
| 01<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|}<br />
<br />
=====Correction maps=====<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=1300px<br />
|+ '''Correction maps'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" rowspan="1"| <span style="color:Red">A correction maps</span><br />
| rowspan="10" align="center" | LFI<br />
| <strike>LFI_CorrMap_030-ACorr_NSNS_R2.xx_full.fits</strike><br />
| <br />
| <br />
| <br />
| <br />
|<br />
| <br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="9"| <span style="color:Blue">Band pass correction<br>maps</span><br />
| LFI_CorrMap_030-BPassCorr_0256_R2.xx_full.fits<br />
| <br />
| <br />
|00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_CorrMap_044-BPassCorr_0256_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
| LFI_CorrMap_070-BPassCorr_0256_R2.xx_full.fits<br />
| <br />
| <br />
|00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_CorrMap_030-BPassCorr_0128_R2.xx_full.fits<br />
| <br />
| <br />
|00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_CorrMap_044-BPassCorr_0128_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
| LFI_CorrMap_070-BPassCorr_0128_R2.xx_full.fits<br />
| <br />
| <br />
|00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_CorrMap_030-BPassCorr_0064_R2.xx_full.fits<br />
| <br />
| <br />
|00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_CorrMap_044-BPassCorr_0064_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
| LFI_CorrMap_070-BPassCorr_0064_R2.xx_full.fits<br />
| <br />
| <br />
|00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="12"| <span style="color:Blue">Dust correction<br>maps</span><br />
| rowspan="12" align="center" |HFI <br />
| HFI_CorrMap 353 GHz leakage global fits maps<br />
| <br />
| <br />
| 00<br />
| 09/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| <strike>HFI_CorrMap_100-dustleak-ground_2048_R2.xx_full.fits</strike><br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
|<br />
|-<br />
| <strike>HFI_CorrMap_353-dustleak-diff_2048_R2.xx_full.fits</strike><br />
| <br />
| <br />
| <br />
| <br />
|<br />
| <br />
| <br />
| <br />
|-<br />
| HFI_CorrMap_353-dustleak-ground_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
|24/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| <strike>HFI_CorrMap_353_dustleak-diff_2048_R2.xx_year-1.fits</strike><br />
| <br />
| <br />
| <br />
|<br />
| <br />
| <br />
| <br />
| <br />
|-<br />
| <strike>HFI_CorrMap_353_dustleak-diff_2048_R2.xx_year-2.fits</strike><br />
| <br />
| <br />
| <br />
| <br />
|<br />
| <br />
| <br />
| <br />
|-<br />
| HFI_CorrMap_353_dustleak-ground_2048_R2.xx_year-1.fits<br />
| <br />
| <br />
| 00<br />
| 24/11/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_CorrMap_353_dustleak-ground_2048_R2.xx_year-2.fits<br />
| <br />
| <br />
| 00<br />
| 24/11/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| <strike>HFI_CorrMap_353-ds1-dustleak-diff_2048_R2.xx_full.fits</strike><br />
| <br />
|<br />
| <br />
| <br />
| <br />
| <br />
| <br />
|<br />
|-<br />
| <strike>HFI_CorrMap_353-ds2-dustleak-diff_2048_R2.xx_full.fits</strike><br />
| <br />
| <br />
| <br />
|<br />
| <br />
| <br />
| <br />
| <br />
|-<br />
| HFI_CorrMap_353-ds1-dustleak-ground_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 24/11/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_CorrMap_353-ds2-dustleak-ground_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 24/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="1"| <span style="color:Blue">CO correction<br>maps</span><br />
| rowspan="1" align="center" | HFI <br />
| <strike>HFI_CorrMap_<freq>-coleak-'''METHOD1'''_2048_R2.xx_full.fits</strike><br />
| <br />
| <br />
| <br />
| <br />
|<br />
| <br />
| <br />
| <br />
|}<br />
<br />
====Covariance matrices====<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=850px<br />
|+ '''Covariance matrices'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" rowspan="4"| Cov. Matrices<br />
| style="text-align:center" rowspan="4"| HFI+LFI<br />
| LFI_NoiseCovMat_030_0016_R2.xx.tgz<br />
| <br />
| <br />
|00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| LFI_NoiseCovMat_044_0016_R2.xx.tgz<br />
| <br />
| <br />
| 00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_NoiseCovMat_070_0016_R2.xx.tgz<br />
| <br />
| <br />
| 00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI covariance matrices<br />
| Not for PR2<br />
| <br />
| 01<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|}<br />
<br />
====CMB maps====<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=1050px<br />
|+ '''CMB Maps'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" rowspan="6" | CMB anisotropy maps<br />
| rowspan="6" align="center" | COM<br />
| COM_CMB_IQU-nilc-field-X_Nside_R2.xx.fits<br />
| <br />
|<br />
|00 <br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_CMB_IQU-sevem-field-X_Nside_R2.xx.fits<br />
| <br />
| <br />
| 00<br />
|09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| COM_CMB_IQU-smica-field-X_Nside_R2.xx.fits<br />
| <br />
| <br />
| 00<br />
|09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_CMB_IQU-commander-field-X_Nside_R2.xx.fits<br />
| <br />
| <br />
| 00<br />
| 09/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| <strike>COM_CMB_IQU-commrul_0256_R2.xx.fits</strike><br />
| <br />
| <br />
| <br />
|<br />
| <br />
| <br />
| <br />
| <br />
|-<br />
| <span style="color:Red"><strike>Other representations</strike></span><br />
| <br />
| <br />
| <br />
|<br />
| <br />
| <br />
| <br />
| <br />
|-<br />
|}<br />
<br />
====Component maps====<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=950px<br />
|+ '''Component Maps'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" rowspan="3" | CO maps<br />
| align="center" rowspan="3"| HFI<br />
| HFI_CompMap_CO-Type1_2048_R2.xx.fits<br />
| <br />
|<br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_CompMap_CO-Type2_2048_R2.xx.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| <strike>HFI_CompMap_CO-Type3_2048_R2.xx.fits</strike><br />
| <br />
| <br />
| <br />
|<br />
| <br />
| <br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="12" | Commander foregrounds<br />
| align="center" rowspan="12"| COM<br />
| COM_CompMap_AME-commander_0256_R2.xx.fits<br />
|<br />
|<br />
| 00<br />
| 11/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| COM_CompMap_CMB-commander_0256_R2.xx.fits<br />
|<br />
|<br />
| 00<br />
| 11/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| COM_CompMap_CO21-commander_2048_R2.xx.fits<br />
|<br />
|<br />
| 00<br />
| 11/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| COM_CompMap_CO-commander_0256_R2.xx.fits<br />
|<br />
|<br />
| 00<br />
| 11/12/2014<br />
| style="background-color: green;" |<br />
|style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_CompMap_dust-commander_0256_R2.xx.fits<br />
|<br />
|<br />
| 00<br />
| 11/12/2014<br />
| style="background-color: green;" |<br />
|style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_CompMap_DustPol-commander_1024_R2.xx.fits<br />
|<br />
|<br />
| 00<br />
| 11/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_CompMap_freefree-commander_0256_R2.xx.fits<br />
|<br />
|<br />
| 00<br />
| 11/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| COM_CompMap_Synchrotron-commander_0256_R2.xx.fits<br />
|<br />
|<br />
| 00<br />
| 11/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| COM_CompMap_SynchrotronPol-commander_0256_R2.xx.fits<br />
|<br />
|<br />
| 00<br />
| 11/12/2014<br />
| style="background-color: green;" |<br />
|style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_CompMap_SZ-commander_0256_R2.xx.fits<br />
|<br />
|<br />
| 00<br />
| 11/12/2014<br />
| style="background-color: green;" |<br />
|style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_CompMap_ThermalDust-commander_2048_R2.xx.fits<br />
|<br />
|<br />
| 00<br />
| 11/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_CompMap_xline-commander_0256_R2.xx.fits<br />
|<br />
|<br />
| 00<br />
| 11/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" | Lensing maps<br />
| align="center" | COM<br />
| COM_CompMap_Lensing_2048_R2.xx.tar + SimMap tars<br />
|<br />
| <br />
|00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
|}<br />
<br />
====Masks====<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=850px<br />
|+ '''Masks'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" rowspan='4'| Masks<br />
| style="text-align:center" | <strike>LFI</strike><br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
|-<br />
| style="text-align:center" | HFI<br />
| HFI_Mask_GalPlane-apo 0 2 5 _2048_R2.xx.fits<br />
|<br />
| <br />
| 00<br />
| 19/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| style="text-align:center" rowspan='2'| COM<br />
| COM_CMB_IQU-common-field-MaskInt_2048_R2.xx.fits<br />
| <br />
|<br />
| 00<br />
| 10/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_CMB_IQU-common-field-MaskPol_1024_R2.xx.fits<br />
| <br />
| <br />
| 00<br />
| 10/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan='2'| Point source masks<br />
| style="text-align:center" rowspan='1'| LFI<br />
| LFI_Mask_PointSrc_2048_R2.xx.fits<br />
| <br />
| <br />
| 00<br />
|27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| style="text-align:center" | HFI<br />
| HFI_Mask_PointSrc_2048_R2.xx.fits<br />
| <br />
| <br />
|00<br />
| 19/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
|}<br />
<br />
===Angular power spectra===<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=1050px<br />
|+ '''Angular power spectra'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" rowspan="2" | CMB angular power spectra<br />
| style="text-align:center" rowspan="2" |COM<br />
| COM_PowerSpect_CMB_R2.xx.fits<br />
|<br />
| <br />
| 00<br />
| 05/02/2015<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| <strike>COM_PowerSpect_CMB_R2.xx.txt</strike><br />
|<br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="1"| <strike>Sky Angular power spectrum</strike><br />
| style="text-align:center" rowspan="4" |<br />
| <strike>LFI_PowerSpect_030_R2.xx.fits</strike><br />
|<br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
| [[#note37|[37]]]<br />
|-<br />
|}<br />
<div id="note37"></div>[37] For this release detector and detector set power spectra will not be provided. Instead the detector and detector set maps will be provided.<br />
<br />
===Characterisation===<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=850px<br />
|+ '''Characterization'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" rowspan="3"| RIMO<br />
| style="text-align:center" | LFI<br />
| LFI_RIMO_R2.xx.fits<br />
| <br />
| <br />
|50<br />
| 16/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| style="text-align:center" | HFI<br />
| HFI_RIMO_R2.xx.fits<br />
| <br />
| <br />
| 00<br />
| 20/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| style="text-align:center" | HFI<br />
| HFI beams RIMO(s)<br />
| <br />
| <br />
| 00<br />
| 05/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
|}<br />
<br />
===Catalogues===<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=850px<br />
|+ '''Catalogues'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" rowspan="9"| PCCS<br />
| style="text-align:center" rowspan="9"| COM<br />
| COM_PCCS_030_R2.xx.fits + excl.<br />
| <br />
| <br />
| 02<br />
|15/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_PCCS_044_R2.xx.fits + excl.<br />
| <br />
| <br />
| 02<br />
|15/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_PCCS_070_R2.xx.fits + excl.<br />
| <br />
| <br />
| 02<br />
| 15/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_PCCS_100_R2.xx.fits<br />
| <br />
| <br />
| 01<br />
| 19/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_PCCS_143_R2.xx.fits<br />
| <br />
| <br />
| 01<br />
| 19/11/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_PCCS_217_R2.xx.fits<br />
| <br />
| <br />
|01<br />
| 19/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_PCCS_353_R2.xx.fits<br />
| <br />
| <br />
| 01<br />
| 19/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_PCCS_545_R2.xx.fits<br />
| <br />
| <br />
| 01<br />
|19/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_PCCS_857_R2.xx.fits<br />
| <br />
| <br />
| 01<br />
|19/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="4"| SZ catalogues<br />
| style="text-align:center" rowspan="4"| COM<br />
| COM_PCCS_SZ-MMF1_R2.xx.fits<br />
| <br />
| <br />
| 08<br />
| 29/01/2015<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_PCCS_SZ-MMF3_R2.xx.fits<br />
| <br />
| <br />
| 08<br />
| 29/01/2015<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
|<br />
|-<br />
| COM_PCCS_SZ-PwS_R2.xx.fits<br />
| <br />
| <br />
| 08<br />
| 29/01/2015<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_PCCS_SZ-union_R2.xx.fits<br />
| <br />
| <br />
| 08<br />
| 03/02/2015<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
|<br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="4"| Other catalogues<br />
| style="text-align:center" rowspan="4"| HFI<br />
| <span style="color:Red"><strike>Dusty source catalogue</strike></span><br />
| <br />
| <br />
|<br />
| <br />
| <br />
| <br />
| <br />
| <br />
|-<br />
| <span style="color:Red"><strike>Radio sources catalogue</strike></span><br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
|-<br />
| <span style="color:Blue">HFI_PCCS_GCC_R2.xx.fits</span><br />
| <br />
| <br />
| 02<br />
| 16/01/2015<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| <span style="color:Blue">High-z catalogue</span><br />
| <br />
| <br />
| <br />
| <br />
|<br />
| <br />
| <br />
| <br />
|-<br />
|}<br />
<br />
===Other products===<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=850px<br />
|+ '''Other products'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" | Cosmological parameters<br />
| style="text-align:center" rowspan="1"| COM<br />
| Cosmological parameter tables<br />
| <br />
| <br />
| 00<br />
| 28/01/2015<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="1"| Codes<br />
| style="text-align:center" rowspan="1"| COM<br />
| Likelihood code<br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
|<br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="11"| Beams<br />
| style="text-align:center" rowspan="5"| <br />
| LFI scanning beams<br />
| <br />
| <br />
| 00<br />
| 21-11-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
| HFI scanning beams<br />
| <br />
| <br />
| 00<br />
| 05/02/2015<br />
| <br />
| <br />
|<br />
| <br />
|-<br />
| Effective beams 30GHz<br />
| <br />
| <br />
| <br />
| 22-09-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
| Effective beams 44GHz<br />
| <br />
| <br />
| <br />
| 24-09-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
| Effective beams 70GHz<br />
| <br />
| <br />
| <br />
| 24-09-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
| style="text-align:center" rowspan="6"| <br />
| Effective beams 100 GHz<br />
| <br />
| <br />
| <br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
| Effective beams 143 GHz<br />
| <br />
| <br />
| <br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
| Effective beams 217 GHz<br />
| <br />
| <br />
| <br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
| Effective beams 353 GHz<br />
| <br />
| <br />
| <br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
| Effective beams 545 GHz<br />
| <br />
| <br />
| <br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
| Effective beams 857 GGz<br />
| <br />
| <br />
| <br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="2"| 4D maps<br />
| style="text-align:center" rowspan="2"| LFI<br />
| Code<br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
|<br />
| [[#noteA|[A]]]<br />
|-<br />
| map4D_calib_DDX11_LFIXX_gal_nsideXXX_npsiXXXX.fits<br />
| <br />
| <br />
| <br />
| 19/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| [[#noteA|[A]]]<br />
|-<br />
!bgcolor="ffdead" scope="row" | Datesobs<br />
| USPDC<br />
| HFI_DatesObs_<Freq>_2048_R2.xx_surveyX.fits.gz<br />
| <br />
| <br />
| 01<br />
|29/01/2015<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" | YSZ package<br />
| COM<br />
| COM_CompMap_YSZ_R2.nn.fits.tgz<br />
| <br />
| 12 Gb<br />
|00<br />
| 05/02/2015<br />
| <br />
| <br />
| <br />
| <br />
|-<br />
|}<br />
<div id="noteA"></div>[A] '''This is not an official product.'''</div>
Xdupac
https://wiki.cosmos.esa.int/planckpla2015/index.php?title=Product_Table_for_PLAv2&diff=11407
Product Table for PLAv2
2015-02-05T10:13:29Z
<p>Xdupac: /* Other products */</p>
<hr />
<div>{{DISPLAYTITLE:Products table for PLAv2}}<br />
==Product categories==<br />
*New products for this release that I believe have been confirmed appear in <span style="color:Blue">blue font</span>, products that are still TBC in <span style="color:Red">red font</span> (if it is one entire category of products I will just use color in the products category name, e.g. <span style="color:Blue">1 year maps</span>). Please check this in the tables and let me know whether there are any errors.<br />
*The Obs column contains links to notes at the end of each table. Please check the notes and let me know your feedback.<br />
*More general comments appear at the end of the numbered notes.<br />
<br />
I suggest you use the [[Talk:Product_Table_for_PLAv2|discussion page associated with this page]] to provide your feedback or make any comments relate to the list of products. The discussion page has the same structures in terms of sections as this page. Please try to write your comments/feedback in the appropriate section. I would also ask you to put your initials in the comments you write so that I can more easily get back to you to try to clarify any questions. Yes, it is true I can find out who wrote what in the history page but it makes my life easier if you associate your name to the comments you provide.<br />
<br />
The '''Description''' column will be used to add a one line description of the product that will appear in the archive as a tooltip associated with the product to allow a quick identification by users.<br />
===Time Series===<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=1050px<br />
|+ '''FITS filenames'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" rowspan="9" | <span style="color:Blue">Detector timeseries</span><br />
|rowspan="3" align="center" | LFI <br />
| LFI_TOI_030-SCI_R2.xx_ODXXXX.fits<br />
| <br />
| <br />
|00 <br />
| 10-09-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| LFI_TOI_044-SCI_R2.xx_ODXXXX.fits<br />
| <br />
| <br />
| 00<br />
| 10-09-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| LFI_TOI_070-SCI_R2.xx_ODXXXX.fits<br />
| <br />
| <br />
| 00<br />
| 10-09-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
|rowspan="6" align="center" | HFI <br />
| HFI_TOI_100-SCI_R2.xx_ODXXXX.fits<br />
| Only PSB: not for Feb. 2015 release<br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
|<br />
|-<br />
| HFI_TOI_143-SCI_R2.xx_ODXXXX.fits<br />
| without PSBs<br />
| <br />
| 00<br />
| 20/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_TOI_217-SCI_R2.xx_ODXXXX.fits<br />
| without PSBs<br />
| <br />
| 00<br />
| 20/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_TOI_353-SCI_R2.xx_ODXXXX.fits<br />
| with PSBs<br />
| <br />
| 00<br />
| 19/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_TOI_545-SCI_R2.xx_ODXXXX.fits<br />
| <br />
| <br />
| 00<br />
| 23/01/2015<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_TOI_857-SCI_R2.xx_ODXXXX.fits<br />
| <br />
| <br />
| 00<br />
| 23/01/2015<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="7" | <span style="color:Blue">Offsets</span><br />
| rowspan="6" align="center"| LFI <br />
| LFI_TOI_030-OFF_R2.xx_ODXXXX-full.fits<br />
| <br />
| <br />
| 00<br />
| 19-09-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_TOI_044-OFF_R2.xx_ODXXXX-full.fits<br />
| <br />
| <br />
| 00<br />
| 19-09-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_TOI_070-OFF_R2.xx_ODXXXX-full.fits<br />
| <br />
| <br />
|00<br />
| 19-09-2014 <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_TOI_030-OFF_R2.xx_ODXXXX-full-ringhalf.fits<br />
| <br />
| <br />
| 00<br />
| 11-11-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_TOI_044-OFF_R2.xx_ODXXXX-full-ringhalf.fits<br />
| <br />
| <br />
| 00<br />
| 11-11-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_TOI_070-OFF_R2.xx_ODXXXX-full-ringhalf.fits<br />
| <br />
| <br />
| 00<br />
| 11-11-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
|align="center"| HFI <br />
| HFI_TOI_AllFreqs-OFF_R2.xx.fits<br />
|<br />
|<br />
|00<br />
|13/01/2015<br />
|style="background-color: green;" |<br />
|style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan=9| <span style="color:Blue">Pointing</span><br />
| align="center" rowspan="3"| LFI <br />
| LFI_TOI_030-PTG_R2.xx_ODXXXX.fits <br />
|<br />
| <br />
|00 <br />
|18-07-2014 <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_TOI_044-PTG_R2.xx_ODXXXX.fits <br />
|<br />
| <br />
| 00 <br />
| 18-07-2014 <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_TOI_070-PTG_R2.xx_ODXXXX.fits <br />
|<br />
| <br />
| 00 <br />
| 18-07-2014 <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| rowspan=6 align="center"| HFI <br />
| HFI_TOI_100-PTG_R2.xx_ODXXXX.fits <br />
|<br />
| <br />
| 01 <br />
| 26-08-2014 <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_TOI_143-PTG_R2.xx_ODXXXX.fits <br />
|<br />
| <br />
| 01 <br />
| 26-08-2014 <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_TOI_217-PTG_R2.xx_ODXXXX.fits <br />
|<br />
| <br />
| 01 <br />
| 26-08-2014 <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_TOI_353-PTG_R2.xx_ODXXXX.fits <br />
|<br />
| <br />
| 01 <br />
| 26-08-2014 <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_TOI_545-PTG_R2.xx_ODXXXX.fits <br />
|<br />
| <br />
| 01 <br />
| 26-08-2014 <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_TOI_857-PTG_R2.xx_ODXXXX.fits <br />
|<br />
| <br />
| 01 <br />
| 26-08-2014 <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="4"| <span style="color:Blue">Time stamps</span><br />
| align="center" rowspan="3"| LFI <br />
| LFI_TOI_030-TAI_R2.xx_ODXXXX.fits <br />
|<br />
| <br />
|00 <br />
| 20-09-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_TOI_044-TAI_R2.xx_ODXXXX.fits <br />
|<br />
| <br />
| 00 <br />
| 20-09-2014 <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_TOI_070-TAI_R2.xx_ODXXXX.fits <br />
|<br />
| <br />
| 00<br />
| 20-09-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| align="center"| HFI <br />
| HFI_TOI_AllFreqs-TAI_R2.xx_ODXXXX.fits <br />
|<br />
| <br />
| 00<br />
| 20-09-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan=8| <span style="color:Blue">HK</span> <br />
|align="center" rowspan="8"| LFI <br />
| LFI_TOI_DAE-FAST-HK_R2.XX_ODXXX.fits<br />
| <br />
| <br />
|00 <br />
|14-08-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| LFI_TOI_DAE-SlowConfiguration-HK_R2.XX_ODXXXX.fits<br />
| <br />
| <br />
|00 <br />
|14-08-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| LFI_TOI_DAE-SlowCurrent-HK_R2.XX_ODXXXX.fits<br />
| <br />
| <br />
|00 <br />
|14-08-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| LFI_TOI_DAE-SlowPhaseSwitch-HK_R2.XX_ODXXXX.fits<br />
| <br />
| <br />
|00 <br />
|14-08-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" | <br />
| <br />
|<br />
|-<br />
| LFI_TOI_DAE-SlowVoltage-HK_R2.XX_ODXXXX.fits<br />
| <br />
| <br />
|00 <br />
|14-08-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" | <br />
| <br />
|<br />
|-<br />
| LFI_TOI_REBA-HK_R2.XX_ODXXXX.fits<br />
| <br />
| <br />
|00 <br />
|14-08-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" | <br />
| <br />
|<br />
|-<br />
| SCS_TOI_EssentialASW(R)-HK_R2.XX_ODXXXX.fits<br />
| <br />
| <br />
|00 <br />
|14-08-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" | <br />
| <br />
| <br />
|-<br />
| SCS_TOI_NonEssentialASW(R)-HK_R2.XX_ODXXXX.fits<br />
| <br />
| <br />
|00 <br />
|14-08-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" | <br />
| <br />
| <br />
|-<br />
|}<br />
<br />
===Maps===<br />
====Sky Maps====<br />
=====All detectors=====<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=1050px<br />
|+ '''All Detectors'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" rowspan="56" | Survey maps<br />
| rowspan="32" align="center"| LFI<br />
| LFI_SkyMap_030_1024_R2.xx_survey-1.fits<br />
| <br />
| <br />
| 01<br />
| 26/01/2015<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_030_1024_R2.xx_survey-2.fits<br />
| <br />
| <br />
| 01<br />
| <br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_030_1024_R2.xx_survey-3.fits<br />
| <br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_030_1024_R2.xx_survey-4.fits<br />
| <br />
| <br />
|01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_030_1024_R2.xx_survey-5.fits<br />
| <br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_030_1024_R2.xx_survey-6.fits<br />
| <br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_030_1024_R2.xx_survey-7.fits<br />
| <br />
|<br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
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|-<br />
| LFI_SkyMap_030_1024_R2.xx_survey-8.fits<br />
| <br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_survey-1.fits<br />
| <br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_survey-2.fits<br />
| <br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_survey-3.fits<br />
| <br />
|<br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_survey-4.fits<br />
|<br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_survey-5.fits<br />
| <br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_survey-6.fits<br />
| <br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_survey-7.fits<br />
| <br />
|<br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_survey-8.fits<br />
| <br />
|<br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_survey-1.fits<br />
|<br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_survey-2.fits<br />
| <br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_survey-3.fits<br />
| <br />
| <br />
|01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_survey-4.fits<br />
| <br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_survey-5.fits<br />
| <br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_survey-6.fits<br />
| <br />
|<br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_survey-7.fits<br />
| <br />
|<br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_survey-8.fits<br />
| <br />
|<br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_2048_R2.xx_survey-1.fits<br />
| <br />
|<br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_2048_R2.xx_survey-2.fits<br />
| <br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_2048_R2.xx_survey-3.fits<br />
| <br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_2048_R2.xx_survey-4.fits<br />
| <br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_2048_R2.xx_survey-5.fits<br />
| <br />
|<br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_2048_R2.xx_survey-6.fits<br />
|<br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_2048_R2.xx_survey-7.fits<br />
| <br />
| <br />
| 01<br />
|<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_2048_R2.xx_survey-8.fits<br />
| <br />
| <br />
| 01<br />
|<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| rowspan="24" align="center"| HFI<br />
| HFI_SkyMap_100_2048_R2.xx_survey-1.fits<br />
| <br />
|<br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_100_2048_R2.xx_survey-2.fits<br />
| <br />
|<br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_100_2048_R2.xx_survey-3.fits<br />
| <br />
|<br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_100_2048_R2.xx_survey-4.fits<br />
| <br />
| <br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_143_2048_R2.xx_survey-1.fits<br />
| <br />
| <br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_143_2048_R2.xx_survey-2.fits<br />
|<br />
| <br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_143_2048_R2.xx_survey-3.fits<br />
| <br />
| <br />
|00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_143_2048_R2.xx_survey-4.fits<br />
| <br />
|<br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_217_2048_R2.xx_survey-1.fits<br />
| <br />
| <br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_217_2048_R2.xx_survey-2.fits<br />
| <br />
| <br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_217_2048_R2.xx_survey-3.fits<br />
| <br />
|<br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_217_2048_R2.xx_survey-4.fits<br />
| <br />
|<br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_353_2048_R2.xx_survey-1.fits<br />
| <br />
| <br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_353_2048_R2.xx_survey-2.fits<br />
| <br />
|<br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_353_2048_R2.xx_survey-3.fits<br />
| <br />
| <br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_353_2048_R2.xx_survey-4.fits<br />
| <br />
| <br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_545_2048_R2.xx_survey-1.fits<br />
| <br />
| <br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_545_2048_R2.xx_survey-2.fits<br />
| <br />
|<br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_545_2048_R2.xx_survey-3.fits<br />
| <br />
| <br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_545_2048_R2.xx_survey-4.fits<br />
| <br />
| <br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_857_2048_R2.xx_survey-1.fits<br />
| <br />
| <br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_857_2048_R2.xx_survey-2.fits<br />
|<br />
| <br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_857_2048_R2.xx_survey-3.fits<br />
| <br />
| <br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_857_2048_R2.xx_survey-4.fits<br />
| <br />
| <br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="28" | <span style="color:Blue">1 year maps</span> <br />
1 year = 2 surveys<br />
<br />
y1=s1+s2<br />
<br />
y2=s3+s4<br />
<br />
y3=s5+s6<br />
<br />
y4=s7+s8<br />
| rowspan="16" align="center" | LFI<br />
| LFI_SkyMap_030_1024_R2.xx_year-1.fits<br />
| <br />
|<br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_030_1024_R2.xx_year-2.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_030_1024_R2.xx_year-3.fits<br />
| <br />
|<br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_030_1024_R2.xx_year-4.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_year-1.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_year-2.fits<br />
| <br />
| <br />
|00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_year-3.fits<br />
| <br />
|<br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_year-4.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_year-1.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_year-2.fits<br />
| <br />
|<br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_year-3.fits<br />
| <br />
|<br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_year-4.fits<br />
| <br />
| <br />
|00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_2048_R2.xx_year-1.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_2048_R2.xx_year-2.fits<br />
| <br />
|<br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_2048_R2.xx_year-3.fits<br />
| <br />
|<br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_2048_R2.xx_year-4.fits<br />
| <br />
| <br />
|00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| rowspan="12" align="center" | HFI<br />
| HFI_SkyMap_100_2048_R2.xx_year-1.fits<br />
| <br />
| <br />
| 00 <br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_100_2048_R2.xx_year-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_143_2048_R2.xx_year-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_143_2048_R2.xx_year-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_217_2048_R2.xx_year-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_217_2048_R2.xx_year-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_353_2048_R2.xx_year-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_353_2048_R2.xx_year-2.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_545_2048_R2.xx_year-1.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_545_2048_R2.xx_year-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_857_2048_R2.xx_year-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_857_2048_R2.xx_year-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="12" | <span style="color:Blue">Half mission maps</span><br />
| rowspan="12" align="center"| HFI<br />
| HFI_SkyMap_100_2048_R2.xx_halfmission-1.fits<br />
| <br />
| <br />
| 00 <br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_100_2048_R2.xx_halfmission-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_143_2048_R2.xx_halfmission-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_143_2048_R2.xx_halfmission-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_217_2048_R2.xx_halfmission-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_217_2048_R2.xx_halfmission-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_353_2048_R2.xx_halfmission-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_353_2048_R2.xx_halfmission-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_545_2048_R2.xx_halfmission-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_545_2048_R2.xx_halfmission-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_857_2048_R2.xx_halfmission-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_857_2048_R2.xx_halfmission-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="12" | <span style="color:Blue">Multi year maps</span><br />
| rowspan="12" align="center"| LFI<br />
| LFI_SkyMap_030_1024_R2.xx_year-1-2.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_030_1024_R2.xx_year-1-3.fits<br />
| <br />
| <br />
| 00<br />
| 21/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_030_1024_R2.xx_year-2-4.fits<br />
| <br />
| <br />
| 00<br />
| 21/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_030_1024_R2.xx_year-3-4.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_year-1-2.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_year-1-3.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_year-2-4.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_year-3-4.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_year-1-2.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_year-1-3.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_year-2-4.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_year-3-4.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="20" | Half-ring maps <br />
| rowspan="8" align="center" | LFI <br />
| LFI_SkyMap_030_1024_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
|00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_030_1024_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| rowspan="12" align="center" | HFI <br />
| HFI_SkyMap_100_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_100_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_143_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_143_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_217_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_217_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_353_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_353_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_545_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_545_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_857_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_857_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="10" | Frequency Maps <br />
| rowspan="4" align="center" | LFI <br />
| LFI_SkyMap_030_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| rowspan="6" align="center" | HFI <br />
| HFI_SkyMap_100_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_143_2048_R2.xx_full.fits<br />
| <br />
|<br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_217_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_353_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_545_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_857_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" | Zodi correction maps <br />
| align="center" | HFI <br />
| HFI_CorrMap_<Freq>-Zodi_2048_R2.xx_<Coverage>.fits<br />
| <br />
| <br />
| 00<br />
| 16/12/2014<br />
| style="background-color: green;" |<br />
|style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
|}<br />
<br />
=====Detector maps=====<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=950px<br />
|+ '''HFI detector maps/LFI radiometer maps'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" rowspan="40" | <span style="color:Blue">Full mission</span><br />
| rowspan="22" align="center" | LFI<br />
| LFI_SkyMap_030-27M_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_030-27S_1024_R2.xx_full.fits<br />
| <br />
| <br />
|00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_030-28M_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_030-28S_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_044-24M_1024_R2.xx_full.fits<br />
| <br />
|<br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_044-24S_1024_R2.xx_full.fits<br />
| <br />
|<br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_044-25M_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
|style="background-color: green;" |<br />
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!bgcolor="ffdead" scope="row" rowspan="80" | <span style="color:Blue">Half rings</span><br />
| rowspan="44" align="center" | LFI<br />
| LFI_SkyMap_030-27M_1024_R2.xx_full-ringhalf-1.fits<br />
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| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_070-22M_1024_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_070-22M_1024_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
|00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_070-22S_1024_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
|00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_070-22S_1024_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_070-23M_1024_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_070-23M_1024_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
|00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_070-23S_1024_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
|00<br />
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| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_070-23S_1024_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| rowspan="36" align="center" | HFI<br />
| HFI_SkyMap_143-5_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
|style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_143-5_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_143-6_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_143-6_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
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|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_143-7_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
|| HFI_SkyMap_143-7_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
|<br />
| 00 <br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_217-1_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_217-1_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_217-2_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
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|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_217-2_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
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| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_217-3_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_217-3_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
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| style="background-color: green;" |<br />
|style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_217-4_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_217-4_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_353-1_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_353-1_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_353-2_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
|00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_353-2_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_353-7_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_353-7_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
|<br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_353-8_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_353-8_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_545-1_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_545-1_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_545-2_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_545-2_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_545-4_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_545-4_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_857-1_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
|00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_857-1_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_857-2_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_857-2_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_857-3_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
|00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_857-3_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_857-4_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_857-4_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|}<br />
<br />
=====Detector set maps=====<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=1050px<br />
|+ '''Detector set maps'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" rowspan="16" | <span style="color:Blue">Full mission</span><br />
| rowspan="8" align="center" | LFI<br />
| LFI_SkyMap_044-24_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| [[#note12|[12]]]<br />
|-<br />
| LFI_SkyMap_044-25-26_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| [[#note12|[12]]]<br />
|-<br />
| LFI_SkyMap_070-18-23_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note12|[12]]]<br />
|-<br />
| LFI_SkyMap_070-19-22_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note12|[12]]]<br />
|-<br />
| LFI_SkyMap_070-20-21_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note12|[12]]]<br />
|-<br />
| LFI_SkyMap_070-18-23_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note12|[12]]]<br />
|-<br />
| LFI_SkyMap_070-19-22_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note12|[12]]]<br />
|-<br />
| LFI_SkyMap_070-20-21_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note12|[12]]]<br />
|-<br />
| rowspan="8" align="center" | HFI<br />
| HFI_SkyMap_100-ds1_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_100-ds2_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_143-ds1_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_143-ds2_2048_R2.xx_full.fits<br />
| <br />
| <br />
|00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_217-ds1_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_217-ds2_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_353-ds1_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_353-ds2_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="26" | <span style="color:Blue">Half rings</span><br />
| rowspan="10" align="center" | LFI<br />
| LFI_SkyMap_044-24_1024_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044-24_1024_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044-25-26_1024_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044-25-26_1024_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070-18-23_1024_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
|00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070-18-23_1024_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070-19-22_1024_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070-19-22_1024_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070-20-21_1024_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070-20-21_1024_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| rowspan="16" align="center" | HFI<br />
| HFI_SkyMap_100-ds1_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
|<br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_100-ds1_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_100-ds2_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_100-ds2_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_143-ds1_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_143-ds1_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
|style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_143-ds2_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_143-ds2_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_217-ds1_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
|00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
|| HFI_SkyMap_217-ds1_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
|00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_217-ds2_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_217-ds2_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_353-ds1_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_353-ds1_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_353-ds2_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_353-ds2_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|}<br />
<br />
=====Low resolution maps=====<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=950px<br />
|+ '''Low resolution maps (with noise cov. mat.)'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" rowspan="2"|Low resolution maps (with noise cov. mat.)<br />
| align="center" | LFI<br />
| LFI_SkyMap_fff_0016_R2.xx_full.fits<br />
| <br />
| <br />
|00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| align="center" | HFI <br />
| HFI_SkyMap_fff_0016_R2.xx_full.fits<br />
| Not for PR2<br />
| <br />
| 01<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|}<br />
<br />
=====Correction maps=====<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=1300px<br />
|+ '''Correction maps'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" rowspan="1"| <span style="color:Red">A correction maps</span><br />
| rowspan="10" align="center" | LFI<br />
| <strike>LFI_CorrMap_030-ACorr_NSNS_R2.xx_full.fits</strike><br />
| <br />
| <br />
| <br />
| <br />
|<br />
| <br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="9"| <span style="color:Blue">Band pass correction<br>maps</span><br />
| LFI_CorrMap_030-BPassCorr_0256_R2.xx_full.fits<br />
| <br />
| <br />
|00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_CorrMap_044-BPassCorr_0256_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
| LFI_CorrMap_070-BPassCorr_0256_R2.xx_full.fits<br />
| <br />
| <br />
|00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_CorrMap_030-BPassCorr_0128_R2.xx_full.fits<br />
| <br />
| <br />
|00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_CorrMap_044-BPassCorr_0128_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
| LFI_CorrMap_070-BPassCorr_0128_R2.xx_full.fits<br />
| <br />
| <br />
|00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_CorrMap_030-BPassCorr_0064_R2.xx_full.fits<br />
| <br />
| <br />
|00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_CorrMap_044-BPassCorr_0064_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
| LFI_CorrMap_070-BPassCorr_0064_R2.xx_full.fits<br />
| <br />
| <br />
|00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="12"| <span style="color:Blue">Dust correction<br>maps</span><br />
| rowspan="12" align="center" |HFI <br />
| HFI_CorrMap 353 GHz leakage global fits maps<br />
| <br />
| <br />
| 00<br />
| 09/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| <strike>HFI_CorrMap_100-dustleak-ground_2048_R2.xx_full.fits</strike><br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
|<br />
|-<br />
| <strike>HFI_CorrMap_353-dustleak-diff_2048_R2.xx_full.fits</strike><br />
| <br />
| <br />
| <br />
| <br />
|<br />
| <br />
| <br />
| <br />
|-<br />
| HFI_CorrMap_353-dustleak-ground_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
|24/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| <strike>HFI_CorrMap_353_dustleak-diff_2048_R2.xx_year-1.fits</strike><br />
| <br />
| <br />
| <br />
|<br />
| <br />
| <br />
| <br />
| <br />
|-<br />
| <strike>HFI_CorrMap_353_dustleak-diff_2048_R2.xx_year-2.fits</strike><br />
| <br />
| <br />
| <br />
| <br />
|<br />
| <br />
| <br />
| <br />
|-<br />
| HFI_CorrMap_353_dustleak-ground_2048_R2.xx_year-1.fits<br />
| <br />
| <br />
| 00<br />
| 24/11/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_CorrMap_353_dustleak-ground_2048_R2.xx_year-2.fits<br />
| <br />
| <br />
| 00<br />
| 24/11/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| <strike>HFI_CorrMap_353-ds1-dustleak-diff_2048_R2.xx_full.fits</strike><br />
| <br />
|<br />
| <br />
| <br />
| <br />
| <br />
| <br />
|<br />
|-<br />
| <strike>HFI_CorrMap_353-ds2-dustleak-diff_2048_R2.xx_full.fits</strike><br />
| <br />
| <br />
| <br />
|<br />
| <br />
| <br />
| <br />
| <br />
|-<br />
| HFI_CorrMap_353-ds1-dustleak-ground_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 24/11/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_CorrMap_353-ds2-dustleak-ground_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 24/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="1"| <span style="color:Blue">CO correction<br>maps</span><br />
| rowspan="1" align="center" | HFI <br />
| <strike>HFI_CorrMap_<freq>-coleak-'''METHOD1'''_2048_R2.xx_full.fits</strike><br />
| <br />
| <br />
| <br />
| <br />
|<br />
| <br />
| <br />
| <br />
|}<br />
<br />
====Covariance matrices====<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=850px<br />
|+ '''Covariance matrices'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" rowspan="4"| Cov. Matrices<br />
| style="text-align:center" rowspan="4"| HFI+LFI<br />
| LFI_NoiseCovMat_030_0016_R2.xx.tgz<br />
| <br />
| <br />
|00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| LFI_NoiseCovMat_044_0016_R2.xx.tgz<br />
| <br />
| <br />
| 00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_NoiseCovMat_070_0016_R2.xx.tgz<br />
| <br />
| <br />
| 00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI covariance matrices<br />
| Not for PR2<br />
| <br />
| 01<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|}<br />
<br />
====CMB maps====<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=1050px<br />
|+ '''CMB Maps'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" rowspan="6" | CMB anisotropy maps<br />
| rowspan="6" align="center" | COM<br />
| COM_CMB_IQU-nilc-field-X_Nside_R2.xx.fits<br />
| <br />
|<br />
|00 <br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_CMB_IQU-sevem-field-X_Nside_R2.xx.fits<br />
| <br />
| <br />
| 00<br />
|09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| COM_CMB_IQU-smica-field-X_Nside_R2.xx.fits<br />
| <br />
| <br />
| 00<br />
|09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_CMB_IQU-commander-field-X_Nside_R2.xx.fits<br />
| <br />
| <br />
| 00<br />
| 09/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| <strike>COM_CMB_IQU-commrul_0256_R2.xx.fits</strike><br />
| <br />
| <br />
| <br />
|<br />
| <br />
| <br />
| <br />
| <br />
|-<br />
| <span style="color:Red"><strike>Other representations</strike></span><br />
| <br />
| <br />
| <br />
|<br />
| <br />
| <br />
| <br />
| <br />
|-<br />
|}<br />
<br />
====Component maps====<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=950px<br />
|+ '''Component Maps'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" rowspan="3" | CO maps<br />
| align="center" rowspan="3"| HFI<br />
| HFI_CompMap_CO-Type1_2048_R2.xx.fits<br />
| <br />
|<br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_CompMap_CO-Type2_2048_R2.xx.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| <strike>HFI_CompMap_CO-Type3_2048_R2.xx.fits</strike><br />
| <br />
| <br />
| <br />
|<br />
| <br />
| <br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="12" | Commander foregrounds<br />
| align="center" rowspan="12"| COM<br />
| COM_CompMap_AME-commander_0256_R2.xx.fits<br />
|<br />
|<br />
| 00<br />
| 11/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| COM_CompMap_CMB-commander_0256_R2.xx.fits<br />
|<br />
|<br />
| 00<br />
| 11/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| COM_CompMap_CO21-commander_2048_R2.xx.fits<br />
|<br />
|<br />
| 00<br />
| 11/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| COM_CompMap_CO-commander_0256_R2.xx.fits<br />
|<br />
|<br />
| 00<br />
| 11/12/2014<br />
| style="background-color: green;" |<br />
|style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_CompMap_dust-commander_0256_R2.xx.fits<br />
|<br />
|<br />
| 00<br />
| 11/12/2014<br />
| style="background-color: green;" |<br />
|style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_CompMap_DustPol-commander_1024_R2.xx.fits<br />
|<br />
|<br />
| 00<br />
| 11/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_CompMap_freefree-commander_0256_R2.xx.fits<br />
|<br />
|<br />
| 00<br />
| 11/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| COM_CompMap_Synchrotron-commander_0256_R2.xx.fits<br />
|<br />
|<br />
| 00<br />
| 11/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| COM_CompMap_SynchrotronPol-commander_0256_R2.xx.fits<br />
|<br />
|<br />
| 00<br />
| 11/12/2014<br />
| style="background-color: green;" |<br />
|style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_CompMap_SZ-commander_0256_R2.xx.fits<br />
|<br />
|<br />
| 00<br />
| 11/12/2014<br />
| style="background-color: green;" |<br />
|style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_CompMap_ThermalDust-commander_2048_R2.xx.fits<br />
|<br />
|<br />
| 00<br />
| 11/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_CompMap_xline-commander_0256_R2.xx.fits<br />
|<br />
|<br />
| 00<br />
| 11/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" | Lensing maps<br />
| align="center" | COM<br />
| COM_CompMap_Lensing_2048_R2.xx.tar + SimMap tars<br />
|<br />
| <br />
|00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
|}<br />
<br />
====Masks====<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=850px<br />
|+ '''Masks'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" rowspan='4'| Masks<br />
| style="text-align:center" | <strike>LFI</strike><br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
|-<br />
| style="text-align:center" | HFI<br />
| HFI_Mask_GalPlane-apo 0 2 5 _2048_R2.xx.fits<br />
|<br />
| <br />
| 00<br />
| 19/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| style="text-align:center" rowspan='2'| COM<br />
| COM_CMB_IQU-common-field-MaskInt_2048_R2.xx.fits<br />
| <br />
|<br />
| 00<br />
| 10/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_CMB_IQU-common-field-MaskPol_1024_R2.xx.fits<br />
| <br />
| <br />
| 00<br />
| 10/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan='2'| Point source masks<br />
| style="text-align:center" rowspan='1'| LFI<br />
| LFI_Mask_PointSrc_2048_R2.xx.fits<br />
| <br />
| <br />
| 00<br />
|27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| style="text-align:center" | HFI<br />
| HFI_Mask_PointSrc_2048_R2.xx.fits<br />
| <br />
| <br />
|00<br />
| 19/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
|}<br />
<br />
===Angular power spectra===<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=1050px<br />
|+ '''Angular power spectra'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" rowspan="2" | CMB angular power spectra<br />
| style="text-align:center" rowspan="2" |COM<br />
| COM_PowerSpect_CMB_R2.xx.fits<br />
|<br />
| <br />
| 00<br />
| 05/02/2015<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| <strike>COM_PowerSpect_CMB_R2.xx.txt</strike><br />
|<br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="1"| <strike>Sky Angular power spectrum</strike><br />
| style="text-align:center" rowspan="4" |<br />
| <strike>LFI_PowerSpect_030_R2.xx.fits</strike><br />
|<br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
| [[#note37|[37]]]<br />
|-<br />
|}<br />
<div id="note37"></div>[37] For this release detector and detector set power spectra will not be provided. Instead the detector and detector set maps will be provided.<br />
<br />
===Characterisation===<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=850px<br />
|+ '''Characterization'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" rowspan="3"| RIMO<br />
| style="text-align:center" | LFI<br />
| LFI_RIMO_R2.xx.fits<br />
| <br />
| <br />
|50<br />
| 16/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| style="text-align:center" | HFI<br />
| HFI_RIMO_R2.xx.fits<br />
| <br />
| <br />
| 00<br />
| 20/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| style="text-align:center" | HFI<br />
| HFI beams RIMO(s)<br />
| <br />
| <br />
| 00<br />
| 05/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
|}<br />
<br />
===Catalogues===<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=850px<br />
|+ '''Catalogues'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" rowspan="9"| PCCS<br />
| style="text-align:center" rowspan="9"| COM<br />
| COM_PCCS_030_R2.xx.fits + excl.<br />
| <br />
| <br />
| 02<br />
|15/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_PCCS_044_R2.xx.fits + excl.<br />
| <br />
| <br />
| 02<br />
|15/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_PCCS_070_R2.xx.fits + excl.<br />
| <br />
| <br />
| 02<br />
| 15/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_PCCS_100_R2.xx.fits<br />
| <br />
| <br />
| 01<br />
| 19/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_PCCS_143_R2.xx.fits<br />
| <br />
| <br />
| 01<br />
| 19/11/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_PCCS_217_R2.xx.fits<br />
| <br />
| <br />
|01<br />
| 19/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_PCCS_353_R2.xx.fits<br />
| <br />
| <br />
| 01<br />
| 19/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_PCCS_545_R2.xx.fits<br />
| <br />
| <br />
| 01<br />
|19/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_PCCS_857_R2.xx.fits<br />
| <br />
| <br />
| 01<br />
|19/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="4"| SZ catalogues<br />
| style="text-align:center" rowspan="4"| COM<br />
| COM_PCCS_SZ-MMF1_R2.xx.fits<br />
| <br />
| <br />
| 08<br />
| 29/01/2015<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_PCCS_SZ-MMF3_R2.xx.fits<br />
| <br />
| <br />
| 08<br />
| 29/01/2015<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
|<br />
|-<br />
| COM_PCCS_SZ-PwS_R2.xx.fits<br />
| <br />
| <br />
| 08<br />
| 29/01/2015<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_PCCS_SZ-union_R2.xx.fits<br />
| <br />
| <br />
| 08<br />
| 03/02/2015<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
|<br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="4"| Other catalogues<br />
| style="text-align:center" rowspan="4"| HFI<br />
| <span style="color:Red"><strike>Dusty source catalogue</strike></span><br />
| <br />
| <br />
|<br />
| <br />
| <br />
| <br />
| <br />
| <br />
|-<br />
| <span style="color:Red"><strike>Radio sources catalogue</strike></span><br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
|-<br />
| <span style="color:Blue">HFI_PCCS_GCC_R2.xx.fits</span><br />
| <br />
| <br />
| 02<br />
| 16/01/2015<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| <span style="color:Blue">High-z catalogue</span><br />
| <br />
| <br />
| <br />
| <br />
|<br />
| <br />
| <br />
| <br />
|-<br />
|}<br />
<br />
===Other products===<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=850px<br />
|+ '''Other products'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" | Cosmological parameters<br />
| style="text-align:center" rowspan="1"| COM<br />
| Cosmological parameter tables<br />
| <br />
| <br />
| 00<br />
| 28/01/2015<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="1"| Codes<br />
| style="text-align:center" rowspan="1"| COM<br />
| Likelihood code<br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
|<br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="11"| Beams<br />
| style="text-align:center" rowspan="5"| <br />
| LFI scanning beams<br />
| <br />
| <br />
| 00<br />
| 21-11-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
| HFI scanning beams<br />
| <br />
| <br />
| 00<br />
| 05/02/2015<br />
| <br />
| <br />
|<br />
| <br />
|-<br />
| Effective beams 30GHz<br />
| <br />
| <br />
| <br />
| 22-09-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
| Effective beams 44GHz<br />
| <br />
| <br />
| <br />
| 24-09-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
| Effective beams 70GHz<br />
| <br />
| <br />
| <br />
| 24-09-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
| style="text-align:center" rowspan="6"| <br />
| Effective beams 100 GHz<br />
| <br />
| <br />
| <br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
| Effective beams 143 GHz<br />
| <br />
| <br />
| <br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
| Effective beams 217 GHz<br />
| <br />
| <br />
| <br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
| Effective beams 353 GHz<br />
| <br />
| <br />
| <br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
| Effective beams 545 GHz<br />
| <br />
| <br />
| <br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
| Effective beams 857 GGz<br />
| <br />
| <br />
| <br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="2"| 4D maps<br />
| style="text-align:center" rowspan="2"| LFI<br />
| Code<br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
|<br />
| [[#noteA|[A]]]<br />
|-<br />
| map4D_calib_DDX11_LFIXX_gal_nsideXXX_npsiXXXX.fits<br />
| <br />
| <br />
| <br />
| 19/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| [[#noteA|[A]]]<br />
|-<br />
!bgcolor="ffdead" scope="row" | Datesobs<br />
| USPDC<br />
| HFI_DatesObs_<Freq>_2048_R2.xx_surveyX.fits.gz<br />
| <br />
| <br />
| 01<br />
|29/01/2015<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" | YSZ package<br />
| COM<br />
| COM_CompMap_YSZ_R2.nn.fits.tgz<br />
| 12 Gb<br />
| <br />
|00<br />
| 05/02/2015<br />
| <br />
| <br />
| <br />
| <br />
|-<br />
|}<br />
<div id="noteA"></div>[A] '''This is not an official product.'''</div>
Xdupac
https://wiki.cosmos.esa.int/planckpla2015/index.php?title=Product_Table_for_PLAv2&diff=11406
Product Table for PLAv2
2015-02-05T10:11:23Z
<p>Xdupac: /* Angular power spectra */</p>
<hr />
<div>{{DISPLAYTITLE:Products table for PLAv2}}<br />
==Product categories==<br />
*New products for this release that I believe have been confirmed appear in <span style="color:Blue">blue font</span>, products that are still TBC in <span style="color:Red">red font</span> (if it is one entire category of products I will just use color in the products category name, e.g. <span style="color:Blue">1 year maps</span>). Please check this in the tables and let me know whether there are any errors.<br />
*The Obs column contains links to notes at the end of each table. Please check the notes and let me know your feedback.<br />
*More general comments appear at the end of the numbered notes.<br />
<br />
I suggest you use the [[Talk:Product_Table_for_PLAv2|discussion page associated with this page]] to provide your feedback or make any comments relate to the list of products. The discussion page has the same structures in terms of sections as this page. Please try to write your comments/feedback in the appropriate section. I would also ask you to put your initials in the comments you write so that I can more easily get back to you to try to clarify any questions. Yes, it is true I can find out who wrote what in the history page but it makes my life easier if you associate your name to the comments you provide.<br />
<br />
The '''Description''' column will be used to add a one line description of the product that will appear in the archive as a tooltip associated with the product to allow a quick identification by users.<br />
===Time Series===<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=1050px<br />
|+ '''FITS filenames'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" rowspan="9" | <span style="color:Blue">Detector timeseries</span><br />
|rowspan="3" align="center" | LFI <br />
| LFI_TOI_030-SCI_R2.xx_ODXXXX.fits<br />
| <br />
| <br />
|00 <br />
| 10-09-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| LFI_TOI_044-SCI_R2.xx_ODXXXX.fits<br />
| <br />
| <br />
| 00<br />
| 10-09-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| LFI_TOI_070-SCI_R2.xx_ODXXXX.fits<br />
| <br />
| <br />
| 00<br />
| 10-09-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
|rowspan="6" align="center" | HFI <br />
| HFI_TOI_100-SCI_R2.xx_ODXXXX.fits<br />
| Only PSB: not for Feb. 2015 release<br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
|<br />
|-<br />
| HFI_TOI_143-SCI_R2.xx_ODXXXX.fits<br />
| without PSBs<br />
| <br />
| 00<br />
| 20/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_TOI_217-SCI_R2.xx_ODXXXX.fits<br />
| without PSBs<br />
| <br />
| 00<br />
| 20/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_TOI_353-SCI_R2.xx_ODXXXX.fits<br />
| with PSBs<br />
| <br />
| 00<br />
| 19/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_TOI_545-SCI_R2.xx_ODXXXX.fits<br />
| <br />
| <br />
| 00<br />
| 23/01/2015<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_TOI_857-SCI_R2.xx_ODXXXX.fits<br />
| <br />
| <br />
| 00<br />
| 23/01/2015<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="7" | <span style="color:Blue">Offsets</span><br />
| rowspan="6" align="center"| LFI <br />
| LFI_TOI_030-OFF_R2.xx_ODXXXX-full.fits<br />
| <br />
| <br />
| 00<br />
| 19-09-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_TOI_044-OFF_R2.xx_ODXXXX-full.fits<br />
| <br />
| <br />
| 00<br />
| 19-09-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_TOI_070-OFF_R2.xx_ODXXXX-full.fits<br />
| <br />
| <br />
|00<br />
| 19-09-2014 <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_TOI_030-OFF_R2.xx_ODXXXX-full-ringhalf.fits<br />
| <br />
| <br />
| 00<br />
| 11-11-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_TOI_044-OFF_R2.xx_ODXXXX-full-ringhalf.fits<br />
| <br />
| <br />
| 00<br />
| 11-11-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_TOI_070-OFF_R2.xx_ODXXXX-full-ringhalf.fits<br />
| <br />
| <br />
| 00<br />
| 11-11-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
|align="center"| HFI <br />
| HFI_TOI_AllFreqs-OFF_R2.xx.fits<br />
|<br />
|<br />
|00<br />
|13/01/2015<br />
|style="background-color: green;" |<br />
|style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan=9| <span style="color:Blue">Pointing</span><br />
| align="center" rowspan="3"| LFI <br />
| LFI_TOI_030-PTG_R2.xx_ODXXXX.fits <br />
|<br />
| <br />
|00 <br />
|18-07-2014 <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_TOI_044-PTG_R2.xx_ODXXXX.fits <br />
|<br />
| <br />
| 00 <br />
| 18-07-2014 <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_TOI_070-PTG_R2.xx_ODXXXX.fits <br />
|<br />
| <br />
| 00 <br />
| 18-07-2014 <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| rowspan=6 align="center"| HFI <br />
| HFI_TOI_100-PTG_R2.xx_ODXXXX.fits <br />
|<br />
| <br />
| 01 <br />
| 26-08-2014 <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_TOI_143-PTG_R2.xx_ODXXXX.fits <br />
|<br />
| <br />
| 01 <br />
| 26-08-2014 <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_TOI_217-PTG_R2.xx_ODXXXX.fits <br />
|<br />
| <br />
| 01 <br />
| 26-08-2014 <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_TOI_353-PTG_R2.xx_ODXXXX.fits <br />
|<br />
| <br />
| 01 <br />
| 26-08-2014 <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_TOI_545-PTG_R2.xx_ODXXXX.fits <br />
|<br />
| <br />
| 01 <br />
| 26-08-2014 <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_TOI_857-PTG_R2.xx_ODXXXX.fits <br />
|<br />
| <br />
| 01 <br />
| 26-08-2014 <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="4"| <span style="color:Blue">Time stamps</span><br />
| align="center" rowspan="3"| LFI <br />
| LFI_TOI_030-TAI_R2.xx_ODXXXX.fits <br />
|<br />
| <br />
|00 <br />
| 20-09-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_TOI_044-TAI_R2.xx_ODXXXX.fits <br />
|<br />
| <br />
| 00 <br />
| 20-09-2014 <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_TOI_070-TAI_R2.xx_ODXXXX.fits <br />
|<br />
| <br />
| 00<br />
| 20-09-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| align="center"| HFI <br />
| HFI_TOI_AllFreqs-TAI_R2.xx_ODXXXX.fits <br />
|<br />
| <br />
| 00<br />
| 20-09-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan=8| <span style="color:Blue">HK</span> <br />
|align="center" rowspan="8"| LFI <br />
| LFI_TOI_DAE-FAST-HK_R2.XX_ODXXX.fits<br />
| <br />
| <br />
|00 <br />
|14-08-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| LFI_TOI_DAE-SlowConfiguration-HK_R2.XX_ODXXXX.fits<br />
| <br />
| <br />
|00 <br />
|14-08-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| LFI_TOI_DAE-SlowCurrent-HK_R2.XX_ODXXXX.fits<br />
| <br />
| <br />
|00 <br />
|14-08-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| LFI_TOI_DAE-SlowPhaseSwitch-HK_R2.XX_ODXXXX.fits<br />
| <br />
| <br />
|00 <br />
|14-08-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" | <br />
| <br />
|<br />
|-<br />
| LFI_TOI_DAE-SlowVoltage-HK_R2.XX_ODXXXX.fits<br />
| <br />
| <br />
|00 <br />
|14-08-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" | <br />
| <br />
|<br />
|-<br />
| LFI_TOI_REBA-HK_R2.XX_ODXXXX.fits<br />
| <br />
| <br />
|00 <br />
|14-08-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" | <br />
| <br />
|<br />
|-<br />
| SCS_TOI_EssentialASW(R)-HK_R2.XX_ODXXXX.fits<br />
| <br />
| <br />
|00 <br />
|14-08-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" | <br />
| <br />
| <br />
|-<br />
| SCS_TOI_NonEssentialASW(R)-HK_R2.XX_ODXXXX.fits<br />
| <br />
| <br />
|00 <br />
|14-08-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" | <br />
| <br />
| <br />
|-<br />
|}<br />
<br />
===Maps===<br />
====Sky Maps====<br />
=====All detectors=====<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=1050px<br />
|+ '''All Detectors'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" rowspan="56" | Survey maps<br />
| rowspan="32" align="center"| LFI<br />
| LFI_SkyMap_030_1024_R2.xx_survey-1.fits<br />
| <br />
| <br />
| 01<br />
| 26/01/2015<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_030_1024_R2.xx_survey-2.fits<br />
| <br />
| <br />
| 01<br />
| <br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_030_1024_R2.xx_survey-3.fits<br />
| <br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_030_1024_R2.xx_survey-4.fits<br />
| <br />
| <br />
|01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_030_1024_R2.xx_survey-5.fits<br />
| <br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_030_1024_R2.xx_survey-6.fits<br />
| <br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_030_1024_R2.xx_survey-7.fits<br />
| <br />
|<br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_030_1024_R2.xx_survey-8.fits<br />
| <br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_survey-1.fits<br />
| <br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_survey-2.fits<br />
| <br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_survey-3.fits<br />
| <br />
|<br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_survey-4.fits<br />
|<br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_survey-5.fits<br />
| <br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_survey-6.fits<br />
| <br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_survey-7.fits<br />
| <br />
|<br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_survey-8.fits<br />
| <br />
|<br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_survey-1.fits<br />
|<br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_survey-2.fits<br />
| <br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_survey-3.fits<br />
| <br />
| <br />
|01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_survey-4.fits<br />
| <br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_survey-5.fits<br />
| <br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_survey-6.fits<br />
| <br />
|<br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_survey-7.fits<br />
| <br />
|<br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_survey-8.fits<br />
| <br />
|<br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_2048_R2.xx_survey-1.fits<br />
| <br />
|<br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_2048_R2.xx_survey-2.fits<br />
| <br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_2048_R2.xx_survey-3.fits<br />
| <br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_2048_R2.xx_survey-4.fits<br />
| <br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_2048_R2.xx_survey-5.fits<br />
| <br />
|<br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_2048_R2.xx_survey-6.fits<br />
|<br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_2048_R2.xx_survey-7.fits<br />
| <br />
| <br />
| 01<br />
|<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_2048_R2.xx_survey-8.fits<br />
| <br />
| <br />
| 01<br />
|<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| rowspan="24" align="center"| HFI<br />
| HFI_SkyMap_100_2048_R2.xx_survey-1.fits<br />
| <br />
|<br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_100_2048_R2.xx_survey-2.fits<br />
| <br />
|<br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_100_2048_R2.xx_survey-3.fits<br />
| <br />
|<br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_100_2048_R2.xx_survey-4.fits<br />
| <br />
| <br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_143_2048_R2.xx_survey-1.fits<br />
| <br />
| <br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_143_2048_R2.xx_survey-2.fits<br />
|<br />
| <br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_143_2048_R2.xx_survey-3.fits<br />
| <br />
| <br />
|00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_143_2048_R2.xx_survey-4.fits<br />
| <br />
|<br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_217_2048_R2.xx_survey-1.fits<br />
| <br />
| <br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_217_2048_R2.xx_survey-2.fits<br />
| <br />
| <br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_217_2048_R2.xx_survey-3.fits<br />
| <br />
|<br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_217_2048_R2.xx_survey-4.fits<br />
| <br />
|<br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_353_2048_R2.xx_survey-1.fits<br />
| <br />
| <br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_353_2048_R2.xx_survey-2.fits<br />
| <br />
|<br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_353_2048_R2.xx_survey-3.fits<br />
| <br />
| <br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_353_2048_R2.xx_survey-4.fits<br />
| <br />
| <br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_545_2048_R2.xx_survey-1.fits<br />
| <br />
| <br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_545_2048_R2.xx_survey-2.fits<br />
| <br />
|<br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_545_2048_R2.xx_survey-3.fits<br />
| <br />
| <br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_545_2048_R2.xx_survey-4.fits<br />
| <br />
| <br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_857_2048_R2.xx_survey-1.fits<br />
| <br />
| <br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_857_2048_R2.xx_survey-2.fits<br />
|<br />
| <br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_857_2048_R2.xx_survey-3.fits<br />
| <br />
| <br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_857_2048_R2.xx_survey-4.fits<br />
| <br />
| <br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="28" | <span style="color:Blue">1 year maps</span> <br />
1 year = 2 surveys<br />
<br />
y1=s1+s2<br />
<br />
y2=s3+s4<br />
<br />
y3=s5+s6<br />
<br />
y4=s7+s8<br />
| rowspan="16" align="center" | LFI<br />
| LFI_SkyMap_030_1024_R2.xx_year-1.fits<br />
| <br />
|<br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_030_1024_R2.xx_year-2.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_030_1024_R2.xx_year-3.fits<br />
| <br />
|<br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_030_1024_R2.xx_year-4.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_year-1.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_year-2.fits<br />
| <br />
| <br />
|00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_year-3.fits<br />
| <br />
|<br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_year-4.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_year-1.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_year-2.fits<br />
| <br />
|<br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_year-3.fits<br />
| <br />
|<br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_year-4.fits<br />
| <br />
| <br />
|00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_2048_R2.xx_year-1.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_2048_R2.xx_year-2.fits<br />
| <br />
|<br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_2048_R2.xx_year-3.fits<br />
| <br />
|<br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_2048_R2.xx_year-4.fits<br />
| <br />
| <br />
|00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| rowspan="12" align="center" | HFI<br />
| HFI_SkyMap_100_2048_R2.xx_year-1.fits<br />
| <br />
| <br />
| 00 <br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_100_2048_R2.xx_year-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_143_2048_R2.xx_year-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_143_2048_R2.xx_year-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_217_2048_R2.xx_year-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_217_2048_R2.xx_year-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_353_2048_R2.xx_year-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_353_2048_R2.xx_year-2.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_545_2048_R2.xx_year-1.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_545_2048_R2.xx_year-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_857_2048_R2.xx_year-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_857_2048_R2.xx_year-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="12" | <span style="color:Blue">Half mission maps</span><br />
| rowspan="12" align="center"| HFI<br />
| HFI_SkyMap_100_2048_R2.xx_halfmission-1.fits<br />
| <br />
| <br />
| 00 <br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_100_2048_R2.xx_halfmission-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_143_2048_R2.xx_halfmission-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_143_2048_R2.xx_halfmission-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_217_2048_R2.xx_halfmission-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_217_2048_R2.xx_halfmission-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_353_2048_R2.xx_halfmission-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_353_2048_R2.xx_halfmission-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_545_2048_R2.xx_halfmission-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_545_2048_R2.xx_halfmission-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_857_2048_R2.xx_halfmission-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_857_2048_R2.xx_halfmission-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="12" | <span style="color:Blue">Multi year maps</span><br />
| rowspan="12" align="center"| LFI<br />
| LFI_SkyMap_030_1024_R2.xx_year-1-2.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_030_1024_R2.xx_year-1-3.fits<br />
| <br />
| <br />
| 00<br />
| 21/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_030_1024_R2.xx_year-2-4.fits<br />
| <br />
| <br />
| 00<br />
| 21/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_030_1024_R2.xx_year-3-4.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_year-1-2.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_year-1-3.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_year-2-4.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_year-3-4.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_year-1-2.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_year-1-3.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_year-2-4.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_year-3-4.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="20" | Half-ring maps <br />
| rowspan="8" align="center" | LFI <br />
| LFI_SkyMap_030_1024_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
|00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_030_1024_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| rowspan="12" align="center" | HFI <br />
| HFI_SkyMap_100_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_100_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_143_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_143_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_217_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_217_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_353_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_353_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_545_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_545_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_857_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_857_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="10" | Frequency Maps <br />
| rowspan="4" align="center" | LFI <br />
| LFI_SkyMap_030_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| rowspan="6" align="center" | HFI <br />
| HFI_SkyMap_100_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_143_2048_R2.xx_full.fits<br />
| <br />
|<br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_217_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_353_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_545_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_857_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" | Zodi correction maps <br />
| align="center" | HFI <br />
| HFI_CorrMap_<Freq>-Zodi_2048_R2.xx_<Coverage>.fits<br />
| <br />
| <br />
| 00<br />
| 16/12/2014<br />
| style="background-color: green;" |<br />
|style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
|}<br />
<br />
=====Detector maps=====<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=950px<br />
|+ '''HFI detector maps/LFI radiometer maps'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" rowspan="40" | <span style="color:Blue">Full mission</span><br />
| rowspan="22" align="center" | LFI<br />
| LFI_SkyMap_030-27M_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_030-27S_1024_R2.xx_full.fits<br />
| <br />
| <br />
|00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_030-28M_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_030-28S_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_044-24M_1024_R2.xx_full.fits<br />
| <br />
|<br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_044-24S_1024_R2.xx_full.fits<br />
| <br />
|<br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_044-25M_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_044-25S_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_044-26M_1024_R2.xx_full.fits<br />
| <br />
|<br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_044-26S_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_070-18M_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_070-18S_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_070-19M_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_070-19S_1024_R2.xx_full.fits<br />
|<br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_070-20M_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_070-20S_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_070-21M_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_070-21S_1024_R2.xx_full.fits<br />
| <br />
| <br />
|00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_070-22M_1024_R2.xx_full.fits<br />
| <br />
|<br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_070-22S_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_070-23M_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_070-23S_1024_R2.xx_full.fits<br />
| <br />
| <br />
|00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| rowspan="18" align="center" | HFI<br />
| HFI_SkyMap_143-5_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_143-6_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_143-7_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_217-1_2048_R2.xx_full.fits<br />
| <br />
|<br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_217-2_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_217-3_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_217-4_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_353-1_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_353-2_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
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| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_353-1_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_353-2_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
|00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_353-2_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_353-7_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_353-7_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
|<br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_353-8_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_353-8_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_545-1_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_545-1_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_545-2_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_545-2_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_545-4_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_545-4_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_857-1_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
|00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_857-1_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_857-2_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_857-2_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_857-3_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
|00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_857-3_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_857-4_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_857-4_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|}<br />
<br />
=====Detector set maps=====<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=1050px<br />
|+ '''Detector set maps'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" rowspan="16" | <span style="color:Blue">Full mission</span><br />
| rowspan="8" align="center" | LFI<br />
| LFI_SkyMap_044-24_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| [[#note12|[12]]]<br />
|-<br />
| LFI_SkyMap_044-25-26_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| [[#note12|[12]]]<br />
|-<br />
| LFI_SkyMap_070-18-23_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note12|[12]]]<br />
|-<br />
| LFI_SkyMap_070-19-22_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note12|[12]]]<br />
|-<br />
| LFI_SkyMap_070-20-21_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note12|[12]]]<br />
|-<br />
| LFI_SkyMap_070-18-23_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note12|[12]]]<br />
|-<br />
| LFI_SkyMap_070-19-22_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note12|[12]]]<br />
|-<br />
| LFI_SkyMap_070-20-21_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note12|[12]]]<br />
|-<br />
| rowspan="8" align="center" | HFI<br />
| HFI_SkyMap_100-ds1_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_100-ds2_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_143-ds1_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_143-ds2_2048_R2.xx_full.fits<br />
| <br />
| <br />
|00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_217-ds1_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_217-ds2_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_353-ds1_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_353-ds2_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="26" | <span style="color:Blue">Half rings</span><br />
| rowspan="10" align="center" | LFI<br />
| LFI_SkyMap_044-24_1024_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044-24_1024_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044-25-26_1024_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044-25-26_1024_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070-18-23_1024_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
|00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070-18-23_1024_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070-19-22_1024_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070-19-22_1024_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070-20-21_1024_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070-20-21_1024_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| rowspan="16" align="center" | HFI<br />
| HFI_SkyMap_100-ds1_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
|<br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_100-ds1_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_100-ds2_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_100-ds2_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_143-ds1_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_143-ds1_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
|style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_143-ds2_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_143-ds2_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_217-ds1_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
|00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
|| HFI_SkyMap_217-ds1_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
|00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_217-ds2_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_217-ds2_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_353-ds1_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_353-ds1_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_353-ds2_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_353-ds2_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|}<br />
<br />
=====Low resolution maps=====<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=950px<br />
|+ '''Low resolution maps (with noise cov. mat.)'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" rowspan="2"|Low resolution maps (with noise cov. mat.)<br />
| align="center" | LFI<br />
| LFI_SkyMap_fff_0016_R2.xx_full.fits<br />
| <br />
| <br />
|00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| align="center" | HFI <br />
| HFI_SkyMap_fff_0016_R2.xx_full.fits<br />
| Not for PR2<br />
| <br />
| 01<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|}<br />
<br />
=====Correction maps=====<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=1300px<br />
|+ '''Correction maps'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" rowspan="1"| <span style="color:Red">A correction maps</span><br />
| rowspan="10" align="center" | LFI<br />
| <strike>LFI_CorrMap_030-ACorr_NSNS_R2.xx_full.fits</strike><br />
| <br />
| <br />
| <br />
| <br />
|<br />
| <br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="9"| <span style="color:Blue">Band pass correction<br>maps</span><br />
| LFI_CorrMap_030-BPassCorr_0256_R2.xx_full.fits<br />
| <br />
| <br />
|00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_CorrMap_044-BPassCorr_0256_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
| LFI_CorrMap_070-BPassCorr_0256_R2.xx_full.fits<br />
| <br />
| <br />
|00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_CorrMap_030-BPassCorr_0128_R2.xx_full.fits<br />
| <br />
| <br />
|00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_CorrMap_044-BPassCorr_0128_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
| LFI_CorrMap_070-BPassCorr_0128_R2.xx_full.fits<br />
| <br />
| <br />
|00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_CorrMap_030-BPassCorr_0064_R2.xx_full.fits<br />
| <br />
| <br />
|00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_CorrMap_044-BPassCorr_0064_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
| LFI_CorrMap_070-BPassCorr_0064_R2.xx_full.fits<br />
| <br />
| <br />
|00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="12"| <span style="color:Blue">Dust correction<br>maps</span><br />
| rowspan="12" align="center" |HFI <br />
| HFI_CorrMap 353 GHz leakage global fits maps<br />
| <br />
| <br />
| 00<br />
| 09/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| <strike>HFI_CorrMap_100-dustleak-ground_2048_R2.xx_full.fits</strike><br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
|<br />
|-<br />
| <strike>HFI_CorrMap_353-dustleak-diff_2048_R2.xx_full.fits</strike><br />
| <br />
| <br />
| <br />
| <br />
|<br />
| <br />
| <br />
| <br />
|-<br />
| HFI_CorrMap_353-dustleak-ground_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
|24/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| <strike>HFI_CorrMap_353_dustleak-diff_2048_R2.xx_year-1.fits</strike><br />
| <br />
| <br />
| <br />
|<br />
| <br />
| <br />
| <br />
| <br />
|-<br />
| <strike>HFI_CorrMap_353_dustleak-diff_2048_R2.xx_year-2.fits</strike><br />
| <br />
| <br />
| <br />
| <br />
|<br />
| <br />
| <br />
| <br />
|-<br />
| HFI_CorrMap_353_dustleak-ground_2048_R2.xx_year-1.fits<br />
| <br />
| <br />
| 00<br />
| 24/11/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_CorrMap_353_dustleak-ground_2048_R2.xx_year-2.fits<br />
| <br />
| <br />
| 00<br />
| 24/11/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| <strike>HFI_CorrMap_353-ds1-dustleak-diff_2048_R2.xx_full.fits</strike><br />
| <br />
|<br />
| <br />
| <br />
| <br />
| <br />
| <br />
|<br />
|-<br />
| <strike>HFI_CorrMap_353-ds2-dustleak-diff_2048_R2.xx_full.fits</strike><br />
| <br />
| <br />
| <br />
|<br />
| <br />
| <br />
| <br />
| <br />
|-<br />
| HFI_CorrMap_353-ds1-dustleak-ground_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 24/11/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_CorrMap_353-ds2-dustleak-ground_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 24/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="1"| <span style="color:Blue">CO correction<br>maps</span><br />
| rowspan="1" align="center" | HFI <br />
| <strike>HFI_CorrMap_<freq>-coleak-'''METHOD1'''_2048_R2.xx_full.fits</strike><br />
| <br />
| <br />
| <br />
| <br />
|<br />
| <br />
| <br />
| <br />
|}<br />
<br />
====Covariance matrices====<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=850px<br />
|+ '''Covariance matrices'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" rowspan="4"| Cov. Matrices<br />
| style="text-align:center" rowspan="4"| HFI+LFI<br />
| LFI_NoiseCovMat_030_0016_R2.xx.tgz<br />
| <br />
| <br />
|00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| LFI_NoiseCovMat_044_0016_R2.xx.tgz<br />
| <br />
| <br />
| 00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_NoiseCovMat_070_0016_R2.xx.tgz<br />
| <br />
| <br />
| 00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI covariance matrices<br />
| Not for PR2<br />
| <br />
| 01<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|}<br />
<br />
====CMB maps====<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=1050px<br />
|+ '''CMB Maps'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" rowspan="6" | CMB anisotropy maps<br />
| rowspan="6" align="center" | COM<br />
| COM_CMB_IQU-nilc-field-X_Nside_R2.xx.fits<br />
| <br />
|<br />
|00 <br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_CMB_IQU-sevem-field-X_Nside_R2.xx.fits<br />
| <br />
| <br />
| 00<br />
|09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| COM_CMB_IQU-smica-field-X_Nside_R2.xx.fits<br />
| <br />
| <br />
| 00<br />
|09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_CMB_IQU-commander-field-X_Nside_R2.xx.fits<br />
| <br />
| <br />
| 00<br />
| 09/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| <strike>COM_CMB_IQU-commrul_0256_R2.xx.fits</strike><br />
| <br />
| <br />
| <br />
|<br />
| <br />
| <br />
| <br />
| <br />
|-<br />
| <span style="color:Red"><strike>Other representations</strike></span><br />
| <br />
| <br />
| <br />
|<br />
| <br />
| <br />
| <br />
| <br />
|-<br />
|}<br />
<br />
====Component maps====<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=950px<br />
|+ '''Component Maps'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" rowspan="3" | CO maps<br />
| align="center" rowspan="3"| HFI<br />
| HFI_CompMap_CO-Type1_2048_R2.xx.fits<br />
| <br />
|<br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_CompMap_CO-Type2_2048_R2.xx.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| <strike>HFI_CompMap_CO-Type3_2048_R2.xx.fits</strike><br />
| <br />
| <br />
| <br />
|<br />
| <br />
| <br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="12" | Commander foregrounds<br />
| align="center" rowspan="12"| COM<br />
| COM_CompMap_AME-commander_0256_R2.xx.fits<br />
|<br />
|<br />
| 00<br />
| 11/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| COM_CompMap_CMB-commander_0256_R2.xx.fits<br />
|<br />
|<br />
| 00<br />
| 11/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| COM_CompMap_CO21-commander_2048_R2.xx.fits<br />
|<br />
|<br />
| 00<br />
| 11/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| COM_CompMap_CO-commander_0256_R2.xx.fits<br />
|<br />
|<br />
| 00<br />
| 11/12/2014<br />
| style="background-color: green;" |<br />
|style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_CompMap_dust-commander_0256_R2.xx.fits<br />
|<br />
|<br />
| 00<br />
| 11/12/2014<br />
| style="background-color: green;" |<br />
|style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_CompMap_DustPol-commander_1024_R2.xx.fits<br />
|<br />
|<br />
| 00<br />
| 11/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_CompMap_freefree-commander_0256_R2.xx.fits<br />
|<br />
|<br />
| 00<br />
| 11/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| COM_CompMap_Synchrotron-commander_0256_R2.xx.fits<br />
|<br />
|<br />
| 00<br />
| 11/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| COM_CompMap_SynchrotronPol-commander_0256_R2.xx.fits<br />
|<br />
|<br />
| 00<br />
| 11/12/2014<br />
| style="background-color: green;" |<br />
|style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_CompMap_SZ-commander_0256_R2.xx.fits<br />
|<br />
|<br />
| 00<br />
| 11/12/2014<br />
| style="background-color: green;" |<br />
|style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_CompMap_ThermalDust-commander_2048_R2.xx.fits<br />
|<br />
|<br />
| 00<br />
| 11/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_CompMap_xline-commander_0256_R2.xx.fits<br />
|<br />
|<br />
| 00<br />
| 11/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" | Lensing maps<br />
| align="center" | COM<br />
| COM_CompMap_Lensing_2048_R2.xx.tar + SimMap tars<br />
|<br />
| <br />
|00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
|}<br />
<br />
====Masks====<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=850px<br />
|+ '''Masks'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" rowspan='4'| Masks<br />
| style="text-align:center" | <strike>LFI</strike><br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
|-<br />
| style="text-align:center" | HFI<br />
| HFI_Mask_GalPlane-apo 0 2 5 _2048_R2.xx.fits<br />
|<br />
| <br />
| 00<br />
| 19/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| style="text-align:center" rowspan='2'| COM<br />
| COM_CMB_IQU-common-field-MaskInt_2048_R2.xx.fits<br />
| <br />
|<br />
| 00<br />
| 10/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_CMB_IQU-common-field-MaskPol_1024_R2.xx.fits<br />
| <br />
| <br />
| 00<br />
| 10/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan='2'| Point source masks<br />
| style="text-align:center" rowspan='1'| LFI<br />
| LFI_Mask_PointSrc_2048_R2.xx.fits<br />
| <br />
| <br />
| 00<br />
|27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| style="text-align:center" | HFI<br />
| HFI_Mask_PointSrc_2048_R2.xx.fits<br />
| <br />
| <br />
|00<br />
| 19/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
|}<br />
<br />
===Angular power spectra===<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=1050px<br />
|+ '''Angular power spectra'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" rowspan="2" | CMB angular power spectra<br />
| style="text-align:center" rowspan="2" |COM<br />
| COM_PowerSpect_CMB_R2.xx.fits<br />
|<br />
| <br />
| 00<br />
| 05/02/2015<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| <strike>COM_PowerSpect_CMB_R2.xx.txt</strike><br />
|<br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="1"| <strike>Sky Angular power spectrum</strike><br />
| style="text-align:center" rowspan="4" |<br />
| <strike>LFI_PowerSpect_030_R2.xx.fits</strike><br />
|<br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
| [[#note37|[37]]]<br />
|-<br />
|}<br />
<div id="note37"></div>[37] For this release detector and detector set power spectra will not be provided. Instead the detector and detector set maps will be provided.<br />
<br />
===Characterisation===<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=850px<br />
|+ '''Characterization'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" rowspan="3"| RIMO<br />
| style="text-align:center" | LFI<br />
| LFI_RIMO_R2.xx.fits<br />
| <br />
| <br />
|50<br />
| 16/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| style="text-align:center" | HFI<br />
| HFI_RIMO_R2.xx.fits<br />
| <br />
| <br />
| 00<br />
| 20/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| style="text-align:center" | HFI<br />
| HFI beams RIMO(s)<br />
| <br />
| <br />
| 00<br />
| 05/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
|}<br />
<br />
===Catalogues===<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=850px<br />
|+ '''Catalogues'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" rowspan="9"| PCCS<br />
| style="text-align:center" rowspan="9"| COM<br />
| COM_PCCS_030_R2.xx.fits + excl.<br />
| <br />
| <br />
| 02<br />
|15/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_PCCS_044_R2.xx.fits + excl.<br />
| <br />
| <br />
| 02<br />
|15/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_PCCS_070_R2.xx.fits + excl.<br />
| <br />
| <br />
| 02<br />
| 15/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_PCCS_100_R2.xx.fits<br />
| <br />
| <br />
| 01<br />
| 19/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_PCCS_143_R2.xx.fits<br />
| <br />
| <br />
| 01<br />
| 19/11/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_PCCS_217_R2.xx.fits<br />
| <br />
| <br />
|01<br />
| 19/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_PCCS_353_R2.xx.fits<br />
| <br />
| <br />
| 01<br />
| 19/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_PCCS_545_R2.xx.fits<br />
| <br />
| <br />
| 01<br />
|19/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_PCCS_857_R2.xx.fits<br />
| <br />
| <br />
| 01<br />
|19/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="4"| SZ catalogues<br />
| style="text-align:center" rowspan="4"| COM<br />
| COM_PCCS_SZ-MMF1_R2.xx.fits<br />
| <br />
| <br />
| 08<br />
| 29/01/2015<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_PCCS_SZ-MMF3_R2.xx.fits<br />
| <br />
| <br />
| 08<br />
| 29/01/2015<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
|<br />
|-<br />
| COM_PCCS_SZ-PwS_R2.xx.fits<br />
| <br />
| <br />
| 08<br />
| 29/01/2015<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_PCCS_SZ-union_R2.xx.fits<br />
| <br />
| <br />
| 08<br />
| 03/02/2015<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
|<br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="4"| Other catalogues<br />
| style="text-align:center" rowspan="4"| HFI<br />
| <span style="color:Red"><strike>Dusty source catalogue</strike></span><br />
| <br />
| <br />
|<br />
| <br />
| <br />
| <br />
| <br />
| <br />
|-<br />
| <span style="color:Red"><strike>Radio sources catalogue</strike></span><br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
|-<br />
| <span style="color:Blue">HFI_PCCS_GCC_R2.xx.fits</span><br />
| <br />
| <br />
| 02<br />
| 16/01/2015<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| <span style="color:Blue">High-z catalogue</span><br />
| <br />
| <br />
| <br />
| <br />
|<br />
| <br />
| <br />
| <br />
|-<br />
|}<br />
<br />
===Other products===<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=850px<br />
|+ '''Other products'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" | Cosmological parameters<br />
| style="text-align:center" rowspan="1"| COM<br />
| Cosmological parameter tables<br />
| <br />
| <br />
| 00<br />
| 28/01/2015<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="1"| Codes<br />
| style="text-align:center" rowspan="1"| COM<br />
| Likelihood code<br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
|<br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="11"| Beams<br />
| style="text-align:center" rowspan="5"| <br />
| LFI scanning beams<br />
| <br />
| <br />
| 00<br />
| 21-11-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
| HFI scanning beams<br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
|<br />
| <br />
|-<br />
| Effective beams 30GHz<br />
| <br />
| <br />
| <br />
| 22-09-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
| Effective beams 44GHz<br />
| <br />
| <br />
| <br />
| 24-09-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
| Effective beams 70GHz<br />
| <br />
| <br />
| <br />
| 24-09-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
| style="text-align:center" rowspan="6"| <br />
| Effective beams 100 GHz<br />
| <br />
| <br />
| <br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
| Effective beams 143 GHz<br />
| <br />
| <br />
| <br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
| Effective beams 217 GHz<br />
| <br />
| <br />
| <br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
| Effective beams 353 GHz<br />
| <br />
| <br />
| <br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
| Effective beams 545 GHz<br />
| <br />
| <br />
| <br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
| Effective beams 857 GGz<br />
| <br />
| <br />
| <br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="2"| 4D maps<br />
| style="text-align:center" rowspan="2"| LFI<br />
| Code<br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
|<br />
| [[#noteA|[A]]]<br />
|-<br />
| map4D_calib_DDX11_LFIXX_gal_nsideXXX_npsiXXXX.fits<br />
| <br />
| <br />
| <br />
| 19/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| [[#noteA|[A]]]<br />
|-<br />
!bgcolor="ffdead" scope="row" | Datesobs<br />
| USPDC<br />
| HFI_DatesObs_<Freq>_2048_R2.xx_surveyX.fits.gz<br />
| <br />
| <br />
| 01<br />
|29/01/2015<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" | <br />
| <br />
| <br />
| <br />
| <br />
|<br />
| <br />
| <br />
| <br />
| <br />
| <br />
|-<br />
|}<br />
<div id="noteA"></div>[A] '''This is not an official product.'''</div>
Xdupac
https://wiki.cosmos.esa.int/planckpla2015/index.php?title=Product_Table_for_PLAv2&diff=11405
Product Table for PLAv2
2015-02-05T10:10:50Z
<p>Xdupac: /* Angular power spectra */</p>
<hr />
<div>{{DISPLAYTITLE:Products table for PLAv2}}<br />
==Product categories==<br />
*New products for this release that I believe have been confirmed appear in <span style="color:Blue">blue font</span>, products that are still TBC in <span style="color:Red">red font</span> (if it is one entire category of products I will just use color in the products category name, e.g. <span style="color:Blue">1 year maps</span>). Please check this in the tables and let me know whether there are any errors.<br />
*The Obs column contains links to notes at the end of each table. Please check the notes and let me know your feedback.<br />
*More general comments appear at the end of the numbered notes.<br />
<br />
I suggest you use the [[Talk:Product_Table_for_PLAv2|discussion page associated with this page]] to provide your feedback or make any comments relate to the list of products. The discussion page has the same structures in terms of sections as this page. Please try to write your comments/feedback in the appropriate section. I would also ask you to put your initials in the comments you write so that I can more easily get back to you to try to clarify any questions. Yes, it is true I can find out who wrote what in the history page but it makes my life easier if you associate your name to the comments you provide.<br />
<br />
The '''Description''' column will be used to add a one line description of the product that will appear in the archive as a tooltip associated with the product to allow a quick identification by users.<br />
===Time Series===<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=1050px<br />
|+ '''FITS filenames'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" rowspan="9" | <span style="color:Blue">Detector timeseries</span><br />
|rowspan="3" align="center" | LFI <br />
| LFI_TOI_030-SCI_R2.xx_ODXXXX.fits<br />
| <br />
| <br />
|00 <br />
| 10-09-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| LFI_TOI_044-SCI_R2.xx_ODXXXX.fits<br />
| <br />
| <br />
| 00<br />
| 10-09-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| LFI_TOI_070-SCI_R2.xx_ODXXXX.fits<br />
| <br />
| <br />
| 00<br />
| 10-09-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
|rowspan="6" align="center" | HFI <br />
| HFI_TOI_100-SCI_R2.xx_ODXXXX.fits<br />
| Only PSB: not for Feb. 2015 release<br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
|<br />
|-<br />
| HFI_TOI_143-SCI_R2.xx_ODXXXX.fits<br />
| without PSBs<br />
| <br />
| 00<br />
| 20/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_TOI_217-SCI_R2.xx_ODXXXX.fits<br />
| without PSBs<br />
| <br />
| 00<br />
| 20/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_TOI_353-SCI_R2.xx_ODXXXX.fits<br />
| with PSBs<br />
| <br />
| 00<br />
| 19/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_TOI_545-SCI_R2.xx_ODXXXX.fits<br />
| <br />
| <br />
| 00<br />
| 23/01/2015<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_TOI_857-SCI_R2.xx_ODXXXX.fits<br />
| <br />
| <br />
| 00<br />
| 23/01/2015<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="7" | <span style="color:Blue">Offsets</span><br />
| rowspan="6" align="center"| LFI <br />
| LFI_TOI_030-OFF_R2.xx_ODXXXX-full.fits<br />
| <br />
| <br />
| 00<br />
| 19-09-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_TOI_044-OFF_R2.xx_ODXXXX-full.fits<br />
| <br />
| <br />
| 00<br />
| 19-09-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_TOI_070-OFF_R2.xx_ODXXXX-full.fits<br />
| <br />
| <br />
|00<br />
| 19-09-2014 <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_TOI_030-OFF_R2.xx_ODXXXX-full-ringhalf.fits<br />
| <br />
| <br />
| 00<br />
| 11-11-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_TOI_044-OFF_R2.xx_ODXXXX-full-ringhalf.fits<br />
| <br />
| <br />
| 00<br />
| 11-11-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_TOI_070-OFF_R2.xx_ODXXXX-full-ringhalf.fits<br />
| <br />
| <br />
| 00<br />
| 11-11-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
|align="center"| HFI <br />
| HFI_TOI_AllFreqs-OFF_R2.xx.fits<br />
|<br />
|<br />
|00<br />
|13/01/2015<br />
|style="background-color: green;" |<br />
|style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan=9| <span style="color:Blue">Pointing</span><br />
| align="center" rowspan="3"| LFI <br />
| LFI_TOI_030-PTG_R2.xx_ODXXXX.fits <br />
|<br />
| <br />
|00 <br />
|18-07-2014 <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_TOI_044-PTG_R2.xx_ODXXXX.fits <br />
|<br />
| <br />
| 00 <br />
| 18-07-2014 <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_TOI_070-PTG_R2.xx_ODXXXX.fits <br />
|<br />
| <br />
| 00 <br />
| 18-07-2014 <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| rowspan=6 align="center"| HFI <br />
| HFI_TOI_100-PTG_R2.xx_ODXXXX.fits <br />
|<br />
| <br />
| 01 <br />
| 26-08-2014 <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_TOI_143-PTG_R2.xx_ODXXXX.fits <br />
|<br />
| <br />
| 01 <br />
| 26-08-2014 <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_TOI_217-PTG_R2.xx_ODXXXX.fits <br />
|<br />
| <br />
| 01 <br />
| 26-08-2014 <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_TOI_353-PTG_R2.xx_ODXXXX.fits <br />
|<br />
| <br />
| 01 <br />
| 26-08-2014 <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_TOI_545-PTG_R2.xx_ODXXXX.fits <br />
|<br />
| <br />
| 01 <br />
| 26-08-2014 <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_TOI_857-PTG_R2.xx_ODXXXX.fits <br />
|<br />
| <br />
| 01 <br />
| 26-08-2014 <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="4"| <span style="color:Blue">Time stamps</span><br />
| align="center" rowspan="3"| LFI <br />
| LFI_TOI_030-TAI_R2.xx_ODXXXX.fits <br />
|<br />
| <br />
|00 <br />
| 20-09-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_TOI_044-TAI_R2.xx_ODXXXX.fits <br />
|<br />
| <br />
| 00 <br />
| 20-09-2014 <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_TOI_070-TAI_R2.xx_ODXXXX.fits <br />
|<br />
| <br />
| 00<br />
| 20-09-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| align="center"| HFI <br />
| HFI_TOI_AllFreqs-TAI_R2.xx_ODXXXX.fits <br />
|<br />
| <br />
| 00<br />
| 20-09-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan=8| <span style="color:Blue">HK</span> <br />
|align="center" rowspan="8"| LFI <br />
| LFI_TOI_DAE-FAST-HK_R2.XX_ODXXX.fits<br />
| <br />
| <br />
|00 <br />
|14-08-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| LFI_TOI_DAE-SlowConfiguration-HK_R2.XX_ODXXXX.fits<br />
| <br />
| <br />
|00 <br />
|14-08-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| LFI_TOI_DAE-SlowCurrent-HK_R2.XX_ODXXXX.fits<br />
| <br />
| <br />
|00 <br />
|14-08-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| LFI_TOI_DAE-SlowPhaseSwitch-HK_R2.XX_ODXXXX.fits<br />
| <br />
| <br />
|00 <br />
|14-08-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" | <br />
| <br />
|<br />
|-<br />
| LFI_TOI_DAE-SlowVoltage-HK_R2.XX_ODXXXX.fits<br />
| <br />
| <br />
|00 <br />
|14-08-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" | <br />
| <br />
|<br />
|-<br />
| LFI_TOI_REBA-HK_R2.XX_ODXXXX.fits<br />
| <br />
| <br />
|00 <br />
|14-08-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" | <br />
| <br />
|<br />
|-<br />
| SCS_TOI_EssentialASW(R)-HK_R2.XX_ODXXXX.fits<br />
| <br />
| <br />
|00 <br />
|14-08-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" | <br />
| <br />
| <br />
|-<br />
| SCS_TOI_NonEssentialASW(R)-HK_R2.XX_ODXXXX.fits<br />
| <br />
| <br />
|00 <br />
|14-08-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" | <br />
| <br />
| <br />
|-<br />
|}<br />
<br />
===Maps===<br />
====Sky Maps====<br />
=====All detectors=====<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=1050px<br />
|+ '''All Detectors'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" rowspan="56" | Survey maps<br />
| rowspan="32" align="center"| LFI<br />
| LFI_SkyMap_030_1024_R2.xx_survey-1.fits<br />
| <br />
| <br />
| 01<br />
| 26/01/2015<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_030_1024_R2.xx_survey-2.fits<br />
| <br />
| <br />
| 01<br />
| <br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_030_1024_R2.xx_survey-3.fits<br />
| <br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_030_1024_R2.xx_survey-4.fits<br />
| <br />
| <br />
|01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_030_1024_R2.xx_survey-5.fits<br />
| <br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_030_1024_R2.xx_survey-6.fits<br />
| <br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_030_1024_R2.xx_survey-7.fits<br />
| <br />
|<br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_030_1024_R2.xx_survey-8.fits<br />
| <br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_survey-1.fits<br />
| <br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_survey-2.fits<br />
| <br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_survey-3.fits<br />
| <br />
|<br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_survey-4.fits<br />
|<br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_survey-5.fits<br />
| <br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_survey-6.fits<br />
| <br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_survey-7.fits<br />
| <br />
|<br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_survey-8.fits<br />
| <br />
|<br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_survey-1.fits<br />
|<br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_survey-2.fits<br />
| <br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_survey-3.fits<br />
| <br />
| <br />
|01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_survey-4.fits<br />
| <br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_survey-5.fits<br />
| <br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_survey-6.fits<br />
| <br />
|<br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_survey-7.fits<br />
| <br />
|<br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_survey-8.fits<br />
| <br />
|<br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_2048_R2.xx_survey-1.fits<br />
| <br />
|<br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_2048_R2.xx_survey-2.fits<br />
| <br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_2048_R2.xx_survey-3.fits<br />
| <br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_2048_R2.xx_survey-4.fits<br />
| <br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_2048_R2.xx_survey-5.fits<br />
| <br />
|<br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_2048_R2.xx_survey-6.fits<br />
|<br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_2048_R2.xx_survey-7.fits<br />
| <br />
| <br />
| 01<br />
|<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_2048_R2.xx_survey-8.fits<br />
| <br />
| <br />
| 01<br />
|<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| rowspan="24" align="center"| HFI<br />
| HFI_SkyMap_100_2048_R2.xx_survey-1.fits<br />
| <br />
|<br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_100_2048_R2.xx_survey-2.fits<br />
| <br />
|<br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_100_2048_R2.xx_survey-3.fits<br />
| <br />
|<br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_100_2048_R2.xx_survey-4.fits<br />
| <br />
| <br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_143_2048_R2.xx_survey-1.fits<br />
| <br />
| <br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_143_2048_R2.xx_survey-2.fits<br />
|<br />
| <br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_143_2048_R2.xx_survey-3.fits<br />
| <br />
| <br />
|00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_143_2048_R2.xx_survey-4.fits<br />
| <br />
|<br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_217_2048_R2.xx_survey-1.fits<br />
| <br />
| <br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_217_2048_R2.xx_survey-2.fits<br />
| <br />
| <br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_217_2048_R2.xx_survey-3.fits<br />
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| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
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| HFI_SkyMap_217_2048_R2.xx_survey-4.fits<br />
| <br />
|<br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_353_2048_R2.xx_survey-1.fits<br />
| <br />
| <br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_353_2048_R2.xx_survey-2.fits<br />
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| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
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|-<br />
| HFI_SkyMap_353_2048_R2.xx_survey-3.fits<br />
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| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
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| HFI_SkyMap_353_2048_R2.xx_survey-4.fits<br />
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| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
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|-<br />
| HFI_SkyMap_545_2048_R2.xx_survey-1.fits<br />
| <br />
| <br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
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| <br />
|-<br />
| HFI_SkyMap_545_2048_R2.xx_survey-2.fits<br />
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| 09/12/2014<br />
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| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_545_2048_R2.xx_survey-3.fits<br />
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| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_545_2048_R2.xx_survey-4.fits<br />
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| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_857_2048_R2.xx_survey-1.fits<br />
| <br />
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| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_857_2048_R2.xx_survey-2.fits<br />
|<br />
| <br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_857_2048_R2.xx_survey-3.fits<br />
| <br />
| <br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_857_2048_R2.xx_survey-4.fits<br />
| <br />
| <br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="28" | <span style="color:Blue">1 year maps</span> <br />
1 year = 2 surveys<br />
<br />
y1=s1+s2<br />
<br />
y2=s3+s4<br />
<br />
y3=s5+s6<br />
<br />
y4=s7+s8<br />
| rowspan="16" align="center" | LFI<br />
| LFI_SkyMap_030_1024_R2.xx_year-1.fits<br />
| <br />
|<br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_030_1024_R2.xx_year-2.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_030_1024_R2.xx_year-3.fits<br />
| <br />
|<br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_030_1024_R2.xx_year-4.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_year-1.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_year-2.fits<br />
| <br />
| <br />
|00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_year-3.fits<br />
| <br />
|<br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_year-4.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_year-1.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_year-2.fits<br />
| <br />
|<br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_year-3.fits<br />
| <br />
|<br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_year-4.fits<br />
| <br />
| <br />
|00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_2048_R2.xx_year-1.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_2048_R2.xx_year-2.fits<br />
| <br />
|<br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_2048_R2.xx_year-3.fits<br />
| <br />
|<br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_2048_R2.xx_year-4.fits<br />
| <br />
| <br />
|00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| rowspan="12" align="center" | HFI<br />
| HFI_SkyMap_100_2048_R2.xx_year-1.fits<br />
| <br />
| <br />
| 00 <br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_100_2048_R2.xx_year-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_143_2048_R2.xx_year-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_143_2048_R2.xx_year-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_217_2048_R2.xx_year-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_217_2048_R2.xx_year-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_353_2048_R2.xx_year-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_353_2048_R2.xx_year-2.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_545_2048_R2.xx_year-1.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_545_2048_R2.xx_year-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_857_2048_R2.xx_year-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_857_2048_R2.xx_year-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="12" | <span style="color:Blue">Half mission maps</span><br />
| rowspan="12" align="center"| HFI<br />
| HFI_SkyMap_100_2048_R2.xx_halfmission-1.fits<br />
| <br />
| <br />
| 00 <br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_100_2048_R2.xx_halfmission-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_143_2048_R2.xx_halfmission-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_143_2048_R2.xx_halfmission-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_217_2048_R2.xx_halfmission-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_217_2048_R2.xx_halfmission-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_353_2048_R2.xx_halfmission-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_353_2048_R2.xx_halfmission-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_545_2048_R2.xx_halfmission-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_545_2048_R2.xx_halfmission-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_857_2048_R2.xx_halfmission-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_857_2048_R2.xx_halfmission-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="12" | <span style="color:Blue">Multi year maps</span><br />
| rowspan="12" align="center"| LFI<br />
| LFI_SkyMap_030_1024_R2.xx_year-1-2.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_030_1024_R2.xx_year-1-3.fits<br />
| <br />
| <br />
| 00<br />
| 21/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_030_1024_R2.xx_year-2-4.fits<br />
| <br />
| <br />
| 00<br />
| 21/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_030_1024_R2.xx_year-3-4.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_year-1-2.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_year-1-3.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_year-2-4.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_year-3-4.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_year-1-2.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_year-1-3.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_year-2-4.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_year-3-4.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="20" | Half-ring maps <br />
| rowspan="8" align="center" | LFI <br />
| LFI_SkyMap_030_1024_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
|00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_030_1024_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| rowspan="12" align="center" | HFI <br />
| HFI_SkyMap_100_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_100_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_143_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_143_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_217_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_217_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_353_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_353_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_545_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_545_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_857_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_857_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="10" | Frequency Maps <br />
| rowspan="4" align="center" | LFI <br />
| LFI_SkyMap_030_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| rowspan="6" align="center" | HFI <br />
| HFI_SkyMap_100_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_143_2048_R2.xx_full.fits<br />
| <br />
|<br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_217_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_353_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_545_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_857_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" | Zodi correction maps <br />
| align="center" | HFI <br />
| HFI_CorrMap_<Freq>-Zodi_2048_R2.xx_<Coverage>.fits<br />
| <br />
| <br />
| 00<br />
| 16/12/2014<br />
| style="background-color: green;" |<br />
|style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
|}<br />
<br />
=====Detector maps=====<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=950px<br />
|+ '''HFI detector maps/LFI radiometer maps'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" rowspan="40" | <span style="color:Blue">Full mission</span><br />
| rowspan="22" align="center" | LFI<br />
| LFI_SkyMap_030-27M_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_030-27S_1024_R2.xx_full.fits<br />
| <br />
| <br />
|00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_030-28M_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_030-28S_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_044-24M_1024_R2.xx_full.fits<br />
| <br />
|<br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_044-24S_1024_R2.xx_full.fits<br />
| <br />
|<br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_044-25M_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_044-25S_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_044-26M_1024_R2.xx_full.fits<br />
| <br />
|<br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_044-26S_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_070-18M_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_070-18S_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_070-19M_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_070-19S_1024_R2.xx_full.fits<br />
|<br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_070-20M_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_070-20S_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_070-21M_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_070-21S_1024_R2.xx_full.fits<br />
| <br />
| <br />
|00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_070-22M_1024_R2.xx_full.fits<br />
| <br />
|<br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_070-22S_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_070-23M_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_070-23S_1024_R2.xx_full.fits<br />
| <br />
| <br />
|00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| rowspan="18" align="center" | HFI<br />
| HFI_SkyMap_143-5_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_143-6_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_143-7_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_217-1_2048_R2.xx_full.fits<br />
| <br />
|<br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_217-2_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_217-3_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_217-4_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_353-1_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_353-2_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_353-7_2048_R2.xx_full.fits<br />
| <br />
| <br />
|00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_353-8_2048_R2.xx_full.fits<br />
| <br />
|<br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_545-1_2048_R2.xx_full.fits<br />
| <br />
| <br />
|00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_545-2_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_545-4_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_857-1_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_857-2_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_857-3_2048_R2.xx_full.fits<br />
| <br />
|<br />
|00 <br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_857-4_2048_R2.xx_full.fits<br />
| <br />
| <br />
|00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="80" | <span style="color:Blue">Half rings</span><br />
| rowspan="44" align="center" | LFI<br />
| LFI_SkyMap_030-27M_1024_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_030-27M_1024_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_030-27S_1024_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
|00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_030-27S_1024_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
|00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_030-28M_1024_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_030-28M_1024_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_030-28S_1024_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_030-28S_1024_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_044-24M_1024_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
|style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_044-24M_1024_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_044-24S_1024_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_044-24S_1024_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
|00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_044-25M_1024_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_044-25M_1024_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_044-25S_1024_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
|00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
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| style="background-color: green;" |<br />
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| style="background-color: green;" |<br />
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| style="background-color: green;" |<br />
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| style="background-color: green;" |<br />
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| style="background-color: green;" |<br />
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| style="background-color: green;" |<br />
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|style="background-color: green;" |<br />
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| style="background-color: green;" |<br />
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|-<br />
| rowspan="36" align="center" | HFI<br />
| HFI_SkyMap_143-5_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
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| 00<br />
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| style="background-color: green;" |<br />
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| 00<br />
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| style="background-color: green;" |<br />
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|}<br />
<br />
=====Detector set maps=====<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=1050px<br />
|+ '''Detector set maps'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" rowspan="16" | <span style="color:Blue">Full mission</span><br />
| rowspan="8" align="center" | LFI<br />
| LFI_SkyMap_044-24_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| [[#note12|[12]]]<br />
|-<br />
| LFI_SkyMap_044-25-26_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| [[#note12|[12]]]<br />
|-<br />
| LFI_SkyMap_070-18-23_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note12|[12]]]<br />
|-<br />
| LFI_SkyMap_070-19-22_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note12|[12]]]<br />
|-<br />
| LFI_SkyMap_070-20-21_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note12|[12]]]<br />
|-<br />
| LFI_SkyMap_070-18-23_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note12|[12]]]<br />
|-<br />
| LFI_SkyMap_070-19-22_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note12|[12]]]<br />
|-<br />
| LFI_SkyMap_070-20-21_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note12|[12]]]<br />
|-<br />
| rowspan="8" align="center" | HFI<br />
| HFI_SkyMap_100-ds1_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_100-ds2_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_143-ds1_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_143-ds2_2048_R2.xx_full.fits<br />
| <br />
| <br />
|00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_217-ds1_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_217-ds2_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_353-ds1_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_353-ds2_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="26" | <span style="color:Blue">Half rings</span><br />
| rowspan="10" align="center" | LFI<br />
| LFI_SkyMap_044-24_1024_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044-24_1024_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044-25-26_1024_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044-25-26_1024_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070-18-23_1024_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
|00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070-18-23_1024_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070-19-22_1024_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070-19-22_1024_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070-20-21_1024_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070-20-21_1024_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| rowspan="16" align="center" | HFI<br />
| HFI_SkyMap_100-ds1_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
|<br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_100-ds1_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_100-ds2_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_100-ds2_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_143-ds1_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_143-ds1_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
|style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_143-ds2_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_143-ds2_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_217-ds1_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
|00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
|| HFI_SkyMap_217-ds1_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
|00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_217-ds2_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_217-ds2_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_353-ds1_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_353-ds1_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_353-ds2_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_353-ds2_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|}<br />
<br />
=====Low resolution maps=====<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=950px<br />
|+ '''Low resolution maps (with noise cov. mat.)'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" rowspan="2"|Low resolution maps (with noise cov. mat.)<br />
| align="center" | LFI<br />
| LFI_SkyMap_fff_0016_R2.xx_full.fits<br />
| <br />
| <br />
|00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| align="center" | HFI <br />
| HFI_SkyMap_fff_0016_R2.xx_full.fits<br />
| Not for PR2<br />
| <br />
| 01<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|}<br />
<br />
=====Correction maps=====<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=1300px<br />
|+ '''Correction maps'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" rowspan="1"| <span style="color:Red">A correction maps</span><br />
| rowspan="10" align="center" | LFI<br />
| <strike>LFI_CorrMap_030-ACorr_NSNS_R2.xx_full.fits</strike><br />
| <br />
| <br />
| <br />
| <br />
|<br />
| <br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="9"| <span style="color:Blue">Band pass correction<br>maps</span><br />
| LFI_CorrMap_030-BPassCorr_0256_R2.xx_full.fits<br />
| <br />
| <br />
|00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_CorrMap_044-BPassCorr_0256_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
| LFI_CorrMap_070-BPassCorr_0256_R2.xx_full.fits<br />
| <br />
| <br />
|00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_CorrMap_030-BPassCorr_0128_R2.xx_full.fits<br />
| <br />
| <br />
|00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_CorrMap_044-BPassCorr_0128_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
| LFI_CorrMap_070-BPassCorr_0128_R2.xx_full.fits<br />
| <br />
| <br />
|00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_CorrMap_030-BPassCorr_0064_R2.xx_full.fits<br />
| <br />
| <br />
|00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_CorrMap_044-BPassCorr_0064_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
| LFI_CorrMap_070-BPassCorr_0064_R2.xx_full.fits<br />
| <br />
| <br />
|00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="12"| <span style="color:Blue">Dust correction<br>maps</span><br />
| rowspan="12" align="center" |HFI <br />
| HFI_CorrMap 353 GHz leakage global fits maps<br />
| <br />
| <br />
| 00<br />
| 09/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| <strike>HFI_CorrMap_100-dustleak-ground_2048_R2.xx_full.fits</strike><br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
|<br />
|-<br />
| <strike>HFI_CorrMap_353-dustleak-diff_2048_R2.xx_full.fits</strike><br />
| <br />
| <br />
| <br />
| <br />
|<br />
| <br />
| <br />
| <br />
|-<br />
| HFI_CorrMap_353-dustleak-ground_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
|24/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| <strike>HFI_CorrMap_353_dustleak-diff_2048_R2.xx_year-1.fits</strike><br />
| <br />
| <br />
| <br />
|<br />
| <br />
| <br />
| <br />
| <br />
|-<br />
| <strike>HFI_CorrMap_353_dustleak-diff_2048_R2.xx_year-2.fits</strike><br />
| <br />
| <br />
| <br />
| <br />
|<br />
| <br />
| <br />
| <br />
|-<br />
| HFI_CorrMap_353_dustleak-ground_2048_R2.xx_year-1.fits<br />
| <br />
| <br />
| 00<br />
| 24/11/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_CorrMap_353_dustleak-ground_2048_R2.xx_year-2.fits<br />
| <br />
| <br />
| 00<br />
| 24/11/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| <strike>HFI_CorrMap_353-ds1-dustleak-diff_2048_R2.xx_full.fits</strike><br />
| <br />
|<br />
| <br />
| <br />
| <br />
| <br />
| <br />
|<br />
|-<br />
| <strike>HFI_CorrMap_353-ds2-dustleak-diff_2048_R2.xx_full.fits</strike><br />
| <br />
| <br />
| <br />
|<br />
| <br />
| <br />
| <br />
| <br />
|-<br />
| HFI_CorrMap_353-ds1-dustleak-ground_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 24/11/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_CorrMap_353-ds2-dustleak-ground_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 24/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="1"| <span style="color:Blue">CO correction<br>maps</span><br />
| rowspan="1" align="center" | HFI <br />
| <strike>HFI_CorrMap_<freq>-coleak-'''METHOD1'''_2048_R2.xx_full.fits</strike><br />
| <br />
| <br />
| <br />
| <br />
|<br />
| <br />
| <br />
| <br />
|}<br />
<br />
====Covariance matrices====<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=850px<br />
|+ '''Covariance matrices'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" rowspan="4"| Cov. Matrices<br />
| style="text-align:center" rowspan="4"| HFI+LFI<br />
| LFI_NoiseCovMat_030_0016_R2.xx.tgz<br />
| <br />
| <br />
|00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| LFI_NoiseCovMat_044_0016_R2.xx.tgz<br />
| <br />
| <br />
| 00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_NoiseCovMat_070_0016_R2.xx.tgz<br />
| <br />
| <br />
| 00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI covariance matrices<br />
| Not for PR2<br />
| <br />
| 01<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|}<br />
<br />
====CMB maps====<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=1050px<br />
|+ '''CMB Maps'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" rowspan="6" | CMB anisotropy maps<br />
| rowspan="6" align="center" | COM<br />
| COM_CMB_IQU-nilc-field-X_Nside_R2.xx.fits<br />
| <br />
|<br />
|00 <br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_CMB_IQU-sevem-field-X_Nside_R2.xx.fits<br />
| <br />
| <br />
| 00<br />
|09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| COM_CMB_IQU-smica-field-X_Nside_R2.xx.fits<br />
| <br />
| <br />
| 00<br />
|09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_CMB_IQU-commander-field-X_Nside_R2.xx.fits<br />
| <br />
| <br />
| 00<br />
| 09/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| <strike>COM_CMB_IQU-commrul_0256_R2.xx.fits</strike><br />
| <br />
| <br />
| <br />
|<br />
| <br />
| <br />
| <br />
| <br />
|-<br />
| <span style="color:Red"><strike>Other representations</strike></span><br />
| <br />
| <br />
| <br />
|<br />
| <br />
| <br />
| <br />
| <br />
|-<br />
|}<br />
<br />
====Component maps====<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=950px<br />
|+ '''Component Maps'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" rowspan="3" | CO maps<br />
| align="center" rowspan="3"| HFI<br />
| HFI_CompMap_CO-Type1_2048_R2.xx.fits<br />
| <br />
|<br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_CompMap_CO-Type2_2048_R2.xx.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| <strike>HFI_CompMap_CO-Type3_2048_R2.xx.fits</strike><br />
| <br />
| <br />
| <br />
|<br />
| <br />
| <br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="12" | Commander foregrounds<br />
| align="center" rowspan="12"| COM<br />
| COM_CompMap_AME-commander_0256_R2.xx.fits<br />
|<br />
|<br />
| 00<br />
| 11/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| COM_CompMap_CMB-commander_0256_R2.xx.fits<br />
|<br />
|<br />
| 00<br />
| 11/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| COM_CompMap_CO21-commander_2048_R2.xx.fits<br />
|<br />
|<br />
| 00<br />
| 11/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| COM_CompMap_CO-commander_0256_R2.xx.fits<br />
|<br />
|<br />
| 00<br />
| 11/12/2014<br />
| style="background-color: green;" |<br />
|style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_CompMap_dust-commander_0256_R2.xx.fits<br />
|<br />
|<br />
| 00<br />
| 11/12/2014<br />
| style="background-color: green;" |<br />
|style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_CompMap_DustPol-commander_1024_R2.xx.fits<br />
|<br />
|<br />
| 00<br />
| 11/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_CompMap_freefree-commander_0256_R2.xx.fits<br />
|<br />
|<br />
| 00<br />
| 11/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| COM_CompMap_Synchrotron-commander_0256_R2.xx.fits<br />
|<br />
|<br />
| 00<br />
| 11/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| COM_CompMap_SynchrotronPol-commander_0256_R2.xx.fits<br />
|<br />
|<br />
| 00<br />
| 11/12/2014<br />
| style="background-color: green;" |<br />
|style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_CompMap_SZ-commander_0256_R2.xx.fits<br />
|<br />
|<br />
| 00<br />
| 11/12/2014<br />
| style="background-color: green;" |<br />
|style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_CompMap_ThermalDust-commander_2048_R2.xx.fits<br />
|<br />
|<br />
| 00<br />
| 11/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_CompMap_xline-commander_0256_R2.xx.fits<br />
|<br />
|<br />
| 00<br />
| 11/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" | Lensing maps<br />
| align="center" | COM<br />
| COM_CompMap_Lensing_2048_R2.xx.tar + SimMap tars<br />
|<br />
| <br />
|00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
|}<br />
<br />
====Masks====<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=850px<br />
|+ '''Masks'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" rowspan='4'| Masks<br />
| style="text-align:center" | <strike>LFI</strike><br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
|-<br />
| style="text-align:center" | HFI<br />
| HFI_Mask_GalPlane-apo 0 2 5 _2048_R2.xx.fits<br />
|<br />
| <br />
| 00<br />
| 19/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| style="text-align:center" rowspan='2'| COM<br />
| COM_CMB_IQU-common-field-MaskInt_2048_R2.xx.fits<br />
| <br />
|<br />
| 00<br />
| 10/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_CMB_IQU-common-field-MaskPol_1024_R2.xx.fits<br />
| <br />
| <br />
| 00<br />
| 10/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan='2'| Point source masks<br />
| style="text-align:center" rowspan='1'| LFI<br />
| LFI_Mask_PointSrc_2048_R2.xx.fits<br />
| <br />
| <br />
| 00<br />
|27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| style="text-align:center" | HFI<br />
| HFI_Mask_PointSrc_2048_R2.xx.fits<br />
| <br />
| <br />
|00<br />
| 19/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
|}<br />
<br />
===Angular power spectra===<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=1050px<br />
|+ '''Angular power spectra'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" rowspan="2" | CMB angular power spectra<br />
| style="text-align:center" rowspan="2" |COM<br />
| COM_PowerSpect_CMB_R2.xx.fits<br />
|<br />
| <br />
| 00<br />
| 05/02/2015<br />
| <br />
| <br />
| <br />
| <br />
|-<br />
| <strike>COM_PowerSpect_CMB_R2.xx.txt</strike><br />
|<br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="1"| <strike>Sky Angular power spectrum</strike><br />
| style="text-align:center" rowspan="4" |<br />
| <strike>LFI_PowerSpect_030_R2.xx.fits</strike><br />
|<br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
| [[#note37|[37]]]<br />
|-<br />
|}<br />
<div id="note37"></div>[37] For this release detector and detector set power spectra will not be provided. Instead the detector and detector set maps will be provided.<br />
<br />
===Characterisation===<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=850px<br />
|+ '''Characterization'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" rowspan="3"| RIMO<br />
| style="text-align:center" | LFI<br />
| LFI_RIMO_R2.xx.fits<br />
| <br />
| <br />
|50<br />
| 16/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| style="text-align:center" | HFI<br />
| HFI_RIMO_R2.xx.fits<br />
| <br />
| <br />
| 00<br />
| 20/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| style="text-align:center" | HFI<br />
| HFI beams RIMO(s)<br />
| <br />
| <br />
| 00<br />
| 05/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
|}<br />
<br />
===Catalogues===<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=850px<br />
|+ '''Catalogues'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" rowspan="9"| PCCS<br />
| style="text-align:center" rowspan="9"| COM<br />
| COM_PCCS_030_R2.xx.fits + excl.<br />
| <br />
| <br />
| 02<br />
|15/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_PCCS_044_R2.xx.fits + excl.<br />
| <br />
| <br />
| 02<br />
|15/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_PCCS_070_R2.xx.fits + excl.<br />
| <br />
| <br />
| 02<br />
| 15/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_PCCS_100_R2.xx.fits<br />
| <br />
| <br />
| 01<br />
| 19/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_PCCS_143_R2.xx.fits<br />
| <br />
| <br />
| 01<br />
| 19/11/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_PCCS_217_R2.xx.fits<br />
| <br />
| <br />
|01<br />
| 19/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_PCCS_353_R2.xx.fits<br />
| <br />
| <br />
| 01<br />
| 19/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_PCCS_545_R2.xx.fits<br />
| <br />
| <br />
| 01<br />
|19/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_PCCS_857_R2.xx.fits<br />
| <br />
| <br />
| 01<br />
|19/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="4"| SZ catalogues<br />
| style="text-align:center" rowspan="4"| COM<br />
| COM_PCCS_SZ-MMF1_R2.xx.fits<br />
| <br />
| <br />
| 08<br />
| 29/01/2015<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_PCCS_SZ-MMF3_R2.xx.fits<br />
| <br />
| <br />
| 08<br />
| 29/01/2015<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
|<br />
|-<br />
| COM_PCCS_SZ-PwS_R2.xx.fits<br />
| <br />
| <br />
| 08<br />
| 29/01/2015<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_PCCS_SZ-union_R2.xx.fits<br />
| <br />
| <br />
| 08<br />
| 03/02/2015<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
|<br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="4"| Other catalogues<br />
| style="text-align:center" rowspan="4"| HFI<br />
| <span style="color:Red"><strike>Dusty source catalogue</strike></span><br />
| <br />
| <br />
|<br />
| <br />
| <br />
| <br />
| <br />
| <br />
|-<br />
| <span style="color:Red"><strike>Radio sources catalogue</strike></span><br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
|-<br />
| <span style="color:Blue">HFI_PCCS_GCC_R2.xx.fits</span><br />
| <br />
| <br />
| 02<br />
| 16/01/2015<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| <span style="color:Blue">High-z catalogue</span><br />
| <br />
| <br />
| <br />
| <br />
|<br />
| <br />
| <br />
| <br />
|-<br />
|}<br />
<br />
===Other products===<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=850px<br />
|+ '''Other products'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" | Cosmological parameters<br />
| style="text-align:center" rowspan="1"| COM<br />
| Cosmological parameter tables<br />
| <br />
| <br />
| 00<br />
| 28/01/2015<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="1"| Codes<br />
| style="text-align:center" rowspan="1"| COM<br />
| Likelihood code<br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
|<br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="11"| Beams<br />
| style="text-align:center" rowspan="5"| <br />
| LFI scanning beams<br />
| <br />
| <br />
| 00<br />
| 21-11-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
| HFI scanning beams<br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
|<br />
| <br />
|-<br />
| Effective beams 30GHz<br />
| <br />
| <br />
| <br />
| 22-09-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
| Effective beams 44GHz<br />
| <br />
| <br />
| <br />
| 24-09-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
| Effective beams 70GHz<br />
| <br />
| <br />
| <br />
| 24-09-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
| style="text-align:center" rowspan="6"| <br />
| Effective beams 100 GHz<br />
| <br />
| <br />
| <br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
| Effective beams 143 GHz<br />
| <br />
| <br />
| <br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
| Effective beams 217 GHz<br />
| <br />
| <br />
| <br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
| Effective beams 353 GHz<br />
| <br />
| <br />
| <br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
| Effective beams 545 GHz<br />
| <br />
| <br />
| <br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
| Effective beams 857 GGz<br />
| <br />
| <br />
| <br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="2"| 4D maps<br />
| style="text-align:center" rowspan="2"| LFI<br />
| Code<br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
|<br />
| [[#noteA|[A]]]<br />
|-<br />
| map4D_calib_DDX11_LFIXX_gal_nsideXXX_npsiXXXX.fits<br />
| <br />
| <br />
| <br />
| 19/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| [[#noteA|[A]]]<br />
|-<br />
!bgcolor="ffdead" scope="row" | Datesobs<br />
| USPDC<br />
| HFI_DatesObs_<Freq>_2048_R2.xx_surveyX.fits.gz<br />
| <br />
| <br />
| 01<br />
|29/01/2015<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" | <br />
| <br />
| <br />
| <br />
| <br />
|<br />
| <br />
| <br />
| <br />
| <br />
| <br />
|-<br />
|}<br />
<div id="noteA"></div>[A] '''This is not an official product.'''</div>
Xdupac
https://wiki.cosmos.esa.int/planckpla2015/index.php?title=Product_Table_for_PLAv2&diff=11404
Product Table for PLAv2
2015-02-05T10:10:20Z
<p>Xdupac: /* Angular power spectra */</p>
<hr />
<div>{{DISPLAYTITLE:Products table for PLAv2}}<br />
==Product categories==<br />
*New products for this release that I believe have been confirmed appear in <span style="color:Blue">blue font</span>, products that are still TBC in <span style="color:Red">red font</span> (if it is one entire category of products I will just use color in the products category name, e.g. <span style="color:Blue">1 year maps</span>). Please check this in the tables and let me know whether there are any errors.<br />
*The Obs column contains links to notes at the end of each table. Please check the notes and let me know your feedback.<br />
*More general comments appear at the end of the numbered notes.<br />
<br />
I suggest you use the [[Talk:Product_Table_for_PLAv2|discussion page associated with this page]] to provide your feedback or make any comments relate to the list of products. The discussion page has the same structures in terms of sections as this page. Please try to write your comments/feedback in the appropriate section. I would also ask you to put your initials in the comments you write so that I can more easily get back to you to try to clarify any questions. Yes, it is true I can find out who wrote what in the history page but it makes my life easier if you associate your name to the comments you provide.<br />
<br />
The '''Description''' column will be used to add a one line description of the product that will appear in the archive as a tooltip associated with the product to allow a quick identification by users.<br />
===Time Series===<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=1050px<br />
|+ '''FITS filenames'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" rowspan="9" | <span style="color:Blue">Detector timeseries</span><br />
|rowspan="3" align="center" | LFI <br />
| LFI_TOI_030-SCI_R2.xx_ODXXXX.fits<br />
| <br />
| <br />
|00 <br />
| 10-09-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| LFI_TOI_044-SCI_R2.xx_ODXXXX.fits<br />
| <br />
| <br />
| 00<br />
| 10-09-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| LFI_TOI_070-SCI_R2.xx_ODXXXX.fits<br />
| <br />
| <br />
| 00<br />
| 10-09-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
|rowspan="6" align="center" | HFI <br />
| HFI_TOI_100-SCI_R2.xx_ODXXXX.fits<br />
| Only PSB: not for Feb. 2015 release<br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
|<br />
|-<br />
| HFI_TOI_143-SCI_R2.xx_ODXXXX.fits<br />
| without PSBs<br />
| <br />
| 00<br />
| 20/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_TOI_217-SCI_R2.xx_ODXXXX.fits<br />
| without PSBs<br />
| <br />
| 00<br />
| 20/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_TOI_353-SCI_R2.xx_ODXXXX.fits<br />
| with PSBs<br />
| <br />
| 00<br />
| 19/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_TOI_545-SCI_R2.xx_ODXXXX.fits<br />
| <br />
| <br />
| 00<br />
| 23/01/2015<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_TOI_857-SCI_R2.xx_ODXXXX.fits<br />
| <br />
| <br />
| 00<br />
| 23/01/2015<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="7" | <span style="color:Blue">Offsets</span><br />
| rowspan="6" align="center"| LFI <br />
| LFI_TOI_030-OFF_R2.xx_ODXXXX-full.fits<br />
| <br />
| <br />
| 00<br />
| 19-09-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_TOI_044-OFF_R2.xx_ODXXXX-full.fits<br />
| <br />
| <br />
| 00<br />
| 19-09-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_TOI_070-OFF_R2.xx_ODXXXX-full.fits<br />
| <br />
| <br />
|00<br />
| 19-09-2014 <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_TOI_030-OFF_R2.xx_ODXXXX-full-ringhalf.fits<br />
| <br />
| <br />
| 00<br />
| 11-11-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_TOI_044-OFF_R2.xx_ODXXXX-full-ringhalf.fits<br />
| <br />
| <br />
| 00<br />
| 11-11-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_TOI_070-OFF_R2.xx_ODXXXX-full-ringhalf.fits<br />
| <br />
| <br />
| 00<br />
| 11-11-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
|align="center"| HFI <br />
| HFI_TOI_AllFreqs-OFF_R2.xx.fits<br />
|<br />
|<br />
|00<br />
|13/01/2015<br />
|style="background-color: green;" |<br />
|style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan=9| <span style="color:Blue">Pointing</span><br />
| align="center" rowspan="3"| LFI <br />
| LFI_TOI_030-PTG_R2.xx_ODXXXX.fits <br />
|<br />
| <br />
|00 <br />
|18-07-2014 <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_TOI_044-PTG_R2.xx_ODXXXX.fits <br />
|<br />
| <br />
| 00 <br />
| 18-07-2014 <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_TOI_070-PTG_R2.xx_ODXXXX.fits <br />
|<br />
| <br />
| 00 <br />
| 18-07-2014 <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| rowspan=6 align="center"| HFI <br />
| HFI_TOI_100-PTG_R2.xx_ODXXXX.fits <br />
|<br />
| <br />
| 01 <br />
| 26-08-2014 <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_TOI_143-PTG_R2.xx_ODXXXX.fits <br />
|<br />
| <br />
| 01 <br />
| 26-08-2014 <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_TOI_217-PTG_R2.xx_ODXXXX.fits <br />
|<br />
| <br />
| 01 <br />
| 26-08-2014 <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_TOI_353-PTG_R2.xx_ODXXXX.fits <br />
|<br />
| <br />
| 01 <br />
| 26-08-2014 <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_TOI_545-PTG_R2.xx_ODXXXX.fits <br />
|<br />
| <br />
| 01 <br />
| 26-08-2014 <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_TOI_857-PTG_R2.xx_ODXXXX.fits <br />
|<br />
| <br />
| 01 <br />
| 26-08-2014 <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="4"| <span style="color:Blue">Time stamps</span><br />
| align="center" rowspan="3"| LFI <br />
| LFI_TOI_030-TAI_R2.xx_ODXXXX.fits <br />
|<br />
| <br />
|00 <br />
| 20-09-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_TOI_044-TAI_R2.xx_ODXXXX.fits <br />
|<br />
| <br />
| 00 <br />
| 20-09-2014 <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_TOI_070-TAI_R2.xx_ODXXXX.fits <br />
|<br />
| <br />
| 00<br />
| 20-09-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| align="center"| HFI <br />
| HFI_TOI_AllFreqs-TAI_R2.xx_ODXXXX.fits <br />
|<br />
| <br />
| 00<br />
| 20-09-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan=8| <span style="color:Blue">HK</span> <br />
|align="center" rowspan="8"| LFI <br />
| LFI_TOI_DAE-FAST-HK_R2.XX_ODXXX.fits<br />
| <br />
| <br />
|00 <br />
|14-08-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| LFI_TOI_DAE-SlowConfiguration-HK_R2.XX_ODXXXX.fits<br />
| <br />
| <br />
|00 <br />
|14-08-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| LFI_TOI_DAE-SlowCurrent-HK_R2.XX_ODXXXX.fits<br />
| <br />
| <br />
|00 <br />
|14-08-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| LFI_TOI_DAE-SlowPhaseSwitch-HK_R2.XX_ODXXXX.fits<br />
| <br />
| <br />
|00 <br />
|14-08-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" | <br />
| <br />
|<br />
|-<br />
| LFI_TOI_DAE-SlowVoltage-HK_R2.XX_ODXXXX.fits<br />
| <br />
| <br />
|00 <br />
|14-08-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" | <br />
| <br />
|<br />
|-<br />
| LFI_TOI_REBA-HK_R2.XX_ODXXXX.fits<br />
| <br />
| <br />
|00 <br />
|14-08-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" | <br />
| <br />
|<br />
|-<br />
| SCS_TOI_EssentialASW(R)-HK_R2.XX_ODXXXX.fits<br />
| <br />
| <br />
|00 <br />
|14-08-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" | <br />
| <br />
| <br />
|-<br />
| SCS_TOI_NonEssentialASW(R)-HK_R2.XX_ODXXXX.fits<br />
| <br />
| <br />
|00 <br />
|14-08-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" | <br />
| <br />
| <br />
|-<br />
|}<br />
<br />
===Maps===<br />
====Sky Maps====<br />
=====All detectors=====<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=1050px<br />
|+ '''All Detectors'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" rowspan="56" | Survey maps<br />
| rowspan="32" align="center"| LFI<br />
| LFI_SkyMap_030_1024_R2.xx_survey-1.fits<br />
| <br />
| <br />
| 01<br />
| 26/01/2015<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_030_1024_R2.xx_survey-2.fits<br />
| <br />
| <br />
| 01<br />
| <br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_030_1024_R2.xx_survey-3.fits<br />
| <br />
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| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
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| LFI_SkyMap_030_1024_R2.xx_survey-4.fits<br />
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|01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
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| LFI_SkyMap_030_1024_R2.xx_survey-5.fits<br />
| <br />
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| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
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| LFI_SkyMap_030_1024_R2.xx_survey-6.fits<br />
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| 01<br />
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| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
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| LFI_SkyMap_030_1024_R2.xx_survey-7.fits<br />
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| style="background-color: green;" |<br />
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| LFI_SkyMap_044_1024_R2.xx_survey-1.fits<br />
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| style="background-color: green;" |<br />
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| LFI_SkyMap_044_1024_R2.xx_survey-5.fits<br />
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| style="background-color: green;" |<br />
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| LFI_SkyMap_044_1024_R2.xx_survey-6.fits<br />
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| 01<br />
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| style="background-color: green;" |<br />
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| LFI_SkyMap_044_1024_R2.xx_survey-7.fits<br />
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| 01<br />
| <br />
| style="background-color: green;" |<br />
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| LFI_SkyMap_044_1024_R2.xx_survey-8.fits<br />
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| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
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| LFI_SkyMap_070_1024_R2.xx_survey-1.fits<br />
|<br />
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| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
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|-<br />
| LFI_SkyMap_070_1024_R2.xx_survey-2.fits<br />
| <br />
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| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
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| LFI_SkyMap_070_1024_R2.xx_survey-3.fits<br />
| <br />
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|01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
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| LFI_SkyMap_070_1024_R2.xx_survey-4.fits<br />
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| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
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| LFI_SkyMap_070_1024_R2.xx_survey-5.fits<br />
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| 01<br />
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| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
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| LFI_SkyMap_070_1024_R2.xx_survey-6.fits<br />
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| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
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| LFI_SkyMap_070_1024_R2.xx_survey-7.fits<br />
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| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
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| LFI_SkyMap_070_1024_R2.xx_survey-8.fits<br />
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| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
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| LFI_SkyMap_070_2048_R2.xx_survey-1.fits<br />
| <br />
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| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
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| LFI_SkyMap_070_2048_R2.xx_survey-2.fits<br />
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| 01<br />
| <br />
| style="background-color: green;" |<br />
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| LFI_SkyMap_070_2048_R2.xx_survey-3.fits<br />
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| 01<br />
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| style="background-color: green;" |<br />
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| LFI_SkyMap_070_2048_R2.xx_survey-4.fits<br />
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| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
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|-<br />
| LFI_SkyMap_070_2048_R2.xx_survey-5.fits<br />
| <br />
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| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
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| LFI_SkyMap_070_2048_R2.xx_survey-6.fits<br />
|<br />
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| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
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|-<br />
| LFI_SkyMap_070_2048_R2.xx_survey-7.fits<br />
| <br />
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| 01<br />
|<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
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| LFI_SkyMap_070_2048_R2.xx_survey-8.fits<br />
| <br />
| <br />
| 01<br />
|<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| rowspan="24" align="center"| HFI<br />
| HFI_SkyMap_100_2048_R2.xx_survey-1.fits<br />
| <br />
|<br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_100_2048_R2.xx_survey-2.fits<br />
| <br />
|<br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
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| HFI_SkyMap_100_2048_R2.xx_survey-3.fits<br />
| <br />
|<br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
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| HFI_SkyMap_100_2048_R2.xx_survey-4.fits<br />
| <br />
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| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_143_2048_R2.xx_survey-1.fits<br />
| <br />
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| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
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| HFI_SkyMap_143_2048_R2.xx_survey-2.fits<br />
|<br />
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| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
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|-<br />
| HFI_SkyMap_143_2048_R2.xx_survey-3.fits<br />
| <br />
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| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
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| HFI_SkyMap_143_2048_R2.xx_survey-4.fits<br />
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| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
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| HFI_SkyMap_217_2048_R2.xx_survey-1.fits<br />
| <br />
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| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
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| HFI_SkyMap_217_2048_R2.xx_survey-2.fits<br />
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| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
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| HFI_SkyMap_217_2048_R2.xx_survey-3.fits<br />
| <br />
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| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
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|-<br />
| HFI_SkyMap_217_2048_R2.xx_survey-4.fits<br />
| <br />
|<br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_353_2048_R2.xx_survey-1.fits<br />
| <br />
| <br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_353_2048_R2.xx_survey-2.fits<br />
| <br />
|<br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_353_2048_R2.xx_survey-3.fits<br />
| <br />
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| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_353_2048_R2.xx_survey-4.fits<br />
| <br />
| <br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_545_2048_R2.xx_survey-1.fits<br />
| <br />
| <br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_545_2048_R2.xx_survey-2.fits<br />
| <br />
|<br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_545_2048_R2.xx_survey-3.fits<br />
| <br />
| <br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_545_2048_R2.xx_survey-4.fits<br />
| <br />
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| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_857_2048_R2.xx_survey-1.fits<br />
| <br />
| <br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
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| <br />
|-<br />
| HFI_SkyMap_857_2048_R2.xx_survey-2.fits<br />
|<br />
| <br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
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|-<br />
| HFI_SkyMap_857_2048_R2.xx_survey-3.fits<br />
| <br />
| <br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_857_2048_R2.xx_survey-4.fits<br />
| <br />
| <br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="28" | <span style="color:Blue">1 year maps</span> <br />
1 year = 2 surveys<br />
<br />
y1=s1+s2<br />
<br />
y2=s3+s4<br />
<br />
y3=s5+s6<br />
<br />
y4=s7+s8<br />
| rowspan="16" align="center" | LFI<br />
| LFI_SkyMap_030_1024_R2.xx_year-1.fits<br />
| <br />
|<br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_030_1024_R2.xx_year-2.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_030_1024_R2.xx_year-3.fits<br />
| <br />
|<br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_030_1024_R2.xx_year-4.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_year-1.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_year-2.fits<br />
| <br />
| <br />
|00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_year-3.fits<br />
| <br />
|<br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_year-4.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_year-1.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_year-2.fits<br />
| <br />
|<br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_year-3.fits<br />
| <br />
|<br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_year-4.fits<br />
| <br />
| <br />
|00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_2048_R2.xx_year-1.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_2048_R2.xx_year-2.fits<br />
| <br />
|<br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_2048_R2.xx_year-3.fits<br />
| <br />
|<br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_2048_R2.xx_year-4.fits<br />
| <br />
| <br />
|00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| rowspan="12" align="center" | HFI<br />
| HFI_SkyMap_100_2048_R2.xx_year-1.fits<br />
| <br />
| <br />
| 00 <br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_100_2048_R2.xx_year-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_143_2048_R2.xx_year-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_143_2048_R2.xx_year-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_217_2048_R2.xx_year-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_217_2048_R2.xx_year-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_353_2048_R2.xx_year-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_353_2048_R2.xx_year-2.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_545_2048_R2.xx_year-1.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_545_2048_R2.xx_year-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_857_2048_R2.xx_year-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_857_2048_R2.xx_year-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="12" | <span style="color:Blue">Half mission maps</span><br />
| rowspan="12" align="center"| HFI<br />
| HFI_SkyMap_100_2048_R2.xx_halfmission-1.fits<br />
| <br />
| <br />
| 00 <br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_100_2048_R2.xx_halfmission-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_143_2048_R2.xx_halfmission-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_143_2048_R2.xx_halfmission-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_217_2048_R2.xx_halfmission-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_217_2048_R2.xx_halfmission-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_353_2048_R2.xx_halfmission-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_353_2048_R2.xx_halfmission-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_545_2048_R2.xx_halfmission-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_545_2048_R2.xx_halfmission-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_857_2048_R2.xx_halfmission-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_857_2048_R2.xx_halfmission-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="12" | <span style="color:Blue">Multi year maps</span><br />
| rowspan="12" align="center"| LFI<br />
| LFI_SkyMap_030_1024_R2.xx_year-1-2.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_030_1024_R2.xx_year-1-3.fits<br />
| <br />
| <br />
| 00<br />
| 21/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_030_1024_R2.xx_year-2-4.fits<br />
| <br />
| <br />
| 00<br />
| 21/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_030_1024_R2.xx_year-3-4.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_year-1-2.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_year-1-3.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_year-2-4.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_year-3-4.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_year-1-2.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_year-1-3.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_year-2-4.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_year-3-4.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="20" | Half-ring maps <br />
| rowspan="8" align="center" | LFI <br />
| LFI_SkyMap_030_1024_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
|00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_030_1024_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| rowspan="12" align="center" | HFI <br />
| HFI_SkyMap_100_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_100_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_143_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_143_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_217_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_217_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_353_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_353_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_545_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_545_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_857_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_857_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="10" | Frequency Maps <br />
| rowspan="4" align="center" | LFI <br />
| LFI_SkyMap_030_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| rowspan="6" align="center" | HFI <br />
| HFI_SkyMap_100_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_143_2048_R2.xx_full.fits<br />
| <br />
|<br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_217_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_353_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_545_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_857_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" | Zodi correction maps <br />
| align="center" | HFI <br />
| HFI_CorrMap_<Freq>-Zodi_2048_R2.xx_<Coverage>.fits<br />
| <br />
| <br />
| 00<br />
| 16/12/2014<br />
| style="background-color: green;" |<br />
|style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
|}<br />
<br />
=====Detector maps=====<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=950px<br />
|+ '''HFI detector maps/LFI radiometer maps'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" rowspan="40" | <span style="color:Blue">Full mission</span><br />
| rowspan="22" align="center" | LFI<br />
| LFI_SkyMap_030-27M_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_030-27S_1024_R2.xx_full.fits<br />
| <br />
| <br />
|00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_030-28M_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_030-28S_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_044-24M_1024_R2.xx_full.fits<br />
| <br />
|<br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_044-24S_1024_R2.xx_full.fits<br />
| <br />
|<br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_044-25M_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_044-25S_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_044-26M_1024_R2.xx_full.fits<br />
| <br />
|<br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_044-26S_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_070-18M_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
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!bgcolor="ffdead" scope="row" rowspan="80" | <span style="color:Blue">Half rings</span><br />
| rowspan="44" align="center" | LFI<br />
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| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_070-23M_1024_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
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|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
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| [[#note9|[9]]]<br />
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| LFI_SkyMap_070-23M_1024_R2.xx_full-ringhalf-2.fits<br />
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|00<br />
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| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
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|-<br />
| LFI_SkyMap_070-23S_1024_R2.xx_full-ringhalf-1.fits<br />
| <br />
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|00<br />
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| style="background-color: green;" |<br />
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|-<br />
| LFI_SkyMap_070-23S_1024_R2.xx_full-ringhalf-2.fits<br />
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| 00<br />
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| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| rowspan="36" align="center" | HFI<br />
| HFI_SkyMap_143-5_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
|style="background-color: green;" |<br />
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| [[#note8|[8]]][[#note9|[9]]]<br />
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| HFI_SkyMap_143-5_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
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|style="background-color: green;" |<br />
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| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
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| HFI_SkyMap_143-6_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
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| style="background-color: green;" |<br />
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| HFI_SkyMap_143-6_2048_R2.xx_full-ringhalf-2.fits<br />
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| 00<br />
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|style="background-color: green;" |<br />
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| HFI_SkyMap_143-7_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
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| style="background-color: green;" |<br />
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|| HFI_SkyMap_143-7_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
|<br />
| 00 <br />
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| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_217-1_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
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| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
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| [[#note8|[8]]][[#note9|[9]]]<br />
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| HFI_SkyMap_217-1_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
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| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
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| 00<br />
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| style="background-color: green;" |<br />
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| [[#note8|[8]]][[#note9|[9]]]<br />
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| HFI_SkyMap_217-3_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
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|style="background-color: green;" |<br />
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| HFI_SkyMap_217-3_2048_R2.xx_full-ringhalf-2.fits<br />
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| 00<br />
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| style="background-color: green;" |<br />
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| HFI_SkyMap_217-4_2048_R2.xx_full-ringhalf-1.fits<br />
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| 00<br />
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| style="background-color: green;" |<br />
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| HFI_SkyMap_217-4_2048_R2.xx_full-ringhalf-2.fits<br />
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|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
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| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_353-1_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
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| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
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| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_353-1_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
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| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
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| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_353-2_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
|00<br />
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| style="background-color: green;" |<br />
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| [[#note8|[8]]][[#note9|[9]]]<br />
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| HFI_SkyMap_353-2_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
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| style="background-color: green;" |<br />
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| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_353-7_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
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| 00<br />
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|style="background-color: green;" |<br />
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| [[#note8|[8]]][[#note9|[9]]]<br />
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| HFI_SkyMap_353-7_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
|<br />
| 00<br />
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| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_353-8_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
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|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
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| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_353-8_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
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| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_545-1_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_545-1_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_545-2_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
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| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_545-2_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
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| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_545-4_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_545-4_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_857-1_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
|00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_857-1_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_857-2_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_857-2_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_857-3_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
|00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_857-3_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_857-4_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_857-4_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|}<br />
<br />
=====Detector set maps=====<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=1050px<br />
|+ '''Detector set maps'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" rowspan="16" | <span style="color:Blue">Full mission</span><br />
| rowspan="8" align="center" | LFI<br />
| LFI_SkyMap_044-24_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| [[#note12|[12]]]<br />
|-<br />
| LFI_SkyMap_044-25-26_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| [[#note12|[12]]]<br />
|-<br />
| LFI_SkyMap_070-18-23_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note12|[12]]]<br />
|-<br />
| LFI_SkyMap_070-19-22_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note12|[12]]]<br />
|-<br />
| LFI_SkyMap_070-20-21_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note12|[12]]]<br />
|-<br />
| LFI_SkyMap_070-18-23_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note12|[12]]]<br />
|-<br />
| LFI_SkyMap_070-19-22_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note12|[12]]]<br />
|-<br />
| LFI_SkyMap_070-20-21_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note12|[12]]]<br />
|-<br />
| rowspan="8" align="center" | HFI<br />
| HFI_SkyMap_100-ds1_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_100-ds2_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_143-ds1_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_143-ds2_2048_R2.xx_full.fits<br />
| <br />
| <br />
|00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_217-ds1_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_217-ds2_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_353-ds1_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_353-ds2_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="26" | <span style="color:Blue">Half rings</span><br />
| rowspan="10" align="center" | LFI<br />
| LFI_SkyMap_044-24_1024_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044-24_1024_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044-25-26_1024_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044-25-26_1024_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070-18-23_1024_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
|00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070-18-23_1024_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070-19-22_1024_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070-19-22_1024_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070-20-21_1024_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070-20-21_1024_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| rowspan="16" align="center" | HFI<br />
| HFI_SkyMap_100-ds1_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
|<br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_100-ds1_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_100-ds2_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_100-ds2_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_143-ds1_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_143-ds1_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
|style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_143-ds2_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_143-ds2_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_217-ds1_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
|00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
|| HFI_SkyMap_217-ds1_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
|00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_217-ds2_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_217-ds2_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_353-ds1_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_353-ds1_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_353-ds2_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_353-ds2_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|}<br />
<br />
=====Low resolution maps=====<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=950px<br />
|+ '''Low resolution maps (with noise cov. mat.)'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" rowspan="2"|Low resolution maps (with noise cov. mat.)<br />
| align="center" | LFI<br />
| LFI_SkyMap_fff_0016_R2.xx_full.fits<br />
| <br />
| <br />
|00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| align="center" | HFI <br />
| HFI_SkyMap_fff_0016_R2.xx_full.fits<br />
| Not for PR2<br />
| <br />
| 01<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|}<br />
<br />
=====Correction maps=====<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=1300px<br />
|+ '''Correction maps'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" rowspan="1"| <span style="color:Red">A correction maps</span><br />
| rowspan="10" align="center" | LFI<br />
| <strike>LFI_CorrMap_030-ACorr_NSNS_R2.xx_full.fits</strike><br />
| <br />
| <br />
| <br />
| <br />
|<br />
| <br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="9"| <span style="color:Blue">Band pass correction<br>maps</span><br />
| LFI_CorrMap_030-BPassCorr_0256_R2.xx_full.fits<br />
| <br />
| <br />
|00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_CorrMap_044-BPassCorr_0256_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
| LFI_CorrMap_070-BPassCorr_0256_R2.xx_full.fits<br />
| <br />
| <br />
|00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_CorrMap_030-BPassCorr_0128_R2.xx_full.fits<br />
| <br />
| <br />
|00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_CorrMap_044-BPassCorr_0128_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
| LFI_CorrMap_070-BPassCorr_0128_R2.xx_full.fits<br />
| <br />
| <br />
|00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_CorrMap_030-BPassCorr_0064_R2.xx_full.fits<br />
| <br />
| <br />
|00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_CorrMap_044-BPassCorr_0064_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
| LFI_CorrMap_070-BPassCorr_0064_R2.xx_full.fits<br />
| <br />
| <br />
|00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="12"| <span style="color:Blue">Dust correction<br>maps</span><br />
| rowspan="12" align="center" |HFI <br />
| HFI_CorrMap 353 GHz leakage global fits maps<br />
| <br />
| <br />
| 00<br />
| 09/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| <strike>HFI_CorrMap_100-dustleak-ground_2048_R2.xx_full.fits</strike><br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
|<br />
|-<br />
| <strike>HFI_CorrMap_353-dustleak-diff_2048_R2.xx_full.fits</strike><br />
| <br />
| <br />
| <br />
| <br />
|<br />
| <br />
| <br />
| <br />
|-<br />
| HFI_CorrMap_353-dustleak-ground_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
|24/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| <strike>HFI_CorrMap_353_dustleak-diff_2048_R2.xx_year-1.fits</strike><br />
| <br />
| <br />
| <br />
|<br />
| <br />
| <br />
| <br />
| <br />
|-<br />
| <strike>HFI_CorrMap_353_dustleak-diff_2048_R2.xx_year-2.fits</strike><br />
| <br />
| <br />
| <br />
| <br />
|<br />
| <br />
| <br />
| <br />
|-<br />
| HFI_CorrMap_353_dustleak-ground_2048_R2.xx_year-1.fits<br />
| <br />
| <br />
| 00<br />
| 24/11/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_CorrMap_353_dustleak-ground_2048_R2.xx_year-2.fits<br />
| <br />
| <br />
| 00<br />
| 24/11/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| <strike>HFI_CorrMap_353-ds1-dustleak-diff_2048_R2.xx_full.fits</strike><br />
| <br />
|<br />
| <br />
| <br />
| <br />
| <br />
| <br />
|<br />
|-<br />
| <strike>HFI_CorrMap_353-ds2-dustleak-diff_2048_R2.xx_full.fits</strike><br />
| <br />
| <br />
| <br />
|<br />
| <br />
| <br />
| <br />
| <br />
|-<br />
| HFI_CorrMap_353-ds1-dustleak-ground_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 24/11/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_CorrMap_353-ds2-dustleak-ground_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 24/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="1"| <span style="color:Blue">CO correction<br>maps</span><br />
| rowspan="1" align="center" | HFI <br />
| <strike>HFI_CorrMap_<freq>-coleak-'''METHOD1'''_2048_R2.xx_full.fits</strike><br />
| <br />
| <br />
| <br />
| <br />
|<br />
| <br />
| <br />
| <br />
|}<br />
<br />
====Covariance matrices====<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=850px<br />
|+ '''Covariance matrices'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" rowspan="4"| Cov. Matrices<br />
| style="text-align:center" rowspan="4"| HFI+LFI<br />
| LFI_NoiseCovMat_030_0016_R2.xx.tgz<br />
| <br />
| <br />
|00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| LFI_NoiseCovMat_044_0016_R2.xx.tgz<br />
| <br />
| <br />
| 00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_NoiseCovMat_070_0016_R2.xx.tgz<br />
| <br />
| <br />
| 00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI covariance matrices<br />
| Not for PR2<br />
| <br />
| 01<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|}<br />
<br />
====CMB maps====<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=1050px<br />
|+ '''CMB Maps'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" rowspan="6" | CMB anisotropy maps<br />
| rowspan="6" align="center" | COM<br />
| COM_CMB_IQU-nilc-field-X_Nside_R2.xx.fits<br />
| <br />
|<br />
|00 <br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_CMB_IQU-sevem-field-X_Nside_R2.xx.fits<br />
| <br />
| <br />
| 00<br />
|09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| COM_CMB_IQU-smica-field-X_Nside_R2.xx.fits<br />
| <br />
| <br />
| 00<br />
|09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_CMB_IQU-commander-field-X_Nside_R2.xx.fits<br />
| <br />
| <br />
| 00<br />
| 09/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| <strike>COM_CMB_IQU-commrul_0256_R2.xx.fits</strike><br />
| <br />
| <br />
| <br />
|<br />
| <br />
| <br />
| <br />
| <br />
|-<br />
| <span style="color:Red"><strike>Other representations</strike></span><br />
| <br />
| <br />
| <br />
|<br />
| <br />
| <br />
| <br />
| <br />
|-<br />
|}<br />
<br />
====Component maps====<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=950px<br />
|+ '''Component Maps'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" rowspan="3" | CO maps<br />
| align="center" rowspan="3"| HFI<br />
| HFI_CompMap_CO-Type1_2048_R2.xx.fits<br />
| <br />
|<br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_CompMap_CO-Type2_2048_R2.xx.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| <strike>HFI_CompMap_CO-Type3_2048_R2.xx.fits</strike><br />
| <br />
| <br />
| <br />
|<br />
| <br />
| <br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="12" | Commander foregrounds<br />
| align="center" rowspan="12"| COM<br />
| COM_CompMap_AME-commander_0256_R2.xx.fits<br />
|<br />
|<br />
| 00<br />
| 11/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| COM_CompMap_CMB-commander_0256_R2.xx.fits<br />
|<br />
|<br />
| 00<br />
| 11/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| COM_CompMap_CO21-commander_2048_R2.xx.fits<br />
|<br />
|<br />
| 00<br />
| 11/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| COM_CompMap_CO-commander_0256_R2.xx.fits<br />
|<br />
|<br />
| 00<br />
| 11/12/2014<br />
| style="background-color: green;" |<br />
|style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_CompMap_dust-commander_0256_R2.xx.fits<br />
|<br />
|<br />
| 00<br />
| 11/12/2014<br />
| style="background-color: green;" |<br />
|style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_CompMap_DustPol-commander_1024_R2.xx.fits<br />
|<br />
|<br />
| 00<br />
| 11/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_CompMap_freefree-commander_0256_R2.xx.fits<br />
|<br />
|<br />
| 00<br />
| 11/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| COM_CompMap_Synchrotron-commander_0256_R2.xx.fits<br />
|<br />
|<br />
| 00<br />
| 11/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| COM_CompMap_SynchrotronPol-commander_0256_R2.xx.fits<br />
|<br />
|<br />
| 00<br />
| 11/12/2014<br />
| style="background-color: green;" |<br />
|style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_CompMap_SZ-commander_0256_R2.xx.fits<br />
|<br />
|<br />
| 00<br />
| 11/12/2014<br />
| style="background-color: green;" |<br />
|style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_CompMap_ThermalDust-commander_2048_R2.xx.fits<br />
|<br />
|<br />
| 00<br />
| 11/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_CompMap_xline-commander_0256_R2.xx.fits<br />
|<br />
|<br />
| 00<br />
| 11/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" | Lensing maps<br />
| align="center" | COM<br />
| COM_CompMap_Lensing_2048_R2.xx.tar + SimMap tars<br />
|<br />
| <br />
|00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
|}<br />
<br />
====Masks====<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=850px<br />
|+ '''Masks'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" rowspan='4'| Masks<br />
| style="text-align:center" | <strike>LFI</strike><br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
|-<br />
| style="text-align:center" | HFI<br />
| HFI_Mask_GalPlane-apo 0 2 5 _2048_R2.xx.fits<br />
|<br />
| <br />
| 00<br />
| 19/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| style="text-align:center" rowspan='2'| COM<br />
| COM_CMB_IQU-common-field-MaskInt_2048_R2.xx.fits<br />
| <br />
|<br />
| 00<br />
| 10/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_CMB_IQU-common-field-MaskPol_1024_R2.xx.fits<br />
| <br />
| <br />
| 00<br />
| 10/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan='2'| Point source masks<br />
| style="text-align:center" rowspan='1'| LFI<br />
| LFI_Mask_PointSrc_2048_R2.xx.fits<br />
| <br />
| <br />
| 00<br />
|27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| style="text-align:center" | HFI<br />
| HFI_Mask_PointSrc_2048_R2.xx.fits<br />
| <br />
| <br />
|00<br />
| 19/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
|}<br />
<br />
===Angular power spectra===<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=1050px<br />
|+ '''Angular power spectra'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" rowspan="2" | CMB angular power spectra<br />
| style="text-align:center" rowspan="2" |COM<br />
| COM_PowerSpect_CMB_R2.xx.fits<br />
|<br />
| <br />
| 05/02/2015<br />
| 00<br />
| <br />
| <br />
| <br />
| <br />
|-<br />
| <strike>COM_PowerSpect_CMB_R2.xx.txt</strike><br />
|<br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="1"| <strike>Sky Angular power spectrum</strike><br />
| style="text-align:center" rowspan="4" |<br />
| <strike>LFI_PowerSpect_030_R2.xx.fits</strike><br />
|<br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
| [[#note37|[37]]]<br />
|-<br />
|}<br />
<div id="note37"></div>[37] For this release detector and detector set power spectra will not be provided. Instead the detector and detector set maps will be provided.<br />
<br />
===Characterisation===<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=850px<br />
|+ '''Characterization'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" rowspan="3"| RIMO<br />
| style="text-align:center" | LFI<br />
| LFI_RIMO_R2.xx.fits<br />
| <br />
| <br />
|50<br />
| 16/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| style="text-align:center" | HFI<br />
| HFI_RIMO_R2.xx.fits<br />
| <br />
| <br />
| 00<br />
| 20/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| style="text-align:center" | HFI<br />
| HFI beams RIMO(s)<br />
| <br />
| <br />
| 00<br />
| 05/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
|}<br />
<br />
===Catalogues===<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=850px<br />
|+ '''Catalogues'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" rowspan="9"| PCCS<br />
| style="text-align:center" rowspan="9"| COM<br />
| COM_PCCS_030_R2.xx.fits + excl.<br />
| <br />
| <br />
| 02<br />
|15/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_PCCS_044_R2.xx.fits + excl.<br />
| <br />
| <br />
| 02<br />
|15/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_PCCS_070_R2.xx.fits + excl.<br />
| <br />
| <br />
| 02<br />
| 15/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_PCCS_100_R2.xx.fits<br />
| <br />
| <br />
| 01<br />
| 19/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_PCCS_143_R2.xx.fits<br />
| <br />
| <br />
| 01<br />
| 19/11/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_PCCS_217_R2.xx.fits<br />
| <br />
| <br />
|01<br />
| 19/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_PCCS_353_R2.xx.fits<br />
| <br />
| <br />
| 01<br />
| 19/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_PCCS_545_R2.xx.fits<br />
| <br />
| <br />
| 01<br />
|19/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_PCCS_857_R2.xx.fits<br />
| <br />
| <br />
| 01<br />
|19/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="4"| SZ catalogues<br />
| style="text-align:center" rowspan="4"| COM<br />
| COM_PCCS_SZ-MMF1_R2.xx.fits<br />
| <br />
| <br />
| 08<br />
| 29/01/2015<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_PCCS_SZ-MMF3_R2.xx.fits<br />
| <br />
| <br />
| 08<br />
| 29/01/2015<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
|<br />
|-<br />
| COM_PCCS_SZ-PwS_R2.xx.fits<br />
| <br />
| <br />
| 08<br />
| 29/01/2015<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_PCCS_SZ-union_R2.xx.fits<br />
| <br />
| <br />
| 08<br />
| 03/02/2015<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
|<br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="4"| Other catalogues<br />
| style="text-align:center" rowspan="4"| HFI<br />
| <span style="color:Red"><strike>Dusty source catalogue</strike></span><br />
| <br />
| <br />
|<br />
| <br />
| <br />
| <br />
| <br />
| <br />
|-<br />
| <span style="color:Red"><strike>Radio sources catalogue</strike></span><br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
|-<br />
| <span style="color:Blue">HFI_PCCS_GCC_R2.xx.fits</span><br />
| <br />
| <br />
| 02<br />
| 16/01/2015<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| <span style="color:Blue">High-z catalogue</span><br />
| <br />
| <br />
| <br />
| <br />
|<br />
| <br />
| <br />
| <br />
|-<br />
|}<br />
<br />
===Other products===<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=850px<br />
|+ '''Other products'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" | Cosmological parameters<br />
| style="text-align:center" rowspan="1"| COM<br />
| Cosmological parameter tables<br />
| <br />
| <br />
| 00<br />
| 28/01/2015<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="1"| Codes<br />
| style="text-align:center" rowspan="1"| COM<br />
| Likelihood code<br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
|<br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="11"| Beams<br />
| style="text-align:center" rowspan="5"| <br />
| LFI scanning beams<br />
| <br />
| <br />
| 00<br />
| 21-11-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
| HFI scanning beams<br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
|<br />
| <br />
|-<br />
| Effective beams 30GHz<br />
| <br />
| <br />
| <br />
| 22-09-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
| Effective beams 44GHz<br />
| <br />
| <br />
| <br />
| 24-09-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
| Effective beams 70GHz<br />
| <br />
| <br />
| <br />
| 24-09-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
| style="text-align:center" rowspan="6"| <br />
| Effective beams 100 GHz<br />
| <br />
| <br />
| <br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
| Effective beams 143 GHz<br />
| <br />
| <br />
| <br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
| Effective beams 217 GHz<br />
| <br />
| <br />
| <br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
| Effective beams 353 GHz<br />
| <br />
| <br />
| <br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
| Effective beams 545 GHz<br />
| <br />
| <br />
| <br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
| Effective beams 857 GGz<br />
| <br />
| <br />
| <br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="2"| 4D maps<br />
| style="text-align:center" rowspan="2"| LFI<br />
| Code<br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
|<br />
| [[#noteA|[A]]]<br />
|-<br />
| map4D_calib_DDX11_LFIXX_gal_nsideXXX_npsiXXXX.fits<br />
| <br />
| <br />
| <br />
| 19/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| [[#noteA|[A]]]<br />
|-<br />
!bgcolor="ffdead" scope="row" | Datesobs<br />
| USPDC<br />
| HFI_DatesObs_<Freq>_2048_R2.xx_surveyX.fits.gz<br />
| <br />
| <br />
| 01<br />
|29/01/2015<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" | <br />
| <br />
| <br />
| <br />
| <br />
|<br />
| <br />
| <br />
| <br />
| <br />
| <br />
|-<br />
|}<br />
<div id="noteA"></div>[A] '''This is not an official product.'''</div>
Xdupac
https://wiki.cosmos.esa.int/planckpla2015/index.php?title=Main_Page&diff=11389
Main Page
2015-02-05T09:35:39Z
<p>Xdupac: </p>
<hr />
<div><!---'''<span style="font-size:180%"> <span style="color:Blue"> This is the Explanatory Supplement development page for the Planck 2015 data release </span><br />
<br />
<br />
<br />
* Instructions for new users: [[Help:READ ME FIRST|Read me first]]<br />
* See [http://meta.wikimedia.org/wiki/Help:Contents User's Guide] for a detailed User Guide of the MediaWiki software;<br />
* See [[Help:Contents|Explanatory Supplement Help page]] for Planck-specific guidelines.---><br />
<br />
==Explanatory Supplement for the 2015 data release ==<br />
<br />
By the [[Planck Collaboration]]<br />
<br />
The Explanatory Supplement is a reference text accompanying the public data delivered from the operations of the European Space Agency’s Planck satellite during its mission.<br />
*[[Questions and Answers|Q&A from PR1]]<br />
<!--- ############# ---><br />
#[[Introduction_WiP|Introduction]]<br />
##[[The Planck mission_WiP|The Planck mission]] <br />
##[[The satellite_WiP|The spacecraft]]<br />
##[[Ground Segment and Operations|Ground segment and operations]]<br />
##[[Survey_scanning_and_performance|Survey scanning and performance]]<br />
<!--- ############# ---><br />
#[[The Instruments_WiP|The Instruments]]<br />
##[[HFI design, qualification, and performance|HFI design, qualification, and performance]]<br />
###[[HFI_cryogenics | Cryogenics]]<br />
###[[HFI_cold_optics | Cold optics]]<br />
###[[HFI_detection_chain | Detection chain]]<br />
###[[HFI_operations | Operations]]<br />
###[[HFI_performance_summary | Performance summary]]<br />
###[[HFI_instrument_annexes | Annexes]]<br />
##[[LFI overview|LFI design, qualification, and performance]]<span style="color:red"></span><br />
###[[LFI design, qualification, and performance#LFIDescription| Instrument description]]<br />
###[[LFI design, qualification, and performance#LFITests| Ground tests]]<br />
###[[LFI design, qualification, and performance#LFICalibration| In-flight calibration]]<br />
###[[LFI design, qualification, and performance#LFIPerformance| Performance summary]]<br />
###[[LFI design, qualification, and performance#LFISystematics| Systematic effects]]<br />
###[[LFI design, qualification, and performance#SCS| Sorption cooler]]<br />
###[[LFIAppendix| Annexes]]<br />
<!--- ############# ---><br />
#[[Data processing]]<br />
##[[The HFI DPC| HFI Data Processing]]<br />
###[[Pre-processing | Pre-processing]]<br />
###[[TOI processing|TOI processing]]<br />
###[[ADC correction]]<br />
###[[Beams | Beams]]<br />
###[[Map-making | Mapmaking]]<br />
###[[Spectral response | Spectral response]]<br />
###[[HFI-Validation | Internal overall validation]]<br />
<!--- ###[[Power spectra | Power spectra]] <span style="color:red">Not ready for release</span> ---><br />
###[[Summary_of_HFI_data_characteristics | Summary of HFI data characteristics]]<br />
##[[The LFI DPC| LFI data processing]] <span style="color:red"></span><br />
###[[Pre-processing_LFI| Pre-processing]]<br />
###[[TOI processing_LFI| TOI processing]] <span style="color:red"></span><br />
###[[Beams_LFI | Beams]] <span style="color:red"></span><br />
###[[Galactic stray light removal]]<br />
###[[Map-making_LFI | Mapmaking]] <span style="color:red"></span><br />
###[[LFI systematic effect uncertainties | Systematic effects uncertainties]]<br />
###[[LFI-Validation | Internal overall validation]] <span style="color:red"></span><br />
<!--- ###[[L3_LFI | Power spectra]] ---><br />
###[[Summary_LFI | Summary of LFI data characteristics ]]<br />
##[[HFI/LFI joint data processing]]<br />
###[[Detector pointing| Detector pointing]]<br />
<!--- ###[[NoiseCovarMatrices | Noise covariance matrices and low-resolution maps ]] ---><br />
###[[Compact Source catalogues| Compact Source Catalogues]]<br />
###[[Astrophysical component separation]]<br />
###[[C2 | CMB Power spectra and Planck likelihood code]]<br />
<!--- ############# ---><br />
#[[Mission products]]<br />
##[[Timelines | Time-ordered data]]<br />
##[[Frequency Maps | Sky temperature and polarization maps]]<br />
<!--- ##[[NoiseCovariance | Noise covariance matrices and low-resolution maps ]]<span style="color:red">(Keskitalo)</span ---><br />
##[[The RIMO|Instrument model]] <br />
##[[Scanning Beams | Scanning Beams]]<br />
##[[Effective Beams | Effective beams]]<br />
##[[Catalogues|Catalogues]]: [[Catalogues#Catalogue of Compact Sources|PCCS]] • [[Catalogues#SZ Catalogue|PSZ]] • [[Catalogues#Catalogue_of_Planck_Galactic_Cold_Clumps|PGCC]]<br />
##[[CMB_and_astrophysical_component maps | CMB and astrophysical component maps]]<br />
##[[CMB spectrum & Likelihood Code | CMB spectrum ]]<br />
##[[Cosmological Parameters | Cosmological parameters and MC chains]]<br />
##[[Specially processed maps | Additional maps]]: [[Specially processed maps#Lensing map | Lensing map]] • [[Specially processed maps#Compton parameter map | Compton parameter map]] <br />
<!---##[[Scientific data used to generate Planck products | Scientific data used to generate Planck products]] <span style="color:red">Not ready for release</span>---><br />
<!---##[[Simulation data | Simulation data]] <span style="color:red">Not ready for release</span><br />
##[[DatesObs|Dates of observations]]---><br />
<!--- ############# ---><br />
#[[Software utilities|Software utilities]]<br />
##[[Unit conversion and Color correction|Unit conversion and Colour correction]] <br />
<!--- ############# ---><br />
#[[Operational data]]<br />
<!---##[[Thermal|Thermal and cooler system]]---><br />
##[[Survey history | Survey history data]]<br />
##[[Planck operational state history]]<br />
<!---##[[FOG|Fibre-optic gyro]]---><br />
##[[SREM|Space radiation environment monitor]]<br />
#[[Appendix]]<br />
##[[Glossary]]<br />
##[[List of acronyms]]<br />
[[Category:PSOBook]]</div>
Xdupac
https://wiki.cosmos.esa.int/planckpla2015/index.php?title=Main_Page&diff=11388
Main Page
2015-02-05T09:35:22Z
<p>Xdupac: </p>
<hr />
<div><br />
<br />
<!---'''<span style="font-size:180%"> <span style="color:Blue"> This is the Explanatory Supplement development page for the Planck 2015 data release </span><br />
<br />
<br />
<br />
* Instructions for new users: [[Help:READ ME FIRST|Read me first]]<br />
* See [http://meta.wikimedia.org/wiki/Help:Contents User's Guide] for a detailed User Guide of the MediaWiki software;<br />
* See [[Help:Contents|Explanatory Supplement Help page]] for Planck-specific guidelines.---><br />
<br />
<br />
==Explanatory Supplement for the 2015 data release ==<br />
<br />
By the [[Planck Collaboration]]<br />
<br />
The Explanatory Supplement is a reference text accompanying the public data delivered from the operations of the European Space Agency’s Planck satellite during its mission.<br />
*[[Questions and Answers|Q&A from PR1]]<br />
<!--- ############# ---><br />
#[[Introduction_WiP|Introduction]]<br />
##[[The Planck mission_WiP|The Planck mission]] <br />
##[[The satellite_WiP|The spacecraft]]<br />
##[[Ground Segment and Operations|Ground segment and operations]]<br />
##[[Survey_scanning_and_performance|Survey scanning and performance]]<br />
<!--- ############# ---><br />
#[[The Instruments_WiP|The Instruments]]<br />
##[[HFI design, qualification, and performance|HFI design, qualification, and performance]]<br />
###[[HFI_cryogenics | Cryogenics]]<br />
###[[HFI_cold_optics | Cold optics]]<br />
###[[HFI_detection_chain | Detection chain]]<br />
###[[HFI_operations | Operations]]<br />
###[[HFI_performance_summary | Performance summary]]<br />
###[[HFI_instrument_annexes | Annexes]]<br />
##[[LFI overview|LFI design, qualification, and performance]]<span style="color:red"></span><br />
###[[LFI design, qualification, and performance#LFIDescription| Instrument description]]<br />
###[[LFI design, qualification, and performance#LFITests| Ground tests]]<br />
###[[LFI design, qualification, and performance#LFICalibration| In-flight calibration]]<br />
###[[LFI design, qualification, and performance#LFIPerformance| Performance summary]]<br />
###[[LFI design, qualification, and performance#LFISystematics| Systematic effects]]<br />
###[[LFI design, qualification, and performance#SCS| Sorption cooler]]<br />
###[[LFIAppendix| Annexes]]<br />
<!--- ############# ---><br />
#[[Data processing]]<br />
##[[The HFI DPC| HFI Data Processing]]<br />
###[[Pre-processing | Pre-processing]]<br />
###[[TOI processing|TOI processing]]<br />
###[[ADC correction]]<br />
###[[Beams | Beams]]<br />
###[[Map-making | Mapmaking]]<br />
###[[Spectral response | Spectral response]]<br />
###[[HFI-Validation | Internal overall validation]]<br />
<!--- ###[[Power spectra | Power spectra]] <span style="color:red">Not ready for release</span> ---><br />
###[[Summary_of_HFI_data_characteristics | Summary of HFI data characteristics]]<br />
##[[The LFI DPC| LFI data processing]] <span style="color:red"></span><br />
###[[Pre-processing_LFI| Pre-processing]]<br />
###[[TOI processing_LFI| TOI processing]] <span style="color:red"></span><br />
###[[Beams_LFI | Beams]] <span style="color:red"></span><br />
###[[Galactic stray light removal]]<br />
###[[Map-making_LFI | Mapmaking]] <span style="color:red"></span><br />
###[[LFI systematic effect uncertainties | Systematic effects uncertainties]]<br />
###[[LFI-Validation | Internal overall validation]] <span style="color:red"></span><br />
<!--- ###[[L3_LFI | Power spectra]] ---><br />
###[[Summary_LFI | Summary of LFI data characteristics ]]<br />
##[[HFI/LFI joint data processing]]<br />
###[[Detector pointing| Detector pointing]]<br />
<!--- ###[[NoiseCovarMatrices | Noise covariance matrices and low-resolution maps ]] ---><br />
###[[Compact Source catalogues| Compact Source Catalogues]]<br />
###[[Astrophysical component separation]]<br />
###[[C2 | CMB Power spectra and Planck likelihood code]]<br />
<!--- ############# ---><br />
#[[Mission products]]<br />
##[[Timelines | Time-ordered data]]<br />
##[[Frequency Maps | Sky temperature and polarization maps]]<br />
<!--- ##[[NoiseCovariance | Noise covariance matrices and low-resolution maps ]]<span style="color:red">(Keskitalo)</span ---><br />
##[[The RIMO|Instrument model]] <br />
##[[Scanning Beams | Scanning Beams]]<br />
##[[Effective Beams | Effective beams]]<br />
##[[Catalogues|Catalogues]]: [[Catalogues#Catalogue of Compact Sources|PCCS]] • [[Catalogues#SZ Catalogue|PSZ]] • [[Catalogues#Catalogue_of_Planck_Galactic_Cold_Clumps|PGCC]]<br />
##[[CMB_and_astrophysical_component maps | CMB and astrophysical component maps]]<br />
##[[CMB spectrum & Likelihood Code | CMB spectrum ]]<br />
##[[Cosmological Parameters | Cosmological parameters and MC chains]]<br />
##[[Specially processed maps | Additional maps]]: [[Specially processed maps#Lensing map | Lensing map]] • [[Specially processed maps#Compton parameter map | Compton parameter map]] <br />
<!---##[[Scientific data used to generate Planck products | Scientific data used to generate Planck products]] <span style="color:red">Not ready for release</span>---><br />
<!---##[[Simulation data | Simulation data]] <span style="color:red">Not ready for release</span><br />
##[[DatesObs|Dates of observations]]---><br />
<!--- ############# ---><br />
#[[Software utilities|Software utilities]]<br />
##[[Unit conversion and Color correction|Unit conversion and Colour correction]] <br />
<!--- ############# ---><br />
#[[Operational data]]<br />
<!---##[[Thermal|Thermal and cooler system]]---><br />
##[[Survey history | Survey history data]]<br />
##[[Planck operational state history]]<br />
<!---##[[FOG|Fibre-optic gyro]]---><br />
##[[SREM|Space radiation environment monitor]]<br />
#[[Appendix]]<br />
##[[Glossary]]<br />
##[[List of acronyms]]<br />
[[Category:PSOBook]]</div>
Xdupac
https://wiki.cosmos.esa.int/planckpla2015/index.php?title=Main_Page&diff=11387
Main Page
2015-02-05T09:34:58Z
<p>Xdupac: </p>
<hr />
<div><br />
<br />
'''<span style="font-size:180%"> <span style="color:Blue"> This is the Explanatory Supplement development page for the Planck 2015 data release </span><br />
<br />
<br />
<br />
* Instructions for new users: [[Help:READ ME FIRST|Read me first]]<br />
* See [http://meta.wikimedia.org/wiki/Help:Contents User's Guide] for a detailed User Guide of the MediaWiki software;<br />
* See [[Help:Contents|Explanatory Supplement Help page]] for Planck-specific guidelines.<br />
<br />
<br />
==Explanatory Supplement for the 2015 data release ==<br />
<br />
By the [[Planck Collaboration]]<br />
<br />
The Explanatory Supplement is a reference text accompanying the public data delivered from the operations of the European Space Agency’s Planck satellite during its mission.<br />
*[[Questions and Answers|Q&A from PR1]]<br />
<!--- ############# ---><br />
#[[Introduction_WiP|Introduction]]<br />
##[[The Planck mission_WiP|The Planck mission]] <br />
##[[The satellite_WiP|The spacecraft]]<br />
##[[Ground Segment and Operations|Ground segment and operations]]<br />
##[[Survey_scanning_and_performance|Survey scanning and performance]]<br />
<!--- ############# ---><br />
#[[The Instruments_WiP|The Instruments]]<br />
##[[HFI design, qualification, and performance|HFI design, qualification, and performance]]<br />
###[[HFI_cryogenics | Cryogenics]]<br />
###[[HFI_cold_optics | Cold optics]]<br />
###[[HFI_detection_chain | Detection chain]]<br />
###[[HFI_operations | Operations]]<br />
###[[HFI_performance_summary | Performance summary]]<br />
###[[HFI_instrument_annexes | Annexes]]<br />
##[[LFI overview|LFI design, qualification, and performance]]<span style="color:red"></span><br />
###[[LFI design, qualification, and performance#LFIDescription| Instrument description]]<br />
###[[LFI design, qualification, and performance#LFITests| Ground tests]]<br />
###[[LFI design, qualification, and performance#LFICalibration| In-flight calibration]]<br />
###[[LFI design, qualification, and performance#LFIPerformance| Performance summary]]<br />
###[[LFI design, qualification, and performance#LFISystematics| Systematic effects]]<br />
###[[LFI design, qualification, and performance#SCS| Sorption cooler]]<br />
###[[LFIAppendix| Annexes]]<br />
<!--- ############# ---><br />
#[[Data processing]]<br />
##[[The HFI DPC| HFI Data Processing]]<br />
###[[Pre-processing | Pre-processing]]<br />
###[[TOI processing|TOI processing]]<br />
###[[ADC correction]]<br />
###[[Beams | Beams]]<br />
###[[Map-making | Mapmaking]]<br />
###[[Spectral response | Spectral response]]<br />
###[[HFI-Validation | Internal overall validation]]<br />
<!--- ###[[Power spectra | Power spectra]] <span style="color:red">Not ready for release</span> ---><br />
###[[Summary_of_HFI_data_characteristics | Summary of HFI data characteristics]]<br />
##[[The LFI DPC| LFI data processing]] <span style="color:red"></span><br />
###[[Pre-processing_LFI| Pre-processing]]<br />
###[[TOI processing_LFI| TOI processing]] <span style="color:red"></span><br />
###[[Beams_LFI | Beams]] <span style="color:red"></span><br />
###[[Galactic stray light removal]]<br />
###[[Map-making_LFI | Mapmaking]] <span style="color:red"></span><br />
###[[LFI systematic effect uncertainties | Systematic effects uncertainties]]<br />
###[[LFI-Validation | Internal overall validation]] <span style="color:red"></span><br />
<!--- ###[[L3_LFI | Power spectra]] ---><br />
###[[Summary_LFI | Summary of LFI data characteristics ]]<br />
##[[HFI/LFI joint data processing]]<br />
###[[Detector pointing| Detector pointing]]<br />
<!--- ###[[NoiseCovarMatrices | Noise covariance matrices and low-resolution maps ]] ---><br />
###[[Compact Source catalogues| Compact Source Catalogues]]<br />
###[[Astrophysical component separation]]<br />
###[[C2 | CMB Power spectra and Planck likelihood code]]<br />
<!--- ############# ---><br />
#[[Mission products]]<br />
##[[Timelines | Time-ordered data]]<br />
##[[Frequency Maps | Sky temperature and polarization maps]]<br />
<!--- ##[[NoiseCovariance | Noise covariance matrices and low-resolution maps ]]<span style="color:red">(Keskitalo)</span ---><br />
##[[The RIMO|Instrument model]] <br />
##[[Scanning Beams | Scanning Beams]]<br />
##[[Effective Beams | Effective beams]]<br />
##[[Catalogues|Catalogues]]: [[Catalogues#Catalogue of Compact Sources|PCCS]] • [[Catalogues#SZ Catalogue|PSZ]] • [[Catalogues#Catalogue_of_Planck_Galactic_Cold_Clumps|PGCC]]<br />
##[[CMB_and_astrophysical_component maps | CMB and astrophysical component maps]]<br />
##[[CMB spectrum & Likelihood Code | CMB spectrum ]]<br />
##[[Cosmological Parameters | Cosmological parameters and MC chains]]<br />
##[[Specially processed maps | Additional maps]]: [[Specially processed maps#Lensing map | Lensing map]] • [[Specially processed maps#Compton parameter map | Compton parameter map]] <br />
<!---##[[Scientific data used to generate Planck products | Scientific data used to generate Planck products]] <span style="color:red">Not ready for release</span>---><br />
<!---##[[Simulation data | Simulation data]] <span style="color:red">Not ready for release</span><br />
##[[DatesObs|Dates of observations]]---><br />
<!--- ############# ---><br />
#[[Software utilities|Software utilities]]<br />
##[[Unit conversion and Color correction|Unit conversion and Colour correction]] <br />
<!--- ############# ---><br />
#[[Operational data]]<br />
<!---##[[Thermal|Thermal and cooler system]]---><br />
##[[Survey history | Survey history data]]<br />
##[[Planck operational state history]]<br />
<!---##[[FOG|Fibre-optic gyro]]---><br />
##[[SREM|Space radiation environment monitor]]<br />
#[[Appendix]]<br />
##[[Glossary]]<br />
##[[List of acronyms]]<br />
[[Category:PSOBook]]</div>
Xdupac
https://wiki.cosmos.esa.int/planckpla2015/index.php?title=Main_Page&diff=11386
Main Page
2015-02-05T09:34:33Z
<p>Xdupac: /* Explanatory Supplement */</p>
<hr />
<div><br />
<br />
'''<span style="font-size:180%"> <span style="color:Blue"> This is the Explanatory Supplement development page for the Planck 2015 data release </span><br />
<br />
<br />
<br />
* Instructions for new users: [[Help:READ ME FIRST|Read me first]]<br />
* See [http://meta.wikimedia.org/wiki/Help:Contents User's Guide] for a detailed User Guide of the MediaWiki software;<br />
* See [[Help:Contents|Explanatory Supplement Help page]] for Planck-specific guidelines.<br />
<br />
<br />
==Explanatory Supplement ==<br />
<br />
By the [[Planck Collaboration]]<br />
<br />
The Explanatory Supplement is a reference text accompanying the public data delivered from the operations of the European Space Agency’s Planck satellite during its mission.<br />
*[[Questions and Answers|Q&A from PR1]]<br />
<!--- ############# ---><br />
#[[Introduction_WiP|Introduction]]<br />
##[[The Planck mission_WiP|The Planck mission]] <br />
##[[The satellite_WiP|The spacecraft]]<br />
##[[Ground Segment and Operations|Ground segment and operations]]<br />
##[[Survey_scanning_and_performance|Survey scanning and performance]]<br />
<!--- ############# ---><br />
#[[The Instruments_WiP|The Instruments]]<br />
##[[HFI design, qualification, and performance|HFI design, qualification, and performance]]<br />
###[[HFI_cryogenics | Cryogenics]]<br />
###[[HFI_cold_optics | Cold optics]]<br />
###[[HFI_detection_chain | Detection chain]]<br />
###[[HFI_operations | Operations]]<br />
###[[HFI_performance_summary | Performance summary]]<br />
###[[HFI_instrument_annexes | Annexes]]<br />
##[[LFI overview|LFI design, qualification, and performance]]<span style="color:red"></span><br />
###[[LFI design, qualification, and performance#LFIDescription| Instrument description]]<br />
###[[LFI design, qualification, and performance#LFITests| Ground tests]]<br />
###[[LFI design, qualification, and performance#LFICalibration| In-flight calibration]]<br />
###[[LFI design, qualification, and performance#LFIPerformance| Performance summary]]<br />
###[[LFI design, qualification, and performance#LFISystematics| Systematic effects]]<br />
###[[LFI design, qualification, and performance#SCS| Sorption cooler]]<br />
###[[LFIAppendix| Annexes]]<br />
<!--- ############# ---><br />
#[[Data processing]]<br />
##[[The HFI DPC| HFI Data Processing]]<br />
###[[Pre-processing | Pre-processing]]<br />
###[[TOI processing|TOI processing]]<br />
###[[ADC correction]]<br />
###[[Beams | Beams]]<br />
###[[Map-making | Mapmaking]]<br />
###[[Spectral response | Spectral response]]<br />
###[[HFI-Validation | Internal overall validation]]<br />
<!--- ###[[Power spectra | Power spectra]] <span style="color:red">Not ready for release</span> ---><br />
###[[Summary_of_HFI_data_characteristics | Summary of HFI data characteristics]]<br />
##[[The LFI DPC| LFI data processing]] <span style="color:red"></span><br />
###[[Pre-processing_LFI| Pre-processing]]<br />
###[[TOI processing_LFI| TOI processing]] <span style="color:red"></span><br />
###[[Beams_LFI | Beams]] <span style="color:red"></span><br />
###[[Galactic stray light removal]]<br />
###[[Map-making_LFI | Mapmaking]] <span style="color:red"></span><br />
###[[LFI systematic effect uncertainties | Systematic effects uncertainties]]<br />
###[[LFI-Validation | Internal overall validation]] <span style="color:red"></span><br />
<!--- ###[[L3_LFI | Power spectra]] ---><br />
###[[Summary_LFI | Summary of LFI data characteristics ]]<br />
##[[HFI/LFI joint data processing]]<br />
###[[Detector pointing| Detector pointing]]<br />
<!--- ###[[NoiseCovarMatrices | Noise covariance matrices and low-resolution maps ]] ---><br />
###[[Compact Source catalogues| Compact Source Catalogues]]<br />
###[[Astrophysical component separation]]<br />
###[[C2 | CMB Power spectra and Planck likelihood code]]<br />
<!--- ############# ---><br />
#[[Mission products]]<br />
##[[Timelines | Time-ordered data]]<br />
##[[Frequency Maps | Sky temperature and polarization maps]]<br />
<!--- ##[[NoiseCovariance | Noise covariance matrices and low-resolution maps ]]<span style="color:red">(Keskitalo)</span ---><br />
##[[The RIMO|Instrument model]] <br />
##[[Scanning Beams | Scanning Beams]]<br />
##[[Effective Beams | Effective beams]]<br />
##[[Catalogues|Catalogues]]: [[Catalogues#Catalogue of Compact Sources|PCCS]] • [[Catalogues#SZ Catalogue|PSZ]] • [[Catalogues#Catalogue_of_Planck_Galactic_Cold_Clumps|PGCC]]<br />
##[[CMB_and_astrophysical_component maps | CMB and astrophysical component maps]]<br />
##[[CMB spectrum & Likelihood Code | CMB spectrum ]]<br />
##[[Cosmological Parameters | Cosmological parameters and MC chains]]<br />
##[[Specially processed maps | Additional maps]]: [[Specially processed maps#Lensing map | Lensing map]] • [[Specially processed maps#Compton parameter map | Compton parameter map]] <br />
<!---##[[Scientific data used to generate Planck products | Scientific data used to generate Planck products]] <span style="color:red">Not ready for release</span>---><br />
<!---##[[Simulation data | Simulation data]] <span style="color:red">Not ready for release</span><br />
##[[DatesObs|Dates of observations]]---><br />
<!--- ############# ---><br />
#[[Software utilities|Software utilities]]<br />
##[[Unit conversion and Color correction|Unit conversion and Colour correction]] <br />
<!--- ############# ---><br />
#[[Operational data]]<br />
<!---##[[Thermal|Thermal and cooler system]]---><br />
##[[Survey history | Survey history data]]<br />
##[[Planck operational state history]]<br />
<!---##[[FOG|Fibre-optic gyro]]---><br />
##[[SREM|Space radiation environment monitor]]<br />
#[[Appendix]]<br />
##[[Glossary]]<br />
##[[List of acronyms]]<br />
[[Category:PSOBook]]</div>
Xdupac
https://wiki.cosmos.esa.int/planckpla2015/index.php?title=Main_Page&diff=11385
Main Page
2015-02-05T09:33:27Z
<p>Xdupac: </p>
<hr />
<div><br />
<br />
'''<span style="font-size:180%"> <span style="color:Blue"> This is the Explanatory Supplement development page for the Planck 2015 data release </span><br />
<br />
<br />
<br />
* Instructions for new users: [[Help:READ ME FIRST|Read me first]]<br />
* See [http://meta.wikimedia.org/wiki/Help:Contents User's Guide] for a detailed User Guide of the MediaWiki software;<br />
* See [[Help:Contents|Explanatory Supplement Help page]] for Planck-specific guidelines.<br />
<br />
<br />
== [[:Category:Explanatory Supplement|Explanatory Supplement]] ==<br />
<br />
By the [[Planck Collaboration]]<br />
<br />
The Explanatory Supplement is a reference text accompanying the public data delivered from the operations of the European Space Agency’s Planck satellite during its mission.<br />
*[[Questions and Answers|Q&A from PR1]]<br />
<!--- ############# ---><br />
#[[Introduction_WiP|Introduction]]<br />
##[[The Planck mission_WiP|The Planck mission]] <br />
##[[The satellite_WiP|The spacecraft]]<br />
##[[Ground Segment and Operations|Ground segment and operations]]<br />
##[[Survey_scanning_and_performance|Survey scanning and performance]]<br />
<!--- ############# ---><br />
#[[The Instruments_WiP|The Instruments]]<br />
##[[HFI design, qualification, and performance|HFI design, qualification, and performance]]<br />
###[[HFI_cryogenics | Cryogenics]]<br />
###[[HFI_cold_optics | Cold optics]]<br />
###[[HFI_detection_chain | Detection chain]]<br />
###[[HFI_operations | Operations]]<br />
###[[HFI_performance_summary | Performance summary]]<br />
###[[HFI_instrument_annexes | Annexes]]<br />
##[[LFI overview|LFI design, qualification, and performance]]<span style="color:red"></span><br />
###[[LFI design, qualification, and performance#LFIDescription| Instrument description]]<br />
###[[LFI design, qualification, and performance#LFITests| Ground tests]]<br />
###[[LFI design, qualification, and performance#LFICalibration| In-flight calibration]]<br />
###[[LFI design, qualification, and performance#LFIPerformance| Performance summary]]<br />
###[[LFI design, qualification, and performance#LFISystematics| Systematic effects]]<br />
###[[LFI design, qualification, and performance#SCS| Sorption cooler]]<br />
###[[LFIAppendix| Annexes]]<br />
<!--- ############# ---><br />
#[[Data processing]]<br />
##[[The HFI DPC| HFI Data Processing]]<br />
###[[Pre-processing | Pre-processing]]<br />
###[[TOI processing|TOI processing]]<br />
###[[ADC correction]]<br />
###[[Beams | Beams]]<br />
###[[Map-making | Mapmaking]]<br />
###[[Spectral response | Spectral response]]<br />
###[[HFI-Validation | Internal overall validation]]<br />
<!--- ###[[Power spectra | Power spectra]] <span style="color:red">Not ready for release</span> ---><br />
###[[Summary_of_HFI_data_characteristics | Summary of HFI data characteristics]]<br />
##[[The LFI DPC| LFI data processing]] <span style="color:red"></span><br />
###[[Pre-processing_LFI| Pre-processing]]<br />
###[[TOI processing_LFI| TOI processing]] <span style="color:red"></span><br />
###[[Beams_LFI | Beams]] <span style="color:red"></span><br />
###[[Galactic stray light removal]]<br />
###[[Map-making_LFI | Mapmaking]] <span style="color:red"></span><br />
###[[LFI systematic effect uncertainties | Systematic effects uncertainties]]<br />
###[[LFI-Validation | Internal overall validation]] <span style="color:red"></span><br />
<!--- ###[[L3_LFI | Power spectra]] ---><br />
###[[Summary_LFI | Summary of LFI data characteristics ]]<br />
##[[HFI/LFI joint data processing]]<br />
###[[Detector pointing| Detector pointing]]<br />
<!--- ###[[NoiseCovarMatrices | Noise covariance matrices and low-resolution maps ]] ---><br />
###[[Compact Source catalogues| Compact Source Catalogues]]<br />
###[[Astrophysical component separation]]<br />
###[[C2 | CMB Power spectra and Planck likelihood code]]<br />
<!--- ############# ---><br />
#[[Mission products]]<br />
##[[Timelines | Time-ordered data]]<br />
##[[Frequency Maps | Sky temperature and polarization maps]]<br />
<!--- ##[[NoiseCovariance | Noise covariance matrices and low-resolution maps ]]<span style="color:red">(Keskitalo)</span ---><br />
##[[The RIMO|Instrument model]] <br />
##[[Scanning Beams | Scanning Beams]]<br />
##[[Effective Beams | Effective beams]]<br />
##[[Catalogues|Catalogues]]: [[Catalogues#Catalogue of Compact Sources|PCCS]] • [[Catalogues#SZ Catalogue|PSZ]] • [[Catalogues#Catalogue_of_Planck_Galactic_Cold_Clumps|PGCC]]<br />
##[[CMB_and_astrophysical_component maps | CMB and astrophysical component maps]]<br />
##[[CMB spectrum & Likelihood Code | CMB spectrum ]]<br />
##[[Cosmological Parameters | Cosmological parameters and MC chains]]<br />
##[[Specially processed maps | Additional maps]]: [[Specially processed maps#Lensing map | Lensing map]] • [[Specially processed maps#Compton parameter map | Compton parameter map]] <br />
<!---##[[Scientific data used to generate Planck products | Scientific data used to generate Planck products]] <span style="color:red">Not ready for release</span>---><br />
<!---##[[Simulation data | Simulation data]] <span style="color:red">Not ready for release</span><br />
##[[DatesObs|Dates of observations]]---><br />
<!--- ############# ---><br />
#[[Software utilities|Software utilities]]<br />
##[[Unit conversion and Color correction|Unit conversion and Colour correction]] <br />
<!--- ############# ---><br />
#[[Operational data]]<br />
<!---##[[Thermal|Thermal and cooler system]]---><br />
##[[Survey history | Survey history data]]<br />
##[[Planck operational state history]]<br />
<!---##[[FOG|Fibre-optic gyro]]---><br />
##[[SREM|Space radiation environment monitor]]<br />
#[[Appendix]]<br />
##[[Glossary]]<br />
##[[List of acronyms]]<br />
[[Category:PSOBook]]</div>
Xdupac
https://wiki.cosmos.esa.int/planckpla2015/index.php?title=Product_Table_for_PLAv2&diff=11026
Product Table for PLAv2
2015-02-03T17:11:00Z
<p>Xdupac: /* Catalogues */</p>
<hr />
<div>{{DISPLAYTITLE:Products table for PLAv2}}<br />
==Product categories==<br />
*New products for this release that I believe have been confirmed appear in <span style="color:Blue">blue font</span>, products that are still TBC in <span style="color:Red">red font</span> (if it is one entire category of products I will just use color in the products category name, e.g. <span style="color:Blue">1 year maps</span>). Please check this in the tables and let me know whether there are any errors.<br />
*The Obs column contains links to notes at the end of each table. Please check the notes and let me know your feedback.<br />
*More general comments appear at the end of the numbered notes.<br />
<br />
I suggest you use the [[Talk:Product_Table_for_PLAv2|discussion page associated with this page]] to provide your feedback or make any comments relate to the list of products. The discussion page has the same structures in terms of sections as this page. Please try to write your comments/feedback in the appropriate section. I would also ask you to put your initials in the comments you write so that I can more easily get back to you to try to clarify any questions. Yes, it is true I can find out who wrote what in the history page but it makes my life easier if you associate your name to the comments you provide.<br />
<br />
The '''Description''' column will be used to add a one line description of the product that will appear in the archive as a tooltip associated with the product to allow a quick identification by users.<br />
===Time Series===<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=1050px<br />
|+ '''FITS filenames'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" rowspan="9" | <span style="color:Blue">Detector timeseries</span><br />
|rowspan="3" align="center" | LFI <br />
| LFI_TOI_030-SCI_R2.xx_ODXXXX.fits<br />
| <br />
| <br />
|00 <br />
| 10-09-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| LFI_TOI_044-SCI_R2.xx_ODXXXX.fits<br />
| <br />
| <br />
| 00<br />
| 10-09-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| LFI_TOI_070-SCI_R2.xx_ODXXXX.fits<br />
| <br />
| <br />
| 00<br />
| 10-09-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
|rowspan="6" align="center" | HFI <br />
| HFI_TOI_100-SCI_R2.xx_ODXXXX.fits<br />
| Only PSB: not for Feb. 2015 release<br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
|<br />
|-<br />
| HFI_TOI_143-SCI_R2.xx_ODXXXX.fits<br />
| without PSBs<br />
| <br />
| 00<br />
| 20/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_TOI_217-SCI_R2.xx_ODXXXX.fits<br />
| without PSBs<br />
| <br />
| 00<br />
| 20/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_TOI_353-SCI_R2.xx_ODXXXX.fits<br />
| with PSBs<br />
| <br />
| 00<br />
| 19/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_TOI_545-SCI_R2.xx_ODXXXX.fits<br />
| <br />
| <br />
| 00<br />
| 23/01/2015<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_TOI_857-SCI_R2.xx_ODXXXX.fits<br />
| <br />
| <br />
| 00<br />
| 23/01/2015<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="7" | <span style="color:Blue">Offsets</span><br />
| rowspan="6" align="center"| LFI <br />
| LFI_TOI_030-OFF_R2.xx_ODXXXX-full.fits<br />
| <br />
| <br />
| 00<br />
| 19-09-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_TOI_044-OFF_R2.xx_ODXXXX-full.fits<br />
| <br />
| <br />
| 00<br />
| 19-09-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_TOI_070-OFF_R2.xx_ODXXXX-full.fits<br />
| <br />
| <br />
|00<br />
| 19-09-2014 <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_TOI_030-OFF_R2.xx_ODXXXX-full-ringhalf.fits<br />
| <br />
| <br />
| 00<br />
| 11-11-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_TOI_044-OFF_R2.xx_ODXXXX-full-ringhalf.fits<br />
| <br />
| <br />
| 00<br />
| 11-11-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_TOI_070-OFF_R2.xx_ODXXXX-full-ringhalf.fits<br />
| <br />
| <br />
| 00<br />
| 11-11-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
|align="center"| HFI <br />
| HFI_TOI_AllFreqs-OFF_R2.xx.fits<br />
|<br />
|<br />
|00<br />
|13/01/2015<br />
|style="background-color: green;" |<br />
|style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan=9| <span style="color:Blue">Pointing</span><br />
| align="center" rowspan="3"| LFI <br />
| LFI_TOI_030-PTG_R2.xx_ODXXXX.fits <br />
|<br />
| <br />
|00 <br />
|18-07-2014 <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_TOI_044-PTG_R2.xx_ODXXXX.fits <br />
|<br />
| <br />
| 00 <br />
| 18-07-2014 <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_TOI_070-PTG_R2.xx_ODXXXX.fits <br />
|<br />
| <br />
| 00 <br />
| 18-07-2014 <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| rowspan=6 align="center"| HFI <br />
| HFI_TOI_100-PTG_R2.xx_ODXXXX.fits <br />
|<br />
| <br />
| 01 <br />
| 26-08-2014 <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_TOI_143-PTG_R2.xx_ODXXXX.fits <br />
|<br />
| <br />
| 01 <br />
| 26-08-2014 <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_TOI_217-PTG_R2.xx_ODXXXX.fits <br />
|<br />
| <br />
| 01 <br />
| 26-08-2014 <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_TOI_353-PTG_R2.xx_ODXXXX.fits <br />
|<br />
| <br />
| 01 <br />
| 26-08-2014 <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_TOI_545-PTG_R2.xx_ODXXXX.fits <br />
|<br />
| <br />
| 01 <br />
| 26-08-2014 <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_TOI_857-PTG_R2.xx_ODXXXX.fits <br />
|<br />
| <br />
| 01 <br />
| 26-08-2014 <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="4"| <span style="color:Blue">Time stamps</span><br />
| align="center" rowspan="3"| LFI <br />
| LFI_TOI_030-TAI_R2.xx_ODXXXX.fits <br />
|<br />
| <br />
|00 <br />
| 20-09-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_TOI_044-TAI_R2.xx_ODXXXX.fits <br />
|<br />
| <br />
| 00 <br />
| 20-09-2014 <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_TOI_070-TAI_R2.xx_ODXXXX.fits <br />
|<br />
| <br />
| 00<br />
| 20-09-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| align="center"| HFI <br />
| HFI_TOI_AllFreqs-TAI_R2.xx_ODXXXX.fits <br />
|<br />
| <br />
| 00<br />
| 20-09-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan=8| <span style="color:Blue">HK</span> <br />
|align="center" rowspan="8"| LFI <br />
| LFI_TOI_DAE-FAST-HK_R2.XX_ODXXX.fits<br />
| <br />
| <br />
|00 <br />
|14-08-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| LFI_TOI_DAE-SlowConfiguration-HK_R2.XX_ODXXXX.fits<br />
| <br />
| <br />
|00 <br />
|14-08-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| LFI_TOI_DAE-SlowCurrent-HK_R2.XX_ODXXXX.fits<br />
| <br />
| <br />
|00 <br />
|14-08-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| LFI_TOI_DAE-SlowPhaseSwitch-HK_R2.XX_ODXXXX.fits<br />
| <br />
| <br />
|00 <br />
|14-08-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" | <br />
| <br />
|<br />
|-<br />
| LFI_TOI_DAE-SlowVoltage-HK_R2.XX_ODXXXX.fits<br />
| <br />
| <br />
|00 <br />
|14-08-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" | <br />
| <br />
|<br />
|-<br />
| LFI_TOI_REBA-HK_R2.XX_ODXXXX.fits<br />
| <br />
| <br />
|00 <br />
|14-08-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" | <br />
| <br />
|<br />
|-<br />
| SCS_TOI_EssentialASW(R)-HK_R2.XX_ODXXXX.fits<br />
| <br />
| <br />
|00 <br />
|14-08-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" | <br />
| <br />
| <br />
|-<br />
| SCS_TOI_NonEssentialASW(R)-HK_R2.XX_ODXXXX.fits<br />
| <br />
| <br />
|00 <br />
|14-08-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" | <br />
| <br />
| <br />
|-<br />
|}<br />
<br />
===Maps===<br />
====Sky Maps====<br />
=====All detectors=====<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=1050px<br />
|+ '''All Detectors'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" rowspan="56" | Survey maps<br />
| rowspan="32" align="center"| LFI<br />
| LFI_SkyMap_030_1024_R2.xx_survey-1.fits<br />
| <br />
| <br />
| 01<br />
| 26/01/2015<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_030_1024_R2.xx_survey-2.fits<br />
| <br />
| <br />
| 01<br />
| <br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_030_1024_R2.xx_survey-3.fits<br />
| <br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_030_1024_R2.xx_survey-4.fits<br />
| <br />
| <br />
|01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_030_1024_R2.xx_survey-5.fits<br />
| <br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_030_1024_R2.xx_survey-6.fits<br />
| <br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_030_1024_R2.xx_survey-7.fits<br />
| <br />
|<br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_030_1024_R2.xx_survey-8.fits<br />
| <br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_survey-1.fits<br />
| <br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_survey-2.fits<br />
| <br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_survey-3.fits<br />
| <br />
|<br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_survey-4.fits<br />
|<br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_survey-5.fits<br />
| <br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_survey-6.fits<br />
| <br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_survey-7.fits<br />
| <br />
|<br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_survey-8.fits<br />
| <br />
|<br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_survey-1.fits<br />
|<br />
| <br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
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|-<br />
| LFI_SkyMap_070_1024_R2.xx_survey-2.fits<br />
| <br />
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| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
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| LFI_SkyMap_070_1024_R2.xx_survey-3.fits<br />
| <br />
| <br />
|01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
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| LFI_SkyMap_070_1024_R2.xx_survey-4.fits<br />
| <br />
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| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
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| LFI_SkyMap_070_1024_R2.xx_survey-5.fits<br />
| <br />
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| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
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| LFI_SkyMap_070_1024_R2.xx_survey-6.fits<br />
| <br />
|<br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
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| LFI_SkyMap_070_1024_R2.xx_survey-7.fits<br />
| <br />
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| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
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| LFI_SkyMap_070_1024_R2.xx_survey-8.fits<br />
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| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
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| LFI_SkyMap_070_2048_R2.xx_survey-1.fits<br />
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| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
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| LFI_SkyMap_070_2048_R2.xx_survey-2.fits<br />
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| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
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| LFI_SkyMap_070_2048_R2.xx_survey-3.fits<br />
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| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
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| LFI_SkyMap_070_2048_R2.xx_survey-4.fits<br />
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| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
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|-<br />
| LFI_SkyMap_070_2048_R2.xx_survey-5.fits<br />
| <br />
|<br />
| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
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|-<br />
| LFI_SkyMap_070_2048_R2.xx_survey-6.fits<br />
|<br />
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| 01<br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
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| LFI_SkyMap_070_2048_R2.xx_survey-7.fits<br />
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| 01<br />
|<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
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| LFI_SkyMap_070_2048_R2.xx_survey-8.fits<br />
| <br />
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| 01<br />
|<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| rowspan="24" align="center"| HFI<br />
| HFI_SkyMap_100_2048_R2.xx_survey-1.fits<br />
| <br />
|<br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
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|-<br />
| HFI_SkyMap_100_2048_R2.xx_survey-2.fits<br />
| <br />
|<br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
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| HFI_SkyMap_100_2048_R2.xx_survey-3.fits<br />
| <br />
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| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
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| HFI_SkyMap_100_2048_R2.xx_survey-4.fits<br />
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| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
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|-<br />
| HFI_SkyMap_143_2048_R2.xx_survey-1.fits<br />
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| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
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| HFI_SkyMap_143_2048_R2.xx_survey-2.fits<br />
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| 00<br />
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| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
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|-<br />
| HFI_SkyMap_143_2048_R2.xx_survey-3.fits<br />
| <br />
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| style="background-color: green;" |<br />
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| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
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| HFI_SkyMap_217_2048_R2.xx_survey-1.fits<br />
| <br />
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| HFI_SkyMap_217_2048_R2.xx_survey-4.fits<br />
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| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
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| HFI_SkyMap_353_2048_R2.xx_survey-1.fits<br />
| <br />
| <br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
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|-<br />
| HFI_SkyMap_353_2048_R2.xx_survey-2.fits<br />
| <br />
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| style="background-color: green;" |<br />
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| HFI_SkyMap_353_2048_R2.xx_survey-3.fits<br />
| <br />
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| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
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| HFI_SkyMap_353_2048_R2.xx_survey-4.fits<br />
| <br />
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| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_545_2048_R2.xx_survey-1.fits<br />
| <br />
| <br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
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|-<br />
| HFI_SkyMap_545_2048_R2.xx_survey-2.fits<br />
| <br />
|<br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
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|-<br />
| HFI_SkyMap_545_2048_R2.xx_survey-3.fits<br />
| <br />
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| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
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| HFI_SkyMap_545_2048_R2.xx_survey-4.fits<br />
| <br />
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| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_857_2048_R2.xx_survey-1.fits<br />
| <br />
| <br />
| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
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|-<br />
| HFI_SkyMap_857_2048_R2.xx_survey-2.fits<br />
|<br />
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| 00<br />
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| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
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|-<br />
| HFI_SkyMap_857_2048_R2.xx_survey-3.fits<br />
| <br />
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| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
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|<br />
|-<br />
| HFI_SkyMap_857_2048_R2.xx_survey-4.fits<br />
| <br />
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| 00<br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="28" | <span style="color:Blue">1 year maps</span> <br />
1 year = 2 surveys<br />
<br />
y1=s1+s2<br />
<br />
y2=s3+s4<br />
<br />
y3=s5+s6<br />
<br />
y4=s7+s8<br />
| rowspan="16" align="center" | LFI<br />
| LFI_SkyMap_030_1024_R2.xx_year-1.fits<br />
| <br />
|<br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_030_1024_R2.xx_year-2.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_030_1024_R2.xx_year-3.fits<br />
| <br />
|<br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_030_1024_R2.xx_year-4.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_year-1.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_year-2.fits<br />
| <br />
| <br />
|00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_year-3.fits<br />
| <br />
|<br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_year-4.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_year-1.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_year-2.fits<br />
| <br />
|<br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_year-3.fits<br />
| <br />
|<br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_year-4.fits<br />
| <br />
| <br />
|00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_2048_R2.xx_year-1.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_2048_R2.xx_year-2.fits<br />
| <br />
|<br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_2048_R2.xx_year-3.fits<br />
| <br />
|<br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_2048_R2.xx_year-4.fits<br />
| <br />
| <br />
|00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| rowspan="12" align="center" | HFI<br />
| HFI_SkyMap_100_2048_R2.xx_year-1.fits<br />
| <br />
| <br />
| 00 <br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_100_2048_R2.xx_year-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_143_2048_R2.xx_year-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_143_2048_R2.xx_year-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_217_2048_R2.xx_year-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_217_2048_R2.xx_year-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_353_2048_R2.xx_year-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_353_2048_R2.xx_year-2.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_545_2048_R2.xx_year-1.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_545_2048_R2.xx_year-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_857_2048_R2.xx_year-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI_SkyMap_857_2048_R2.xx_year-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="12" | <span style="color:Blue">Half mission maps</span><br />
| rowspan="12" align="center"| HFI<br />
| HFI_SkyMap_100_2048_R2.xx_halfmission-1.fits<br />
| <br />
| <br />
| 00 <br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_100_2048_R2.xx_halfmission-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_143_2048_R2.xx_halfmission-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_143_2048_R2.xx_halfmission-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_217_2048_R2.xx_halfmission-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_217_2048_R2.xx_halfmission-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_353_2048_R2.xx_halfmission-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_353_2048_R2.xx_halfmission-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_545_2048_R2.xx_halfmission-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_545_2048_R2.xx_halfmission-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_857_2048_R2.xx_halfmission-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_857_2048_R2.xx_halfmission-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="12" | <span style="color:Blue">Multi year maps</span><br />
| rowspan="12" align="center"| LFI<br />
| LFI_SkyMap_030_1024_R2.xx_year-1-2.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_030_1024_R2.xx_year-1-3.fits<br />
| <br />
| <br />
| 00<br />
| 21/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_030_1024_R2.xx_year-2-4.fits<br />
| <br />
| <br />
| 00<br />
| 21/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_030_1024_R2.xx_year-3-4.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_year-1-2.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_year-1-3.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_year-2-4.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_year-3-4.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_year-1-2.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_year-1-3.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_year-2-4.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_year-3-4.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="20" | Half-ring maps <br />
| rowspan="8" align="center" | LFI <br />
| LFI_SkyMap_030_1024_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
|00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_030_1024_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| rowspan="12" align="center" | HFI <br />
| HFI_SkyMap_100_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_100_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_143_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_143_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_217_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_217_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_353_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_353_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_545_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_545_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_857_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_857_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="10" | Frequency Maps <br />
| rowspan="4" align="center" | LFI <br />
| LFI_SkyMap_030_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| rowspan="6" align="center" | HFI <br />
| HFI_SkyMap_100_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_143_2048_R2.xx_full.fits<br />
| <br />
|<br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_217_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_353_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_545_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_857_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" | Zodi correction maps <br />
| align="center" | HFI <br />
| HFI_CorrMap_<Freq>-Zodi_2048_R2.xx_<Coverage>.fits<br />
| <br />
| <br />
| 00<br />
| 16/12/2014<br />
| style="background-color: green;" |<br />
|style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
|}<br />
<br />
=====Detector maps=====<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=950px<br />
|+ '''HFI detector maps/LFI radiometer maps'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" rowspan="40" | <span style="color:Blue">Full mission</span><br />
| rowspan="22" align="center" | LFI<br />
| LFI_SkyMap_030-27M_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_030-27S_1024_R2.xx_full.fits<br />
| <br />
| <br />
|00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_030-28M_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_030-28S_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_044-24M_1024_R2.xx_full.fits<br />
| <br />
|<br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_044-24S_1024_R2.xx_full.fits<br />
| <br />
|<br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_044-25M_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_044-25S_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_044-26M_1024_R2.xx_full.fits<br />
| <br />
|<br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_044-26S_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_070-18M_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_070-18S_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_070-19M_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_070-19S_1024_R2.xx_full.fits<br />
|<br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_070-20M_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_070-20S_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_070-21M_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_070-21S_1024_R2.xx_full.fits<br />
| <br />
| <br />
|00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_070-22M_1024_R2.xx_full.fits<br />
| <br />
|<br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_070-22S_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_070-23M_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| LFI_SkyMap_070-23S_1024_R2.xx_full.fits<br />
| <br />
| <br />
|00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note9|[9]]]<br />
|-<br />
| rowspan="18" align="center" | HFI<br />
| HFI_SkyMap_143-5_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_143-6_2048_R2.xx_full.fits<br />
| <br />
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!bgcolor="ffdead" scope="row" rowspan="80" | <span style="color:Blue">Half rings</span><br />
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| rowspan="36" align="center" | HFI<br />
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| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_217-1_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_217-2_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
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| [[#note8|[8]]][[#note9|[9]]]<br />
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| HFI_SkyMap_217-2_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
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| HFI_SkyMap_217-3_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
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| [[#note8|[8]]][[#note9|[9]]]<br />
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| HFI_SkyMap_217-3_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
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| style="background-color: green;" |<br />
|style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_217-4_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_217-4_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
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|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_353-1_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_353-1_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_353-2_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
|00<br />
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| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
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| HFI_SkyMap_353-2_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
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| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_353-7_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_353-7_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
|<br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_353-8_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_353-8_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_545-1_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_545-1_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_545-2_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_545-2_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_545-4_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_545-4_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_857-1_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
|00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_857-1_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_857-2_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_857-2_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_857-3_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
|00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note8|[8]]][[#note9|[9]]]<br />
|-<br />
| HFI_SkyMap_857-3_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_857-4_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_857-4_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|}<br />
<br />
=====Detector set maps=====<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=1050px<br />
|+ '''Detector set maps'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" rowspan="16" | <span style="color:Blue">Full mission</span><br />
| rowspan="8" align="center" | LFI<br />
| LFI_SkyMap_044-24_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| [[#note12|[12]]]<br />
|-<br />
| LFI_SkyMap_044-25-26_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| [[#note12|[12]]]<br />
|-<br />
| LFI_SkyMap_070-18-23_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note12|[12]]]<br />
|-<br />
| LFI_SkyMap_070-19-22_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note12|[12]]]<br />
|-<br />
| LFI_SkyMap_070-20-21_1024_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note12|[12]]]<br />
|-<br />
| LFI_SkyMap_070-18-23_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note12|[12]]]<br />
|-<br />
| LFI_SkyMap_070-19-22_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note12|[12]]]<br />
|-<br />
| LFI_SkyMap_070-20-21_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note12|[12]]]<br />
|-<br />
| rowspan="8" align="center" | HFI<br />
| HFI_SkyMap_100-ds1_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_100-ds2_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_143-ds1_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_143-ds2_2048_R2.xx_full.fits<br />
| <br />
| <br />
|00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_217-ds1_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_217-ds2_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_353-ds1_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_353-ds2_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="26" | <span style="color:Blue">Half rings</span><br />
| rowspan="10" align="center" | LFI<br />
| LFI_SkyMap_044-24_1024_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044-24_1024_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044-25-26_1024_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_044-25-26_1024_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070-18-23_1024_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
|00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070-18-23_1024_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070-19-22_1024_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070-19-22_1024_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070-20-21_1024_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
|18/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_SkyMap_070-20-21_1024_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 18/11/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| rowspan="16" align="center" | HFI<br />
| HFI_SkyMap_100-ds1_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
|<br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_100-ds1_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_100-ds2_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_100-ds2_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_143-ds1_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_143-ds1_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
|style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_143-ds2_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_SkyMap_143-ds2_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_217-ds1_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
|00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
|| HFI_SkyMap_217-ds1_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
|00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_217-ds2_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_217-ds2_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_353-ds1_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_353-ds1_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_353-ds2_2048_R2.xx_full-ringhalf-1.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| [[#note11|[11]]]<br />
|-<br />
| HFI_SkyMap_353-ds2_2048_R2.xx_full-ringhalf-2.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|}<br />
<br />
=====Low resolution maps=====<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=950px<br />
|+ '''Low resolution maps (with noise cov. mat.)'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" rowspan="2"|Low resolution maps (with noise cov. mat.)<br />
| align="center" | LFI<br />
| LFI_SkyMap_fff_0016_R2.xx_full.fits<br />
| <br />
| <br />
|00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| align="center" | HFI <br />
| HFI_SkyMap_fff_0016_R2.xx_full.fits<br />
| Not for PR2<br />
| <br />
| 01<br />
|04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|}<br />
<br />
=====Correction maps=====<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=1300px<br />
|+ '''Correction maps'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" rowspan="1"| <span style="color:Red">A correction maps</span><br />
| rowspan="10" align="center" | LFI<br />
| <strike>LFI_CorrMap_030-ACorr_NSNS_R2.xx_full.fits</strike><br />
| <br />
| <br />
| <br />
| <br />
|<br />
| <br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="9"| <span style="color:Blue">Band pass correction<br>maps</span><br />
| LFI_CorrMap_030-BPassCorr_0256_R2.xx_full.fits<br />
| <br />
| <br />
|00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_CorrMap_044-BPassCorr_0256_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
| LFI_CorrMap_070-BPassCorr_0256_R2.xx_full.fits<br />
| <br />
| <br />
|00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_CorrMap_030-BPassCorr_0128_R2.xx_full.fits<br />
| <br />
| <br />
|00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_CorrMap_044-BPassCorr_0128_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
| LFI_CorrMap_070-BPassCorr_0128_R2.xx_full.fits<br />
| <br />
| <br />
|00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_CorrMap_030-BPassCorr_0064_R2.xx_full.fits<br />
| <br />
| <br />
|00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_CorrMap_044-BPassCorr_0064_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
| LFI_CorrMap_070-BPassCorr_0064_R2.xx_full.fits<br />
| <br />
| <br />
|00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="12"| <span style="color:Blue">Dust correction<br>maps</span><br />
| rowspan="12" align="center" |HFI <br />
| HFI_CorrMap 353 GHz leakage global fits maps<br />
| <br />
| <br />
| 00<br />
| 09/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| <strike>HFI_CorrMap_100-dustleak-ground_2048_R2.xx_full.fits</strike><br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
|<br />
|-<br />
| <strike>HFI_CorrMap_353-dustleak-diff_2048_R2.xx_full.fits</strike><br />
| <br />
| <br />
| <br />
| <br />
|<br />
| <br />
| <br />
| <br />
|-<br />
| HFI_CorrMap_353-dustleak-ground_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
|24/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| <strike>HFI_CorrMap_353_dustleak-diff_2048_R2.xx_year-1.fits</strike><br />
| <br />
| <br />
| <br />
|<br />
| <br />
| <br />
| <br />
| <br />
|-<br />
| <strike>HFI_CorrMap_353_dustleak-diff_2048_R2.xx_year-2.fits</strike><br />
| <br />
| <br />
| <br />
| <br />
|<br />
| <br />
| <br />
| <br />
|-<br />
| HFI_CorrMap_353_dustleak-ground_2048_R2.xx_year-1.fits<br />
| <br />
| <br />
| 00<br />
| 24/11/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_CorrMap_353_dustleak-ground_2048_R2.xx_year-2.fits<br />
| <br />
| <br />
| 00<br />
| 24/11/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| <strike>HFI_CorrMap_353-ds1-dustleak-diff_2048_R2.xx_full.fits</strike><br />
| <br />
|<br />
| <br />
| <br />
| <br />
| <br />
| <br />
|<br />
|-<br />
| <strike>HFI_CorrMap_353-ds2-dustleak-diff_2048_R2.xx_full.fits</strike><br />
| <br />
| <br />
| <br />
|<br />
| <br />
| <br />
| <br />
| <br />
|-<br />
| HFI_CorrMap_353-ds1-dustleak-ground_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 24/11/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_CorrMap_353-ds2-dustleak-ground_2048_R2.xx_full.fits<br />
| <br />
| <br />
| 00<br />
| 24/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="1"| <span style="color:Blue">CO correction<br>maps</span><br />
| rowspan="1" align="center" | HFI <br />
| <strike>HFI_CorrMap_<freq>-coleak-'''METHOD1'''_2048_R2.xx_full.fits</strike><br />
| <br />
| <br />
| <br />
| <br />
|<br />
| <br />
| <br />
| <br />
|}<br />
<br />
====Covariance matrices====<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=850px<br />
|+ '''Covariance matrices'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" rowspan="4"| Cov. Matrices<br />
| style="text-align:center" rowspan="4"| HFI+LFI<br />
| LFI_NoiseCovMat_030_0016_R2.xx.tgz<br />
| <br />
| <br />
|00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| LFI_NoiseCovMat_044_0016_R2.xx.tgz<br />
| <br />
| <br />
| 00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| LFI_NoiseCovMat_070_0016_R2.xx.tgz<br />
| <br />
| <br />
| 00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| HFI covariance matrices<br />
| Not for PR2<br />
| <br />
| 01<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|}<br />
<br />
====CMB maps====<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=1050px<br />
|+ '''CMB Maps'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" rowspan="6" | CMB anisotropy maps<br />
| rowspan="6" align="center" | COM<br />
| COM_CMB_IQU-nilc-field-X_Nside_R2.xx.fits<br />
| <br />
|<br />
|00 <br />
| 09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_CMB_IQU-sevem-field-X_Nside_R2.xx.fits<br />
| <br />
| <br />
| 00<br />
|09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| COM_CMB_IQU-smica-field-X_Nside_R2.xx.fits<br />
| <br />
| <br />
| 00<br />
|09/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_CMB_IQU-commander-field-X_Nside_R2.xx.fits<br />
| <br />
| <br />
| 00<br />
| 09/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| <strike>COM_CMB_IQU-commrul_0256_R2.xx.fits</strike><br />
| <br />
| <br />
| <br />
|<br />
| <br />
| <br />
| <br />
| <br />
|-<br />
| <span style="color:Red"><strike>Other representations</strike></span><br />
| <br />
| <br />
| <br />
|<br />
| <br />
| <br />
| <br />
| <br />
|-<br />
|}<br />
<br />
====Component maps====<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=950px<br />
|+ '''Component Maps'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" rowspan="3" | CO maps<br />
| align="center" rowspan="3"| HFI<br />
| HFI_CompMap_CO-Type1_2048_R2.xx.fits<br />
| <br />
|<br />
| 00<br />
| 04/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| HFI_CompMap_CO-Type2_2048_R2.xx.fits<br />
| <br />
| <br />
| 00<br />
| 04/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| <strike>HFI_CompMap_CO-Type3_2048_R2.xx.fits</strike><br />
| <br />
| <br />
| <br />
|<br />
| <br />
| <br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="12" | Commander foregrounds<br />
| align="center" rowspan="12"| COM<br />
| COM_CompMap_AME-commander_0256_R2.xx.fits<br />
|<br />
|<br />
| 00<br />
| 11/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| COM_CompMap_CMB-commander_0256_R2.xx.fits<br />
|<br />
|<br />
| 00<br />
| 11/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| COM_CompMap_CO21-commander_2048_R2.xx.fits<br />
|<br />
|<br />
| 00<br />
| 11/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| COM_CompMap_CO-commander_0256_R2.xx.fits<br />
|<br />
|<br />
| 00<br />
| 11/12/2014<br />
| style="background-color: green;" |<br />
|style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_CompMap_dust-commander_0256_R2.xx.fits<br />
|<br />
|<br />
| 00<br />
| 11/12/2014<br />
| style="background-color: green;" |<br />
|style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_CompMap_DustPol-commander_1024_R2.xx.fits<br />
|<br />
|<br />
| 00<br />
| 11/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_CompMap_freefree-commander_0256_R2.xx.fits<br />
|<br />
|<br />
| 00<br />
| 11/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| COM_CompMap_Synchrotron-commander_0256_R2.xx.fits<br />
|<br />
|<br />
| 00<br />
| 11/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
| COM_CompMap_SynchrotronPol-commander_0256_R2.xx.fits<br />
|<br />
|<br />
| 00<br />
| 11/12/2014<br />
| style="background-color: green;" |<br />
|style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_CompMap_SZ-commander_0256_R2.xx.fits<br />
|<br />
|<br />
| 00<br />
| 11/12/2014<br />
| style="background-color: green;" |<br />
|style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_CompMap_ThermalDust-commander_2048_R2.xx.fits<br />
|<br />
|<br />
| 00<br />
| 11/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_CompMap_xline-commander_0256_R2.xx.fits<br />
|<br />
|<br />
| 00<br />
| 11/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" | Lensing maps<br />
| align="center" | COM<br />
| COM_CompMap_Lensing_2048_R2.xx.tar + SimMap tars<br />
|<br />
| <br />
|00<br />
| 27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
|}<br />
<br />
====Masks====<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=850px<br />
|+ '''Masks'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" rowspan='4'| Masks<br />
| style="text-align:center" | <strike>LFI</strike><br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
|-<br />
| style="text-align:center" | HFI<br />
| HFI_Mask_GalPlane-apo 0 2 5 _2048_R2.xx.fits<br />
|<br />
| <br />
| 00<br />
| 19/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| style="text-align:center" rowspan='2'| COM<br />
| COM_CMB_IQU-common-field-MaskInt_2048_R2.xx.fits<br />
| <br />
|<br />
| 00<br />
| 10/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_CMB_IQU-common-field-MaskPol_1024_R2.xx.fits<br />
| <br />
| <br />
| 00<br />
| 10/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan='2'| Point source masks<br />
| style="text-align:center" rowspan='1'| LFI<br />
| LFI_Mask_PointSrc_2048_R2.xx.fits<br />
| <br />
| <br />
| 00<br />
|27/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| style="text-align:center" | HFI<br />
| HFI_Mask_PointSrc_2048_R2.xx.fits<br />
| <br />
| <br />
|00<br />
| 19/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
|}<br />
<br />
===Angular power spectra===<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=1050px<br />
|+ '''Angular power spectra'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" rowspan="2" | CMB angular power spectra<br />
| style="text-align:center" rowspan="2" |COM<br />
| COM_PowerSpect_CMB_R2.xx.fits<br />
|<br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
|-<br />
| <strike>COM_PowerSpect_CMB_R2.xx.txt</strike><br />
|<br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="1"| <strike>Sky Angular power spectrum</strike><br />
| style="text-align:center" rowspan="4" |<br />
| <strike>LFI_PowerSpect_030_R2.xx.fits</strike><br />
|<br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
| [[#note37|[37]]]<br />
|-<br />
|}<br />
<div id="note37"></div>[37] For this release detector and detector set power spectra will not be provided. Instead the detector and detector set maps will be provided.<br />
<br />
===Characterisation===<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=850px<br />
|+ '''Characterization'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" rowspan="3"| RIMO<br />
| style="text-align:center" | LFI<br />
| LFI_RIMO_R2.xx.fits<br />
| <br />
| <br />
|50<br />
| 16/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| style="text-align:center" | HFI<br />
| HFI_RIMO_R2.xx.fits<br />
| <br />
| <br />
| 00<br />
| 20/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| style="text-align:center" | HFI<br />
| HFI beams RIMO(s)<br />
| <br />
| <br />
| 00<br />
| 05/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
|}<br />
<br />
===Catalogues===<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=850px<br />
|+ '''Catalogues'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" rowspan="9"| PCCS<br />
| style="text-align:center" rowspan="9"| COM<br />
| COM_PCCS_030_R2.xx.fits + excl.<br />
| <br />
| <br />
| 02<br />
|15/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_PCCS_044_R2.xx.fits + excl.<br />
| <br />
| <br />
| 02<br />
|15/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_PCCS_070_R2.xx.fits + excl.<br />
| <br />
| <br />
| 02<br />
| 15/12/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_PCCS_100_R2.xx.fits<br />
| <br />
| <br />
| 01<br />
| 19/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_PCCS_143_R2.xx.fits<br />
| <br />
| <br />
| 01<br />
| 19/11/2014<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_PCCS_217_R2.xx.fits<br />
| <br />
| <br />
|01<br />
| 19/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_PCCS_353_R2.xx.fits<br />
| <br />
| <br />
| 01<br />
| 19/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_PCCS_545_R2.xx.fits<br />
| <br />
| <br />
| 01<br />
|19/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_PCCS_857_R2.xx.fits<br />
| <br />
| <br />
| 01<br />
|19/11/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="4"| SZ catalogues<br />
| style="text-align:center" rowspan="4"| COM<br />
| COM_PCCS_SZ-MMF1_R2.xx.fits<br />
| <br />
| <br />
| 08<br />
| 29/01/2015<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_PCCS_SZ-MMF3_R2.xx.fits<br />
| <br />
| <br />
| 08<br />
| 29/01/2015<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
|<br />
|-<br />
| COM_PCCS_SZ-PwS_R2.xx.fits<br />
| <br />
| <br />
| 08<br />
| 29/01/2015<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| COM_PCCS_SZ-union_R2.xx.fits<br />
| <br />
| <br />
| 08<br />
| 03/02/2015<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
|<br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="4"| Other catalogues<br />
| style="text-align:center" rowspan="4"| HFI<br />
| <span style="color:Red"><strike>Dusty source catalogue</strike></span><br />
| <br />
| <br />
|<br />
| <br />
| <br />
| <br />
| <br />
| <br />
|-<br />
| <span style="color:Red"><strike>Radio sources catalogue</strike></span><br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
|-<br />
| <span style="color:Blue">HFI_PCCS_GCC_R2.xx.fits</span><br />
| <br />
| <br />
| 02<br />
| 16/01/2015<br />
|style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
| <span style="color:Blue">High-z catalogue</span><br />
| <br />
| <br />
| <br />
| <br />
|<br />
| <br />
| <br />
| <br />
|-<br />
|}<br />
<br />
===Other products===<br />
{| class="wikitable" align="center" border="1" cellpadding="5" cellspacing="0" width=850px<br />
|+ '''Other products'''<br />
|- <br />
! scope="col" rowspan="2" |<br />
! bgcolor="ffdead" scope="col" rowspan="2" | DPC <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Name <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Description <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Size <br />
! bgcolor="ffdead" scope="col" rowspan="2" | Version<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Date <br />
! bgcolor="ffdead" scope="col" colspan="2" | Verification<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Final<br />
! bgcolor="ffdead" scope="col" rowspan="2" | Obs<br />
|- bgcolor="ffdead"<br />
! scope="col" | PSO<br />
! scope="col" | SAT<br />
|- <br />
!bgcolor="ffdead" scope="row" | Cosmological parameters<br />
| style="text-align:center" rowspan="1"| COM<br />
| Cosmological parameter tables<br />
| <br />
| <br />
| 00<br />
| 28/01/2015<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
|<br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="1"| Codes<br />
| style="text-align:center" rowspan="1"| COM<br />
| Likelihood code<br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
|<br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="11"| Beams<br />
| style="text-align:center" rowspan="5"| <br />
| LFI scanning beams<br />
| <br />
| <br />
| 00<br />
| 21-11-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
| HFI scanning beams<br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
|<br />
| <br />
|-<br />
| Effective beams 30GHz<br />
| <br />
| <br />
| <br />
| 22-09-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
| Effective beams 44GHz<br />
| <br />
| <br />
| <br />
| 24-09-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
| Effective beams 70GHz<br />
| <br />
| <br />
| <br />
| 24-09-2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
| style="text-align:center" rowspan="6"| <br />
| Effective beams 100 GHz<br />
| <br />
| <br />
| <br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
| Effective beams 143 GHz<br />
| <br />
| <br />
| <br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
| Effective beams 217 GHz<br />
| <br />
| <br />
| <br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
| Effective beams 353 GHz<br />
| <br />
| <br />
| <br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
| Effective beams 545 GHz<br />
| <br />
| <br />
| <br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
| Effective beams 857 GGz<br />
| <br />
| <br />
| <br />
| <br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" rowspan="2"| 4D maps<br />
| style="text-align:center" rowspan="2"| LFI<br />
| Code<br />
| <br />
| <br />
| <br />
| <br />
| <br />
| <br />
|<br />
| [[#noteA|[A]]]<br />
|-<br />
| map4D_calib_DDX11_LFIXX_gal_nsideXXX_npsiXXXX.fits<br />
| <br />
| <br />
| <br />
| 19/12/2014<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
|<br />
| [[#noteA|[A]]]<br />
|-<br />
!bgcolor="ffdead" scope="row" | Datesobs<br />
| USPDC<br />
| HFI_DatesObs_<Freq>_2048_R2.xx_surveyX.fits.gz<br />
| <br />
| <br />
| 01<br />
|29/01/2015<br />
| style="background-color: green;" |<br />
| style="background-color: green;" |<br />
| <br />
| <br />
|-<br />
!bgcolor="ffdead" scope="row" | <br />
| <br />
| <br />
| <br />
| <br />
|<br />
| <br />
| <br />
| <br />
| <br />
| <br />
|-<br />
|}<br />
<div id="noteA"></div>[A] '''This is not an official product.'''</div>
Xdupac
https://wiki.cosmos.esa.int/planckpla2015/index.php?title=Survey_scanning_and_performance&diff=11021
Survey scanning and performance
2015-02-03T16:31:13Z
<p>Xdupac: /* Start and end of surveys */</p>
<hr />
<div>== The observation strategy ==<br />
<br />
The Planck ''observation strategy'', or ''scanning strategy'', made use of the characteristics of the Planck spacecraft {{PlanckPapers|planck2011-1-1}} and orbit in order to achieve the survey goals in terms of sky coverage and scanning directions.<br />
<br />
The Planck focal plane scanned the sky in the way explained in the figure below.<br />
<br />
[[file:FocalPlane.png|thumb|300px|Planck focal plane showing the direction of scanning. Polarization-sensitive detectors are drawn with crosses indicating the polarization orientation.]]<br />
<br />
The 353 GHz row scanned the sky in small circles with an 85 deg. bore-sight angle from the spin axis. 545 GHz, 857 GHz, and 143 GHz bolometers, as well as LFI radiometers 25 and 26 had a slightly smaller bore-sight angle, while the other part of the Planck focal plane had larger ones (up to about 89 deg.). The Planck spacecraft spun at a rate of 1 rpm.<br />
<br />
Planck, being at L2, moved along the Ecliptic at approximately one degree per day, and needed to keep the Solar aspect angle below about 9 degrees at all times. In practice, during the surveys, the limit considered was 8 deg. Another celestial constraint is that the angle between the Planck spin axis and the anti-Earth direction could not exceed 15 deg. (relaxed to 17 deg. from Survey 5 onward). These constraints had a very direct influence on the chosen scanning strategy.<br />
<br />
[[File:ScannStrategy.png|thumb|300px|Simplified illustration of the Planck scanning strategy, without additional motion of the spin axis.]]<br />
<br />
[[File:Observing_strat.png|thumb|300px|left|Planck scanning strategy, showing the additional motion of the spin axis.]]<br />
<br />
The path followed by the Planck spin axis was defined with respect to the Ecliptic plane. It corresponded to a motion in longitude which maintained an anti-Sun pointing (about one degree per day), to which was added a cycloidal motion (precession) of the spin axis around the anti-Sun position (fiducial point). The cycloidal path was defined by the functions: <br />
<br />
$ λ = θ sin((-1)^n ω (t-t_0)+φ) $ (eq. 1),<br />
<br />
$β = -θ cos((-1)^n ω(t-t_0) + φ) $ (eq. 2),<br />
<br />
where λ is the angular distance from the fiducial point in Ecliptic longitude, β the angular distance from the fiducial point in Ecliptic latitude, θ the spin axis precession amplitude, ω the pulsation of the precession, φ its phase, n the parameter which controls the motion direction of the precession, t is the time, and $t_0$ is the first time during the Planck survey at which the fiducial point crosses the Ecliptic longitude =0 line.<br />
<br />
[[File:Cycloidal_scanning.JPG|thumb|300px|Spin axis path with a 7 deg. amplitude cycloidal scanning, from Ref.{{BibCite|dupac2005}}]]<br />
<br />
The reasons to decide to use such a precession of the spin axis are the following.<br />
<br />
* An excursion of the spin axis from the anti-Sun direction is required to fully observe the whole sky (no excursion would leave a large area unobserved around the Ecliptic poles).<br />
<br />
* The precession motion keeps the Sun aspect angle constant during the whole survey, therefore minimizing the thermal constraint variations on the spacecraft.<br />
<br />
The following precession parameters were chosen for the BSS.<br />
<br />
* Amplitude θ = 7.5deg. (this value is the lowest possible which allows the whole sky to be covered with all detectors).<br />
<br />
* n = 1 (anti-clockwise motion as seen from the Sun).<br />
<br />
* Pulsation ω = 2π / (half a year), faster precession was considered, and has interesting advantages, but was not possible given the constraints if one wants to keep a 7.5 deg. amplitude (which is necessary to cover the whole sky).<br />
<br />
* The phase of the precession was decided according to this set of criteria (in order of importance):<br />
<br />
a) respecting the operational constraints;<br />
<br />
b) allowing the largest possible angle between two scans on the Crab Nebula (a polarization calibrator);<br />
<br />
c) avoiding null dipole amplitude for the whole mission;<br />
<br />
d) optimizing the position of the planets in the beginning of the survey and with respect to the feasibility of their recovery;<br />
<br />
e) placing the two “deep fields” where Galactic foregrounds are minimum;<br />
<br />
f) allowing a reasonable survey margin (i.e. the time allowed to recover lost pointings if a problem occurs).<br />
<br />
The phase is 340 deg. for Surveys 1 to 4, and 250 deg. for Surveys 5 to 8.<br />
<br />
The scanning strategy for the second year of Routine Operations (i.e. Surveys 3 and 4) was exactly the same as for the first year, except that all pointings were shifted by 1 arcmin along the cross-scanning direction, in order to provide finer sky sampling for the highest frequency detectors when combining two years of observations.<br />
<br />
The change of phase between Survey 4 and Survey 5 occurred because it was found essential (especially on the HFI side) that scanning direction crossings should be increased in the Planck survey. By choosing a phase 90 deg. away from the original one, one optimizes the scanning strategy in this respect.<br />
<br />
The details of the justifications for these parameters can be found in PL-WG9-TN-001.<br />
<br />
The scanning strategy parameters are input to the PSO Survey Planning and Performance Tool, which is the software which generates the series of pointing records to be sent out to MOC for implementation.<br />
<br />
An approximate visualization of the Planck scanning strategy can be found [http://www.youtube.com/watch?v=WwFXuZ0B3B8 here] and [http://www.youtube.com/watch?v=7Zu-aiEiDtY here].<br />
<br />
<br />
===Spin axis manoeuvres and exact pointings===<br />
The motion of the spin axis was not continuous. Every change in the spin axis position was initiated by a manoeuvre which required less than 5 minutes time to complete. <br />
<br />
The duration between spin-axis manoeuvres is hereafter referred to as the “dwelling time" and the angular distance between manoeuvres along the spin axis path is hereafter referred to as the “spacing”. <br />
<br />
The dwelling times and spacings are defined as follows:<br />
<br />
* the spacings are fixed to 2arcmin, which roughly corresponds to the Nyquist criterion for sampling the highest-frequency HFI detectors;<br />
<br />
* the dwell times vary from 2360 s to 3904 s.<br />
The exact series of coordinates and dwell times are set by Eqs. (1) and (2) when one has fixed the spacings.<br />
<br />
== Data gap recoveries ==<br />
<br />
Gaps in the data flow can occur for various reasons.<br />
<br />
Anomalies may occur at spacecraft or instrument level, but also due to failures in the ground-to-spacecraft link or the ground segment itself. The adverse effects of such anomalies may be the loss of scientific data corresponding to one or several planned pointings, which have not been acquired and/or stored in memory.<br />
<br />
Failure to acquire proper scientific data may occur to one or both instruments.<br />
<br />
When a gap occurred, scientific criteria were applied to decide whether to recover the data through the Small-Gap Recovery procedure.<br />
<br />
[[File:AHF_353_OD389.png|thumb|400px|Integration time of the 353 GHz detectors ({{PlanckPapers|lamarre2010}}) after 389 Operational Days (the unit is seconds per square degree, normalized to one detector). The first significant data gap and recovery are clearly visible.]]<br />
<br />
The Small-Gap Recovery (SGR) procedure could be applied by MOC or PSO.<br />
<br />
* '''MOC-triggered SGR''': Within its nominal scheduling procedure for an OD, the MOC searches the PPL for PREF corresponding to the OD being processed and any pointings which are the subject of a Small Gap Recovery. As the PREF are sorted in chronological order according to their nominal start time, those corresponding to a small gap will naturally be the earliest. After checking attitude constraints, all observable pointings are listed and their dwell times reduced (initially) to the Minimum Dwell Time (MDT), as given in the PPL.<br />
Having included all valid PREF the required slew times are calculated. With the required slew times and minimum dwell times for all pointings, the OD schedule may be under-populated; in this case the dwell times of all scheduled pointings will be increased equally to make use of all available time in the OD. If the resulting schedule is over-populated, even with MDT for all pointings, the recovery cannot be constrained to a single OD. The sequence of pointings for the ODs involved is optimized in PREF scheduling and dwell times determined in order to effect the recovery and revert to the nominal timeline as quickly as possible.<br />
<br />
* '''PSO-triggered SGR''':<br />
PSO declares a small gap when pointings that have been executed result in data of insufficient quality or inadequate frequency coverage. This assessment is based on data quality and instrument health information provided by the DPCs. The algorithm that was used by the PSO to check the scientific validity of a pointing was implemented within the SPPT software tool. The SPPT ingested on a weekly basis a Weekly Health Report (WHR) for the HFI and LFI containing information on the working status of each detector and their expected condition over the following four weeks. On a daily basis, a Daily Quality Report (DQR) provided by the DPCs for both instruments, included a set of parameters that described the quality of the detection achieved by each individual detector for every pointing executed.<br />
<br />
The scheme for declaring a Small-Gap Recovery from PSO is the following.<br />
<br />
- If a pointing fails to meet the chosen requirement, it becomes an SGR candidate.<br />
<br />
- If there are at least 12 consecutive pointings which are declared SGR candidates, and the problem has been identified and solved, then an SGR is triggered.<br />
Recoveries are only carried out if the recovery slewing is guaranteed to be in OCM. MOC carried out this analysis and decided whether they should perform the SGR accordingly.<br />
<br />
- The start and end times of the gap and the list of the pointing numbers (or just the numbers of the first and last pointings to be recovered) were then sent to MOC by E-mail, with the notification to start a Small-Gap Recovery.<br />
<br />
- MOC implemented the Small-Gap Recovery, provided the pointings could still be scheduled with respect to their latest start time, using the same scheme as described in the MOC-triggered SGR section<br />
<br />
Throughout the Planck mission, data losses were very rare. In fact Small-Gap Recovery was applied only a couple of times.<br />
<br />
==Special observations==<br />
The special observations are now described.<br />
<br />
* Normal scanning on Solar System objects for calibration purposes.<br />
<br />
[[File:Crab_Nebula.jpg|thumb|200px|The Crab Nebula (Messier 1, NGC 1952, Taurus A), here seen by the Hubble Space Telescope.]]<br />
<br />
[[File:Mars.jpg|thumb|200px|Mars as seen by the Hubble Space Telescope in 1999.]]<br />
<br />
This concerns the following objects (specifically planets): Mars; Jupiter; Saturn; Uranus; and Neptune. Their thermal emission in the far-infrared and the small angular sizes make them ideal calibrators for bolometers and radiometers.<br />
<br />
Mars is a particularly interesting calibrator for Planck, because of its proper motion.<br />
However this proper motion makes it difficult to observe it many times during the mission.<br />
<br />
Jupiter is the brightest source for (non-polarized) calibration. Saturn was also used significantly, with Uranus and Neptune being secondary calibrators.<br />
<br />
* Normal scanning on other (non-moving) sources for calibration purposes.<br />
<br />
This concerns mostly the Crab Nebula for polarization calibration purposes.<br />
This supernova remnant is highly polarized, and as such represents the main polarization calibrator for Planck.<br />
<br />
* Special pointings during the calibration phase, not relative to celestial sources.<br />
<br />
* "Deep rings," special observations that were performed on each passage of Jupiter and the Crab Nebula, from January 2012 onward.<br />
<br />
These consist of very deeply sampled observations (0.5') with the spin axis along the Ecliptic plane, typically lasting two to three weeks.<br />
<br />
Such observations benefit from special relaxing of the celestial constraints, with Solar Aspect Angles < 9 deg. rather than < 8 deg. during cycloidal surveying.<br />
<br />
* "Drift scans," special observations performed on Mars, making use of its proper motion.<br />
<br />
==Start and end of surveys==<br />
<br />
The completion of a given “survey” is declared when the logical AND of all frequency-coverage maps is greater than 95 %, OR the sky has been surveyed over a consecutive period of 7.5 months. Note that this definition is that of the Project Scientist and Planck Science Office. Data processing centres do not use exactly the same concept of surveys to create "survey" maps.<br />
<br />
In practice, since the gaps during the surveys have always been very small, this results in approximately 6 months per survey.<br />
<br />
[[File:PlanckMissionTimeline.JPG|thumb|300px|Planck mission timeline with the distribution of the "sky surveys".]]<br />
<br />
* '''Survey 1''': starts 13 August 2009, ends 13 February 2010.<br />
<br />
* '''Survey 2''': starts 14 February 2010, ends 13 August 2010.<br />
<br />
* '''Survey 3''': starts 14 August 2010, ends 13 February 2011.<br />
<br />
* '''Survey 4''': starts 14 February 2011, ends 29 July 2011.<br />
<br />
(This survey was shortened in ordered to start earlier with the new scanning strategy; see above).<br />
<br />
* '''Survey 5''': starts 29 July 2011, ends 30 January 2012.<br />
<br />
* '''Survey 6''' (LFI only): starts 30 January 2012, ends 31 July 2012.<br />
<br />
* '''Survey 7''' (LFI only): starts 31 July 2012, ends 31 January 2013.<br />
<br />
* '''Survey 8''' (LFI only): starts 1 February 2013, ends 1 August 2013.<br />
<br />
* '''Survey 9''' (LFI only): ends Oct. 3rd, 2013<br />
<br />
<br />
=== Completion of full sky coverage during Surveys 1-2 ===<br />
<br />
The picture gallery below exhibits the progress of sky coverage during the first months of survey (black colour = unobserved areas).<br />
<br />
<br />
<gallery widths=330 perrow=3 caption="HFI 353 GHz integration time after N months of survey. The units here are seconds per square degree, normalized to one detector."><br />
File:353_1month.png|After 1 month<br />
File:353_2month.png|After 2 months<br />
File:353_3month.png|After 3 months<br />
File:353_4month.png|After 4 months<br />
File:353_5month.png|After 5 months<br />
File:353_6month.png|After 6 months<br />
File:353_7month.png|After 7 months<br />
File:353_8month.png|After 8 months<br />
File:353_9months.png|After 9 months<br />
File:353_10months.png|After 10 months<br />
File:353_11months.png|After 11 months<br />
File:353_12months.png|After 12 months<br />
</gallery><br />
<br />
== Main planet and Crab observations ==<br />
<br />
Solar System objects and the Crab Nebula have been observed many times during the Planck surveys. Here is a list of these observations, with the ''deep rings'' (Jupiter and the Crab) and ''drift scans'' (Mars only) in '''boldface'''.<br />
<br />
* Crab: 16-22 September 2009<br />
<br />
* Mars: 17-29 October 2009<br />
<br />
* Jupiter: 25 October – 1 November 2009<br />
<br />
* Neptune: 1-8 November 2009<br />
<br />
* Uranus: 6-16 December 2009<br />
<br />
* Saturn: 2-8 January 2010<br />
<br />
* Crab: 6-12 March 2010<br />
<br />
* Mars: 9-18 April 2010<br />
<br />
* Neptune: 15-23 May 2010<br />
<br />
* Saturn: 13-22 June 2010<br />
<br />
* Uranus: 27 June – 5 July 2010<br />
<br />
* Jupiter: 1-9 July 2010<br />
<br />
* Crab: 15-21 September 2010<br />
<br />
* Neptune: 3-11 November 2010<br />
<br />
* Jupiter: 9-18 December 2010<br />
<br />
* Uranus: 12-21 December 2010<br />
<br />
* Saturn: 15-22 January 2011<br />
<br />
* Crab: 7-12 March 2011<br />
<br />
* Neptune: 18-26 May 2011<br />
<br />
* Saturn: 30 June - 9 July 2011<br />
<br />
* Uranus: 3-11 July 2011<br />
<br />
* Jupiter: 9-15 August 2011<br />
<br />
* Crab: 10-18 September 2011 (performed with the 250 deg. phase cycloidal strategy)<br />
<br />
* Crab: 20-23 September 2011 (performed with the 340 deg. phase cycloidal strategy)<br />
<br />
* '''Mars''': 8-16 December 2011 ("drift scan", Mars allowed to move through the Planck focal plane via its proper motion)<br />
<br />
* Mars: 17-26 December 2011 (normal scanning)<br />
<br />
* '''Jupiter''': 8-30 January 2012 (deep ring)<br />
<br />
* '''Crab''': 26 February - 16 March 2012 (deep ring)<br />
<br />
* '''Jupiter''': 1-14 September 2012 (deep ring)<br />
<br />
* '''Crab''': 14 September - 1 October 2012 (deep ring)<br />
<br />
* Neptune: 19-27 November 2012<br />
<br />
* Uranus: 24-30 December 2012<br />
<br />
* Saturn: 30 January - 5 February 2013<br />
<br />
* '''Jupiter''': February 2013 (deep ring)<br />
<br />
* '''Crab''': Feb. 28th - March 15th, 2013 (deep ring)<br />
<br />
* Neptune: June 4th - June 12th, 2013<br />
<br />
* Uranus: July 9-16th, 2013<br />
<br />
* Saturn: July 20-26th, 2013<br />
<br />
* '''Crab''': Sept. 10th - Oct. 3rd, 2013 (deep ring)<br />
<br />
Note that on Sept. 14-16th, 2013, LFI also performed a special dipole calibration observation.<br />
<br />
== Resulting integration time distribution ==<br />
<br />
The integration time after the end of HFI operations (January 2012) is shown in the following picture gallery.<br />
<br />
Units are seconds per square degree, normalized to one detector, for all maps. The projection is full-sky Mollweide centred on the Galactic centre.<br />
<br />
<br />
<br />
<gallery widths=330px perrow=3 caption="Integration time after the end of HFI operations (January 2012). The units here are seconds per square degree, normalized to one detector."><br />
File:HFI_fullmission_100GHz1-4.png|HFI 100 GHz 1,4<br />
File:HFI_fullmission_100GHz2-3.png|HFI 100 GHz 2,3<br />
File:HFI_fullmission_143GHz1-4.png|HFI 143 GHz 1-4<br />
File:HFI_fullmission_143GHz5-8.png|HFI 143 GHz 5-8<br />
File:HFI_fullmission_217GHz1-4.png|HFI 217 GHz 1-4<br />
File:HFI_fullmission_217GHz5-8.png|HFI 217 GHz 5-8<br />
File:HFI_fullmission_353GHz.png|HFI 353 GHz<br />
File:HFI_fullmission_545-857GHz.png|HFI 545 GHz / 857 GHz<br />
File:LFI25_coldmission.png|LFI-25 (44 GHz)<br />
File:LFI27_coldmission.png|LFI 30 GHz<br />
</gallery><br />
<br />
==References==<br />
<references /><br />
<br />
[[Category:Introduction|004]]<br />
[[Category:PSOBook]]</div>
Xdupac
https://wiki.cosmos.esa.int/planckpla2015/index.php?title=Survey_scanning_and_performance&diff=11019
Survey scanning and performance
2015-02-03T16:27:27Z
<p>Xdupac: /* Main planet and Crab observations */</p>
<hr />
<div>== The observation strategy ==<br />
<br />
The Planck ''observation strategy'', or ''scanning strategy'', made use of the characteristics of the Planck spacecraft {{PlanckPapers|planck2011-1-1}} and orbit in order to achieve the survey goals in terms of sky coverage and scanning directions.<br />
<br />
The Planck focal plane scanned the sky in the way explained in the figure below.<br />
<br />
[[file:FocalPlane.png|thumb|300px|Planck focal plane showing the direction of scanning. Polarization-sensitive detectors are drawn with crosses indicating the polarization orientation.]]<br />
<br />
The 353 GHz row scanned the sky in small circles with an 85 deg. bore-sight angle from the spin axis. 545 GHz, 857 GHz, and 143 GHz bolometers, as well as LFI radiometers 25 and 26 had a slightly smaller bore-sight angle, while the other part of the Planck focal plane had larger ones (up to about 89 deg.). The Planck spacecraft spun at a rate of 1 rpm.<br />
<br />
Planck, being at L2, moved along the Ecliptic at approximately one degree per day, and needed to keep the Solar aspect angle below about 9 degrees at all times. In practice, during the surveys, the limit considered was 8 deg. Another celestial constraint is that the angle between the Planck spin axis and the anti-Earth direction could not exceed 15 deg. (relaxed to 17 deg. from Survey 5 onward). These constraints had a very direct influence on the chosen scanning strategy.<br />
<br />
[[File:ScannStrategy.png|thumb|300px|Simplified illustration of the Planck scanning strategy, without additional motion of the spin axis.]]<br />
<br />
[[File:Observing_strat.png|thumb|300px|left|Planck scanning strategy, showing the additional motion of the spin axis.]]<br />
<br />
The path followed by the Planck spin axis was defined with respect to the Ecliptic plane. It corresponded to a motion in longitude which maintained an anti-Sun pointing (about one degree per day), to which was added a cycloidal motion (precession) of the spin axis around the anti-Sun position (fiducial point). The cycloidal path was defined by the functions: <br />
<br />
$ λ = θ sin((-1)^n ω (t-t_0)+φ) $ (eq. 1),<br />
<br />
$β = -θ cos((-1)^n ω(t-t_0) + φ) $ (eq. 2),<br />
<br />
where λ is the angular distance from the fiducial point in Ecliptic longitude, β the angular distance from the fiducial point in Ecliptic latitude, θ the spin axis precession amplitude, ω the pulsation of the precession, φ its phase, n the parameter which controls the motion direction of the precession, t is the time, and $t_0$ is the first time during the Planck survey at which the fiducial point crosses the Ecliptic longitude =0 line.<br />
<br />
[[File:Cycloidal_scanning.JPG|thumb|300px|Spin axis path with a 7 deg. amplitude cycloidal scanning, from Ref.{{BibCite|dupac2005}}]]<br />
<br />
The reasons to decide to use such a precession of the spin axis are the following.<br />
<br />
* An excursion of the spin axis from the anti-Sun direction is required to fully observe the whole sky (no excursion would leave a large area unobserved around the Ecliptic poles).<br />
<br />
* The precession motion keeps the Sun aspect angle constant during the whole survey, therefore minimizing the thermal constraint variations on the spacecraft.<br />
<br />
The following precession parameters were chosen for the BSS.<br />
<br />
* Amplitude θ = 7.5deg. (this value is the lowest possible which allows the whole sky to be covered with all detectors).<br />
<br />
* n = 1 (anti-clockwise motion as seen from the Sun).<br />
<br />
* Pulsation ω = 2π / (half a year), faster precession was considered, and has interesting advantages, but was not possible given the constraints if one wants to keep a 7.5 deg. amplitude (which is necessary to cover the whole sky).<br />
<br />
* The phase of the precession was decided according to this set of criteria (in order of importance):<br />
<br />
a) respecting the operational constraints;<br />
<br />
b) allowing the largest possible angle between two scans on the Crab Nebula (a polarization calibrator);<br />
<br />
c) avoiding null dipole amplitude for the whole mission;<br />
<br />
d) optimizing the position of the planets in the beginning of the survey and with respect to the feasibility of their recovery;<br />
<br />
e) placing the two “deep fields” where Galactic foregrounds are minimum;<br />
<br />
f) allowing a reasonable survey margin (i.e. the time allowed to recover lost pointings if a problem occurs).<br />
<br />
The phase is 340 deg. for Surveys 1 to 4, and 250 deg. for Surveys 5 to 8.<br />
<br />
The scanning strategy for the second year of Routine Operations (i.e. Surveys 3 and 4) was exactly the same as for the first year, except that all pointings were shifted by 1 arcmin along the cross-scanning direction, in order to provide finer sky sampling for the highest frequency detectors when combining two years of observations.<br />
<br />
The change of phase between Survey 4 and Survey 5 occurred because it was found essential (especially on the HFI side) that scanning direction crossings should be increased in the Planck survey. By choosing a phase 90 deg. away from the original one, one optimizes the scanning strategy in this respect.<br />
<br />
The details of the justifications for these parameters can be found in PL-WG9-TN-001.<br />
<br />
The scanning strategy parameters are input to the PSO Survey Planning and Performance Tool, which is the software which generates the series of pointing records to be sent out to MOC for implementation.<br />
<br />
An approximate visualization of the Planck scanning strategy can be found [http://www.youtube.com/watch?v=WwFXuZ0B3B8 here] and [http://www.youtube.com/watch?v=7Zu-aiEiDtY here].<br />
<br />
<br />
===Spin axis manoeuvres and exact pointings===<br />
The motion of the spin axis was not continuous. Every change in the spin axis position was initiated by a manoeuvre which required less than 5 minutes time to complete. <br />
<br />
The duration between spin-axis manoeuvres is hereafter referred to as the “dwelling time" and the angular distance between manoeuvres along the spin axis path is hereafter referred to as the “spacing”. <br />
<br />
The dwelling times and spacings are defined as follows:<br />
<br />
* the spacings are fixed to 2arcmin, which roughly corresponds to the Nyquist criterion for sampling the highest-frequency HFI detectors;<br />
<br />
* the dwell times vary from 2360 s to 3904 s.<br />
The exact series of coordinates and dwell times are set by Eqs. (1) and (2) when one has fixed the spacings.<br />
<br />
== Data gap recoveries ==<br />
<br />
Gaps in the data flow can occur for various reasons.<br />
<br />
Anomalies may occur at spacecraft or instrument level, but also due to failures in the ground-to-spacecraft link or the ground segment itself. The adverse effects of such anomalies may be the loss of scientific data corresponding to one or several planned pointings, which have not been acquired and/or stored in memory.<br />
<br />
Failure to acquire proper scientific data may occur to one or both instruments.<br />
<br />
When a gap occurred, scientific criteria were applied to decide whether to recover the data through the Small-Gap Recovery procedure.<br />
<br />
[[File:AHF_353_OD389.png|thumb|400px|Integration time of the 353 GHz detectors ({{PlanckPapers|lamarre2010}}) after 389 Operational Days (the unit is seconds per square degree, normalized to one detector). The first significant data gap and recovery are clearly visible.]]<br />
<br />
The Small-Gap Recovery (SGR) procedure could be applied by MOC or PSO.<br />
<br />
* '''MOC-triggered SGR''': Within its nominal scheduling procedure for an OD, the MOC searches the PPL for PREF corresponding to the OD being processed and any pointings which are the subject of a Small Gap Recovery. As the PREF are sorted in chronological order according to their nominal start time, those corresponding to a small gap will naturally be the earliest. After checking attitude constraints, all observable pointings are listed and their dwell times reduced (initially) to the Minimum Dwell Time (MDT), as given in the PPL.<br />
Having included all valid PREF the required slew times are calculated. With the required slew times and minimum dwell times for all pointings, the OD schedule may be under-populated; in this case the dwell times of all scheduled pointings will be increased equally to make use of all available time in the OD. If the resulting schedule is over-populated, even with MDT for all pointings, the recovery cannot be constrained to a single OD. The sequence of pointings for the ODs involved is optimized in PREF scheduling and dwell times determined in order to effect the recovery and revert to the nominal timeline as quickly as possible.<br />
<br />
* '''PSO-triggered SGR''':<br />
PSO declares a small gap when pointings that have been executed result in data of insufficient quality or inadequate frequency coverage. This assessment is based on data quality and instrument health information provided by the DPCs. The algorithm that was used by the PSO to check the scientific validity of a pointing was implemented within the SPPT software tool. The SPPT ingested on a weekly basis a Weekly Health Report (WHR) for the HFI and LFI containing information on the working status of each detector and their expected condition over the following four weeks. On a daily basis, a Daily Quality Report (DQR) provided by the DPCs for both instruments, included a set of parameters that described the quality of the detection achieved by each individual detector for every pointing executed.<br />
<br />
The scheme for declaring a Small-Gap Recovery from PSO is the following.<br />
<br />
- If a pointing fails to meet the chosen requirement, it becomes an SGR candidate.<br />
<br />
- If there are at least 12 consecutive pointings which are declared SGR candidates, and the problem has been identified and solved, then an SGR is triggered.<br />
Recoveries are only carried out if the recovery slewing is guaranteed to be in OCM. MOC carried out this analysis and decided whether they should perform the SGR accordingly.<br />
<br />
- The start and end times of the gap and the list of the pointing numbers (or just the numbers of the first and last pointings to be recovered) were then sent to MOC by E-mail, with the notification to start a Small-Gap Recovery.<br />
<br />
- MOC implemented the Small-Gap Recovery, provided the pointings could still be scheduled with respect to their latest start time, using the same scheme as described in the MOC-triggered SGR section<br />
<br />
Throughout the Planck mission, data losses were very rare. In fact Small-Gap Recovery was applied only a couple of times.<br />
<br />
==Special observations==<br />
The special observations are now described.<br />
<br />
* Normal scanning on Solar System objects for calibration purposes.<br />
<br />
[[File:Crab_Nebula.jpg|thumb|200px|The Crab Nebula (Messier 1, NGC 1952, Taurus A), here seen by the Hubble Space Telescope.]]<br />
<br />
[[File:Mars.jpg|thumb|200px|Mars as seen by the Hubble Space Telescope in 1999.]]<br />
<br />
This concerns the following objects (specifically planets): Mars; Jupiter; Saturn; Uranus; and Neptune. Their thermal emission in the far-infrared and the small angular sizes make them ideal calibrators for bolometers and radiometers.<br />
<br />
Mars is a particularly interesting calibrator for Planck, because of its proper motion.<br />
However this proper motion makes it difficult to observe it many times during the mission.<br />
<br />
Jupiter is the brightest source for (non-polarized) calibration. Saturn was also used significantly, with Uranus and Neptune being secondary calibrators.<br />
<br />
* Normal scanning on other (non-moving) sources for calibration purposes.<br />
<br />
This concerns mostly the Crab Nebula for polarization calibration purposes.<br />
This supernova remnant is highly polarized, and as such represents the main polarization calibrator for Planck.<br />
<br />
* Special pointings during the calibration phase, not relative to celestial sources.<br />
<br />
* "Deep rings," special observations that were performed on each passage of Jupiter and the Crab Nebula, from January 2012 onward.<br />
<br />
These consist of very deeply sampled observations (0.5') with the spin axis along the Ecliptic plane, typically lasting two to three weeks.<br />
<br />
Such observations benefit from special relaxing of the celestial constraints, with Solar Aspect Angles < 9 deg. rather than < 8 deg. during cycloidal surveying.<br />
<br />
* "Drift scans," special observations performed on Mars, making use of its proper motion.<br />
<br />
==Start and end of surveys==<br />
<br />
The completion of a given “survey” is declared when the logical AND of all frequency-coverage maps is greater than 95 %, OR the sky has been surveyed over a consecutive period of 7.5 months. Note that this definition is that of the Project Scientist and Planck Science Office. Data processing centres do not use exactly the same concept of surveys to create "survey" maps.<br />
<br />
In practice, since the gaps during the surveys have always been very small, this results in approximately 6 months per survey.<br />
<br />
[[File:PlanckMissionTimeline.JPG|thumb|300px|Planck mission timeline with the distribution of the "sky surveys".]]<br />
<br />
* '''Survey 1''': starts 13 August 2009, ends 13 February 2010.<br />
<br />
* '''Survey 2''': starts 14 February 2010, ends 13 August 2010.<br />
<br />
* '''Survey 3''': starts 14 August 2010, ends 13 February 2011.<br />
<br />
* '''Survey 4''': starts 14 February 2011, ends 29 July 2011.<br />
<br />
(This survey was shortened in ordered to start earlier with the new scanning strategy; see above).<br />
<br />
* '''Survey 5''': starts 29 July 2011, ends 30 January 2012.<br />
<br />
* '''Survey 6''' (LFI only): starts 30 January 2012, ends 31 July 2012.<br />
<br />
* '''Survey 7''' (LFI only): starts 31 July 2012, ends 31 January 2013.<br />
<br />
* '''Survey 8''' (LFI only): starts 1 February 2013, ends 1 August 2013.<br />
<br />
<br />
=== Completion of full sky coverage during Surveys 1-2 ===<br />
<br />
The picture gallery below exhibits the progress of sky coverage during the first months of survey (black colour = unobserved areas).<br />
<br />
<br />
<gallery widths=330 perrow=3 caption="HFI 353 GHz integration time after N months of survey. The units here are seconds per square degree, normalized to one detector."><br />
File:353_1month.png|After 1 month<br />
File:353_2month.png|After 2 months<br />
File:353_3month.png|After 3 months<br />
File:353_4month.png|After 4 months<br />
File:353_5month.png|After 5 months<br />
File:353_6month.png|After 6 months<br />
File:353_7month.png|After 7 months<br />
File:353_8month.png|After 8 months<br />
File:353_9months.png|After 9 months<br />
File:353_10months.png|After 10 months<br />
File:353_11months.png|After 11 months<br />
File:353_12months.png|After 12 months<br />
</gallery><br />
<br />
== Main planet and Crab observations ==<br />
<br />
Solar System objects and the Crab Nebula have been observed many times during the Planck surveys. Here is a list of these observations, with the ''deep rings'' (Jupiter and the Crab) and ''drift scans'' (Mars only) in '''boldface'''.<br />
<br />
* Crab: 16-22 September 2009<br />
<br />
* Mars: 17-29 October 2009<br />
<br />
* Jupiter: 25 October – 1 November 2009<br />
<br />
* Neptune: 1-8 November 2009<br />
<br />
* Uranus: 6-16 December 2009<br />
<br />
* Saturn: 2-8 January 2010<br />
<br />
* Crab: 6-12 March 2010<br />
<br />
* Mars: 9-18 April 2010<br />
<br />
* Neptune: 15-23 May 2010<br />
<br />
* Saturn: 13-22 June 2010<br />
<br />
* Uranus: 27 June – 5 July 2010<br />
<br />
* Jupiter: 1-9 July 2010<br />
<br />
* Crab: 15-21 September 2010<br />
<br />
* Neptune: 3-11 November 2010<br />
<br />
* Jupiter: 9-18 December 2010<br />
<br />
* Uranus: 12-21 December 2010<br />
<br />
* Saturn: 15-22 January 2011<br />
<br />
* Crab: 7-12 March 2011<br />
<br />
* Neptune: 18-26 May 2011<br />
<br />
* Saturn: 30 June - 9 July 2011<br />
<br />
* Uranus: 3-11 July 2011<br />
<br />
* Jupiter: 9-15 August 2011<br />
<br />
* Crab: 10-18 September 2011 (performed with the 250 deg. phase cycloidal strategy)<br />
<br />
* Crab: 20-23 September 2011 (performed with the 340 deg. phase cycloidal strategy)<br />
<br />
* '''Mars''': 8-16 December 2011 ("drift scan", Mars allowed to move through the Planck focal plane via its proper motion)<br />
<br />
* Mars: 17-26 December 2011 (normal scanning)<br />
<br />
* '''Jupiter''': 8-30 January 2012 (deep ring)<br />
<br />
* '''Crab''': 26 February - 16 March 2012 (deep ring)<br />
<br />
* '''Jupiter''': 1-14 September 2012 (deep ring)<br />
<br />
* '''Crab''': 14 September - 1 October 2012 (deep ring)<br />
<br />
* Neptune: 19-27 November 2012<br />
<br />
* Uranus: 24-30 December 2012<br />
<br />
* Saturn: 30 January - 5 February 2013<br />
<br />
* '''Jupiter''': February 2013 (deep ring)<br />
<br />
* '''Crab''': Feb. 28th - March 15th, 2013 (deep ring)<br />
<br />
* Neptune: June 4th - June 12th, 2013<br />
<br />
* Uranus: July 9-16th, 2013<br />
<br />
* Saturn: July 20-26th, 2013<br />
<br />
* '''Crab''': Sept. 10th - Oct. 3rd, 2013 (deep ring)<br />
<br />
Note that on Sept. 14-16th, 2013, LFI also performed a special dipole calibration observation.<br />
<br />
== Resulting integration time distribution ==<br />
<br />
The integration time after the end of HFI operations (January 2012) is shown in the following picture gallery.<br />
<br />
Units are seconds per square degree, normalized to one detector, for all maps. The projection is full-sky Mollweide centred on the Galactic centre.<br />
<br />
<br />
<br />
<gallery widths=330px perrow=3 caption="Integration time after the end of HFI operations (January 2012). The units here are seconds per square degree, normalized to one detector."><br />
File:HFI_fullmission_100GHz1-4.png|HFI 100 GHz 1,4<br />
File:HFI_fullmission_100GHz2-3.png|HFI 100 GHz 2,3<br />
File:HFI_fullmission_143GHz1-4.png|HFI 143 GHz 1-4<br />
File:HFI_fullmission_143GHz5-8.png|HFI 143 GHz 5-8<br />
File:HFI_fullmission_217GHz1-4.png|HFI 217 GHz 1-4<br />
File:HFI_fullmission_217GHz5-8.png|HFI 217 GHz 5-8<br />
File:HFI_fullmission_353GHz.png|HFI 353 GHz<br />
File:HFI_fullmission_545-857GHz.png|HFI 545 GHz / 857 GHz<br />
File:LFI25_coldmission.png|LFI-25 (44 GHz)<br />
File:LFI27_coldmission.png|LFI 30 GHz<br />
</gallery><br />
<br />
==References==<br />
<references /><br />
<br />
[[Category:Introduction|004]]<br />
[[Category:PSOBook]]</div>
Xdupac
https://wiki.cosmos.esa.int/planckpla2015/index.php?title=Survey_scanning_and_performance&diff=11018
Survey scanning and performance
2015-02-03T16:25:59Z
<p>Xdupac: /* Main planet and Crab observations */</p>
<hr />
<div>== The observation strategy ==<br />
<br />
The Planck ''observation strategy'', or ''scanning strategy'', made use of the characteristics of the Planck spacecraft {{PlanckPapers|planck2011-1-1}} and orbit in order to achieve the survey goals in terms of sky coverage and scanning directions.<br />
<br />
The Planck focal plane scanned the sky in the way explained in the figure below.<br />
<br />
[[file:FocalPlane.png|thumb|300px|Planck focal plane showing the direction of scanning. Polarization-sensitive detectors are drawn with crosses indicating the polarization orientation.]]<br />
<br />
The 353 GHz row scanned the sky in small circles with an 85 deg. bore-sight angle from the spin axis. 545 GHz, 857 GHz, and 143 GHz bolometers, as well as LFI radiometers 25 and 26 had a slightly smaller bore-sight angle, while the other part of the Planck focal plane had larger ones (up to about 89 deg.). The Planck spacecraft spun at a rate of 1 rpm.<br />
<br />
Planck, being at L2, moved along the Ecliptic at approximately one degree per day, and needed to keep the Solar aspect angle below about 9 degrees at all times. In practice, during the surveys, the limit considered was 8 deg. Another celestial constraint is that the angle between the Planck spin axis and the anti-Earth direction could not exceed 15 deg. (relaxed to 17 deg. from Survey 5 onward). These constraints had a very direct influence on the chosen scanning strategy.<br />
<br />
[[File:ScannStrategy.png|thumb|300px|Simplified illustration of the Planck scanning strategy, without additional motion of the spin axis.]]<br />
<br />
[[File:Observing_strat.png|thumb|300px|left|Planck scanning strategy, showing the additional motion of the spin axis.]]<br />
<br />
The path followed by the Planck spin axis was defined with respect to the Ecliptic plane. It corresponded to a motion in longitude which maintained an anti-Sun pointing (about one degree per day), to which was added a cycloidal motion (precession) of the spin axis around the anti-Sun position (fiducial point). The cycloidal path was defined by the functions: <br />
<br />
$ λ = θ sin((-1)^n ω (t-t_0)+φ) $ (eq. 1),<br />
<br />
$β = -θ cos((-1)^n ω(t-t_0) + φ) $ (eq. 2),<br />
<br />
where λ is the angular distance from the fiducial point in Ecliptic longitude, β the angular distance from the fiducial point in Ecliptic latitude, θ the spin axis precession amplitude, ω the pulsation of the precession, φ its phase, n the parameter which controls the motion direction of the precession, t is the time, and $t_0$ is the first time during the Planck survey at which the fiducial point crosses the Ecliptic longitude =0 line.<br />
<br />
[[File:Cycloidal_scanning.JPG|thumb|300px|Spin axis path with a 7 deg. amplitude cycloidal scanning, from Ref.{{BibCite|dupac2005}}]]<br />
<br />
The reasons to decide to use such a precession of the spin axis are the following.<br />
<br />
* An excursion of the spin axis from the anti-Sun direction is required to fully observe the whole sky (no excursion would leave a large area unobserved around the Ecliptic poles).<br />
<br />
* The precession motion keeps the Sun aspect angle constant during the whole survey, therefore minimizing the thermal constraint variations on the spacecraft.<br />
<br />
The following precession parameters were chosen for the BSS.<br />
<br />
* Amplitude θ = 7.5deg. (this value is the lowest possible which allows the whole sky to be covered with all detectors).<br />
<br />
* n = 1 (anti-clockwise motion as seen from the Sun).<br />
<br />
* Pulsation ω = 2π / (half a year), faster precession was considered, and has interesting advantages, but was not possible given the constraints if one wants to keep a 7.5 deg. amplitude (which is necessary to cover the whole sky).<br />
<br />
* The phase of the precession was decided according to this set of criteria (in order of importance):<br />
<br />
a) respecting the operational constraints;<br />
<br />
b) allowing the largest possible angle between two scans on the Crab Nebula (a polarization calibrator);<br />
<br />
c) avoiding null dipole amplitude for the whole mission;<br />
<br />
d) optimizing the position of the planets in the beginning of the survey and with respect to the feasibility of their recovery;<br />
<br />
e) placing the two “deep fields” where Galactic foregrounds are minimum;<br />
<br />
f) allowing a reasonable survey margin (i.e. the time allowed to recover lost pointings if a problem occurs).<br />
<br />
The phase is 340 deg. for Surveys 1 to 4, and 250 deg. for Surveys 5 to 8.<br />
<br />
The scanning strategy for the second year of Routine Operations (i.e. Surveys 3 and 4) was exactly the same as for the first year, except that all pointings were shifted by 1 arcmin along the cross-scanning direction, in order to provide finer sky sampling for the highest frequency detectors when combining two years of observations.<br />
<br />
The change of phase between Survey 4 and Survey 5 occurred because it was found essential (especially on the HFI side) that scanning direction crossings should be increased in the Planck survey. By choosing a phase 90 deg. away from the original one, one optimizes the scanning strategy in this respect.<br />
<br />
The details of the justifications for these parameters can be found in PL-WG9-TN-001.<br />
<br />
The scanning strategy parameters are input to the PSO Survey Planning and Performance Tool, which is the software which generates the series of pointing records to be sent out to MOC for implementation.<br />
<br />
An approximate visualization of the Planck scanning strategy can be found [http://www.youtube.com/watch?v=WwFXuZ0B3B8 here] and [http://www.youtube.com/watch?v=7Zu-aiEiDtY here].<br />
<br />
<br />
===Spin axis manoeuvres and exact pointings===<br />
The motion of the spin axis was not continuous. Every change in the spin axis position was initiated by a manoeuvre which required less than 5 minutes time to complete. <br />
<br />
The duration between spin-axis manoeuvres is hereafter referred to as the “dwelling time" and the angular distance between manoeuvres along the spin axis path is hereafter referred to as the “spacing”. <br />
<br />
The dwelling times and spacings are defined as follows:<br />
<br />
* the spacings are fixed to 2arcmin, which roughly corresponds to the Nyquist criterion for sampling the highest-frequency HFI detectors;<br />
<br />
* the dwell times vary from 2360 s to 3904 s.<br />
The exact series of coordinates and dwell times are set by Eqs. (1) and (2) when one has fixed the spacings.<br />
<br />
== Data gap recoveries ==<br />
<br />
Gaps in the data flow can occur for various reasons.<br />
<br />
Anomalies may occur at spacecraft or instrument level, but also due to failures in the ground-to-spacecraft link or the ground segment itself. The adverse effects of such anomalies may be the loss of scientific data corresponding to one or several planned pointings, which have not been acquired and/or stored in memory.<br />
<br />
Failure to acquire proper scientific data may occur to one or both instruments.<br />
<br />
When a gap occurred, scientific criteria were applied to decide whether to recover the data through the Small-Gap Recovery procedure.<br />
<br />
[[File:AHF_353_OD389.png|thumb|400px|Integration time of the 353 GHz detectors ({{PlanckPapers|lamarre2010}}) after 389 Operational Days (the unit is seconds per square degree, normalized to one detector). The first significant data gap and recovery are clearly visible.]]<br />
<br />
The Small-Gap Recovery (SGR) procedure could be applied by MOC or PSO.<br />
<br />
* '''MOC-triggered SGR''': Within its nominal scheduling procedure for an OD, the MOC searches the PPL for PREF corresponding to the OD being processed and any pointings which are the subject of a Small Gap Recovery. As the PREF are sorted in chronological order according to their nominal start time, those corresponding to a small gap will naturally be the earliest. After checking attitude constraints, all observable pointings are listed and their dwell times reduced (initially) to the Minimum Dwell Time (MDT), as given in the PPL.<br />
Having included all valid PREF the required slew times are calculated. With the required slew times and minimum dwell times for all pointings, the OD schedule may be under-populated; in this case the dwell times of all scheduled pointings will be increased equally to make use of all available time in the OD. If the resulting schedule is over-populated, even with MDT for all pointings, the recovery cannot be constrained to a single OD. The sequence of pointings for the ODs involved is optimized in PREF scheduling and dwell times determined in order to effect the recovery and revert to the nominal timeline as quickly as possible.<br />
<br />
* '''PSO-triggered SGR''':<br />
PSO declares a small gap when pointings that have been executed result in data of insufficient quality or inadequate frequency coverage. This assessment is based on data quality and instrument health information provided by the DPCs. The algorithm that was used by the PSO to check the scientific validity of a pointing was implemented within the SPPT software tool. The SPPT ingested on a weekly basis a Weekly Health Report (WHR) for the HFI and LFI containing information on the working status of each detector and their expected condition over the following four weeks. On a daily basis, a Daily Quality Report (DQR) provided by the DPCs for both instruments, included a set of parameters that described the quality of the detection achieved by each individual detector for every pointing executed.<br />
<br />
The scheme for declaring a Small-Gap Recovery from PSO is the following.<br />
<br />
- If a pointing fails to meet the chosen requirement, it becomes an SGR candidate.<br />
<br />
- If there are at least 12 consecutive pointings which are declared SGR candidates, and the problem has been identified and solved, then an SGR is triggered.<br />
Recoveries are only carried out if the recovery slewing is guaranteed to be in OCM. MOC carried out this analysis and decided whether they should perform the SGR accordingly.<br />
<br />
- The start and end times of the gap and the list of the pointing numbers (or just the numbers of the first and last pointings to be recovered) were then sent to MOC by E-mail, with the notification to start a Small-Gap Recovery.<br />
<br />
- MOC implemented the Small-Gap Recovery, provided the pointings could still be scheduled with respect to their latest start time, using the same scheme as described in the MOC-triggered SGR section<br />
<br />
Throughout the Planck mission, data losses were very rare. In fact Small-Gap Recovery was applied only a couple of times.<br />
<br />
==Special observations==<br />
The special observations are now described.<br />
<br />
* Normal scanning on Solar System objects for calibration purposes.<br />
<br />
[[File:Crab_Nebula.jpg|thumb|200px|The Crab Nebula (Messier 1, NGC 1952, Taurus A), here seen by the Hubble Space Telescope.]]<br />
<br />
[[File:Mars.jpg|thumb|200px|Mars as seen by the Hubble Space Telescope in 1999.]]<br />
<br />
This concerns the following objects (specifically planets): Mars; Jupiter; Saturn; Uranus; and Neptune. Their thermal emission in the far-infrared and the small angular sizes make them ideal calibrators for bolometers and radiometers.<br />
<br />
Mars is a particularly interesting calibrator for Planck, because of its proper motion.<br />
However this proper motion makes it difficult to observe it many times during the mission.<br />
<br />
Jupiter is the brightest source for (non-polarized) calibration. Saturn was also used significantly, with Uranus and Neptune being secondary calibrators.<br />
<br />
* Normal scanning on other (non-moving) sources for calibration purposes.<br />
<br />
This concerns mostly the Crab Nebula for polarization calibration purposes.<br />
This supernova remnant is highly polarized, and as such represents the main polarization calibrator for Planck.<br />
<br />
* Special pointings during the calibration phase, not relative to celestial sources.<br />
<br />
* "Deep rings," special observations that were performed on each passage of Jupiter and the Crab Nebula, from January 2012 onward.<br />
<br />
These consist of very deeply sampled observations (0.5') with the spin axis along the Ecliptic plane, typically lasting two to three weeks.<br />
<br />
Such observations benefit from special relaxing of the celestial constraints, with Solar Aspect Angles < 9 deg. rather than < 8 deg. during cycloidal surveying.<br />
<br />
* "Drift scans," special observations performed on Mars, making use of its proper motion.<br />
<br />
==Start and end of surveys==<br />
<br />
The completion of a given “survey” is declared when the logical AND of all frequency-coverage maps is greater than 95 %, OR the sky has been surveyed over a consecutive period of 7.5 months. Note that this definition is that of the Project Scientist and Planck Science Office. Data processing centres do not use exactly the same concept of surveys to create "survey" maps.<br />
<br />
In practice, since the gaps during the surveys have always been very small, this results in approximately 6 months per survey.<br />
<br />
[[File:PlanckMissionTimeline.JPG|thumb|300px|Planck mission timeline with the distribution of the "sky surveys".]]<br />
<br />
* '''Survey 1''': starts 13 August 2009, ends 13 February 2010.<br />
<br />
* '''Survey 2''': starts 14 February 2010, ends 13 August 2010.<br />
<br />
* '''Survey 3''': starts 14 August 2010, ends 13 February 2011.<br />
<br />
* '''Survey 4''': starts 14 February 2011, ends 29 July 2011.<br />
<br />
(This survey was shortened in ordered to start earlier with the new scanning strategy; see above).<br />
<br />
* '''Survey 5''': starts 29 July 2011, ends 30 January 2012.<br />
<br />
* '''Survey 6''' (LFI only): starts 30 January 2012, ends 31 July 2012.<br />
<br />
* '''Survey 7''' (LFI only): starts 31 July 2012, ends 31 January 2013.<br />
<br />
* '''Survey 8''' (LFI only): starts 1 February 2013, ends 1 August 2013.<br />
<br />
<br />
=== Completion of full sky coverage during Surveys 1-2 ===<br />
<br />
The picture gallery below exhibits the progress of sky coverage during the first months of survey (black colour = unobserved areas).<br />
<br />
<br />
<gallery widths=330 perrow=3 caption="HFI 353 GHz integration time after N months of survey. The units here are seconds per square degree, normalized to one detector."><br />
File:353_1month.png|After 1 month<br />
File:353_2month.png|After 2 months<br />
File:353_3month.png|After 3 months<br />
File:353_4month.png|After 4 months<br />
File:353_5month.png|After 5 months<br />
File:353_6month.png|After 6 months<br />
File:353_7month.png|After 7 months<br />
File:353_8month.png|After 8 months<br />
File:353_9months.png|After 9 months<br />
File:353_10months.png|After 10 months<br />
File:353_11months.png|After 11 months<br />
File:353_12months.png|After 12 months<br />
</gallery><br />
<br />
== Main planet and Crab observations ==<br />
<br />
Solar System objects and the Crab Nebula have been observed many times during the Planck surveys. Here is a list of these observations, with the ''deep rings'' (Jupiter and the Crab) and ''drift scans'' (Mars only) in '''boldface'''.<br />
<br />
* Crab: 16-22 September 2009<br />
<br />
* Mars: 17-29 October 2009<br />
<br />
* Jupiter: 25 October – 1 November 2009<br />
<br />
* Neptune: 1-8 November 2009<br />
<br />
* Uranus: 6-16 December 2009<br />
<br />
* Saturn: 2-8 January 2010<br />
<br />
* Crab: 6-12 March 2010<br />
<br />
* Mars: 9-18 April 2010<br />
<br />
* Neptune: 15-23 May 2010<br />
<br />
* Saturn: 13-22 June 2010<br />
<br />
* Uranus: 27 June – 5 July 2010<br />
<br />
* Jupiter: 1-9 July 2010<br />
<br />
* Crab: 15-21 September 2010<br />
<br />
* Neptune: 3-11 November 2010<br />
<br />
* Jupiter: 9-18 December 2010<br />
<br />
* Uranus: 12-21 December 2010<br />
<br />
* Saturn: 15-22 January 2011<br />
<br />
* Crab: 7-12 March 2011<br />
<br />
* Neptune: 18-26 May 2011<br />
<br />
* Saturn: 30 June - 9 July 2011<br />
<br />
* Uranus: 3-11 July 2011<br />
<br />
* Jupiter: 9-15 August 2011<br />
<br />
* Crab: 10-18 September 2011 (performed with the 250 deg. phase cycloidal strategy)<br />
<br />
* Crab: 20-23 September 2011 (performed with the 340 deg. phase cycloidal strategy)<br />
<br />
* '''Mars''': 8-16 December 2011 ("drift scan", Mars allowed to move through the Planck focal plane via its proper motion)<br />
<br />
* Mars: 17-26 December 2011 (normal scanning)<br />
<br />
* '''Jupiter''': 8-30 January 2012 (deep ring)<br />
<br />
* '''Crab''': 26 February - 16 March 2012 (deep ring)<br />
<br />
* '''Jupiter''': 1-14 September 2012 (deep ring)<br />
<br />
* '''Crab''': 14 September - 1 October 2012 (deep ring)<br />
<br />
* Neptune: 19-27 November 2012<br />
<br />
* Uranus: 24-30 December 2012<br />
<br />
* Saturn: 30 January - 5 February 2013<br />
<br />
* '''Jupiter''': February 2013 (deep ring)<br />
<br />
* '''Crab''': Feb. 28th - March 15th, 2013 (deep ring)<br />
<br />
* Neptune: June 4th - June 12th, 2013<br />
<br />
* Uranus: July 9-16th, 2013<br />
<br />
* Saturn: July 20-26th, 2013<br />
<br />
* '''Crab''': Sept. 10th - Oct. 3rd, 2013 (deep ring)<br />
<br />
== Resulting integration time distribution ==<br />
<br />
The integration time after the end of HFI operations (January 2012) is shown in the following picture gallery.<br />
<br />
Units are seconds per square degree, normalized to one detector, for all maps. The projection is full-sky Mollweide centred on the Galactic centre.<br />
<br />
<br />
<br />
<gallery widths=330px perrow=3 caption="Integration time after the end of HFI operations (January 2012). The units here are seconds per square degree, normalized to one detector."><br />
File:HFI_fullmission_100GHz1-4.png|HFI 100 GHz 1,4<br />
File:HFI_fullmission_100GHz2-3.png|HFI 100 GHz 2,3<br />
File:HFI_fullmission_143GHz1-4.png|HFI 143 GHz 1-4<br />
File:HFI_fullmission_143GHz5-8.png|HFI 143 GHz 5-8<br />
File:HFI_fullmission_217GHz1-4.png|HFI 217 GHz 1-4<br />
File:HFI_fullmission_217GHz5-8.png|HFI 217 GHz 5-8<br />
File:HFI_fullmission_353GHz.png|HFI 353 GHz<br />
File:HFI_fullmission_545-857GHz.png|HFI 545 GHz / 857 GHz<br />
File:LFI25_coldmission.png|LFI-25 (44 GHz)<br />
File:LFI27_coldmission.png|LFI 30 GHz<br />
</gallery><br />
<br />
==References==<br />
<references /><br />
<br />
[[Category:Introduction|004]]<br />
[[Category:PSOBook]]</div>
Xdupac
https://wiki.cosmos.esa.int/planckpla2015/index.php?title=Survey_scanning_and_performance&diff=11016
Survey scanning and performance
2015-02-03T16:20:26Z
<p>Xdupac: /* Main planet and Crab observations */</p>
<hr />
<div>== The observation strategy ==<br />
<br />
The Planck ''observation strategy'', or ''scanning strategy'', made use of the characteristics of the Planck spacecraft {{PlanckPapers|planck2011-1-1}} and orbit in order to achieve the survey goals in terms of sky coverage and scanning directions.<br />
<br />
The Planck focal plane scanned the sky in the way explained in the figure below.<br />
<br />
[[file:FocalPlane.png|thumb|300px|Planck focal plane showing the direction of scanning. Polarization-sensitive detectors are drawn with crosses indicating the polarization orientation.]]<br />
<br />
The 353 GHz row scanned the sky in small circles with an 85 deg. bore-sight angle from the spin axis. 545 GHz, 857 GHz, and 143 GHz bolometers, as well as LFI radiometers 25 and 26 had a slightly smaller bore-sight angle, while the other part of the Planck focal plane had larger ones (up to about 89 deg.). The Planck spacecraft spun at a rate of 1 rpm.<br />
<br />
Planck, being at L2, moved along the Ecliptic at approximately one degree per day, and needed to keep the Solar aspect angle below about 9 degrees at all times. In practice, during the surveys, the limit considered was 8 deg. Another celestial constraint is that the angle between the Planck spin axis and the anti-Earth direction could not exceed 15 deg. (relaxed to 17 deg. from Survey 5 onward). These constraints had a very direct influence on the chosen scanning strategy.<br />
<br />
[[File:ScannStrategy.png|thumb|300px|Simplified illustration of the Planck scanning strategy, without additional motion of the spin axis.]]<br />
<br />
[[File:Observing_strat.png|thumb|300px|left|Planck scanning strategy, showing the additional motion of the spin axis.]]<br />
<br />
The path followed by the Planck spin axis was defined with respect to the Ecliptic plane. It corresponded to a motion in longitude which maintained an anti-Sun pointing (about one degree per day), to which was added a cycloidal motion (precession) of the spin axis around the anti-Sun position (fiducial point). The cycloidal path was defined by the functions: <br />
<br />
$ λ = θ sin((-1)^n ω (t-t_0)+φ) $ (eq. 1),<br />
<br />
$β = -θ cos((-1)^n ω(t-t_0) + φ) $ (eq. 2),<br />
<br />
where λ is the angular distance from the fiducial point in Ecliptic longitude, β the angular distance from the fiducial point in Ecliptic latitude, θ the spin axis precession amplitude, ω the pulsation of the precession, φ its phase, n the parameter which controls the motion direction of the precession, t is the time, and $t_0$ is the first time during the Planck survey at which the fiducial point crosses the Ecliptic longitude =0 line.<br />
<br />
[[File:Cycloidal_scanning.JPG|thumb|300px|Spin axis path with a 7 deg. amplitude cycloidal scanning, from Ref.{{BibCite|dupac2005}}]]<br />
<br />
The reasons to decide to use such a precession of the spin axis are the following.<br />
<br />
* An excursion of the spin axis from the anti-Sun direction is required to fully observe the whole sky (no excursion would leave a large area unobserved around the Ecliptic poles).<br />
<br />
* The precession motion keeps the Sun aspect angle constant during the whole survey, therefore minimizing the thermal constraint variations on the spacecraft.<br />
<br />
The following precession parameters were chosen for the BSS.<br />
<br />
* Amplitude θ = 7.5deg. (this value is the lowest possible which allows the whole sky to be covered with all detectors).<br />
<br />
* n = 1 (anti-clockwise motion as seen from the Sun).<br />
<br />
* Pulsation ω = 2π / (half a year), faster precession was considered, and has interesting advantages, but was not possible given the constraints if one wants to keep a 7.5 deg. amplitude (which is necessary to cover the whole sky).<br />
<br />
* The phase of the precession was decided according to this set of criteria (in order of importance):<br />
<br />
a) respecting the operational constraints;<br />
<br />
b) allowing the largest possible angle between two scans on the Crab Nebula (a polarization calibrator);<br />
<br />
c) avoiding null dipole amplitude for the whole mission;<br />
<br />
d) optimizing the position of the planets in the beginning of the survey and with respect to the feasibility of their recovery;<br />
<br />
e) placing the two “deep fields” where Galactic foregrounds are minimum;<br />
<br />
f) allowing a reasonable survey margin (i.e. the time allowed to recover lost pointings if a problem occurs).<br />
<br />
The phase is 340 deg. for Surveys 1 to 4, and 250 deg. for Surveys 5 to 8.<br />
<br />
The scanning strategy for the second year of Routine Operations (i.e. Surveys 3 and 4) was exactly the same as for the first year, except that all pointings were shifted by 1 arcmin along the cross-scanning direction, in order to provide finer sky sampling for the highest frequency detectors when combining two years of observations.<br />
<br />
The change of phase between Survey 4 and Survey 5 occurred because it was found essential (especially on the HFI side) that scanning direction crossings should be increased in the Planck survey. By choosing a phase 90 deg. away from the original one, one optimizes the scanning strategy in this respect.<br />
<br />
The details of the justifications for these parameters can be found in PL-WG9-TN-001.<br />
<br />
The scanning strategy parameters are input to the PSO Survey Planning and Performance Tool, which is the software which generates the series of pointing records to be sent out to MOC for implementation.<br />
<br />
An approximate visualization of the Planck scanning strategy can be found [http://www.youtube.com/watch?v=WwFXuZ0B3B8 here] and [http://www.youtube.com/watch?v=7Zu-aiEiDtY here].<br />
<br />
<br />
===Spin axis manoeuvres and exact pointings===<br />
The motion of the spin axis was not continuous. Every change in the spin axis position was initiated by a manoeuvre which required less than 5 minutes time to complete. <br />
<br />
The duration between spin-axis manoeuvres is hereafter referred to as the “dwelling time" and the angular distance between manoeuvres along the spin axis path is hereafter referred to as the “spacing”. <br />
<br />
The dwelling times and spacings are defined as follows:<br />
<br />
* the spacings are fixed to 2arcmin, which roughly corresponds to the Nyquist criterion for sampling the highest-frequency HFI detectors;<br />
<br />
* the dwell times vary from 2360 s to 3904 s.<br />
The exact series of coordinates and dwell times are set by Eqs. (1) and (2) when one has fixed the spacings.<br />
<br />
== Data gap recoveries ==<br />
<br />
Gaps in the data flow can occur for various reasons.<br />
<br />
Anomalies may occur at spacecraft or instrument level, but also due to failures in the ground-to-spacecraft link or the ground segment itself. The adverse effects of such anomalies may be the loss of scientific data corresponding to one or several planned pointings, which have not been acquired and/or stored in memory.<br />
<br />
Failure to acquire proper scientific data may occur to one or both instruments.<br />
<br />
When a gap occurred, scientific criteria were applied to decide whether to recover the data through the Small-Gap Recovery procedure.<br />
<br />
[[File:AHF_353_OD389.png|thumb|400px|Integration time of the 353 GHz detectors ({{PlanckPapers|lamarre2010}}) after 389 Operational Days (the unit is seconds per square degree, normalized to one detector). The first significant data gap and recovery are clearly visible.]]<br />
<br />
The Small-Gap Recovery (SGR) procedure could be applied by MOC or PSO.<br />
<br />
* '''MOC-triggered SGR''': Within its nominal scheduling procedure for an OD, the MOC searches the PPL for PREF corresponding to the OD being processed and any pointings which are the subject of a Small Gap Recovery. As the PREF are sorted in chronological order according to their nominal start time, those corresponding to a small gap will naturally be the earliest. After checking attitude constraints, all observable pointings are listed and their dwell times reduced (initially) to the Minimum Dwell Time (MDT), as given in the PPL.<br />
Having included all valid PREF the required slew times are calculated. With the required slew times and minimum dwell times for all pointings, the OD schedule may be under-populated; in this case the dwell times of all scheduled pointings will be increased equally to make use of all available time in the OD. If the resulting schedule is over-populated, even with MDT for all pointings, the recovery cannot be constrained to a single OD. The sequence of pointings for the ODs involved is optimized in PREF scheduling and dwell times determined in order to effect the recovery and revert to the nominal timeline as quickly as possible.<br />
<br />
* '''PSO-triggered SGR''':<br />
PSO declares a small gap when pointings that have been executed result in data of insufficient quality or inadequate frequency coverage. This assessment is based on data quality and instrument health information provided by the DPCs. The algorithm that was used by the PSO to check the scientific validity of a pointing was implemented within the SPPT software tool. The SPPT ingested on a weekly basis a Weekly Health Report (WHR) for the HFI and LFI containing information on the working status of each detector and their expected condition over the following four weeks. On a daily basis, a Daily Quality Report (DQR) provided by the DPCs for both instruments, included a set of parameters that described the quality of the detection achieved by each individual detector for every pointing executed.<br />
<br />
The scheme for declaring a Small-Gap Recovery from PSO is the following.<br />
<br />
- If a pointing fails to meet the chosen requirement, it becomes an SGR candidate.<br />
<br />
- If there are at least 12 consecutive pointings which are declared SGR candidates, and the problem has been identified and solved, then an SGR is triggered.<br />
Recoveries are only carried out if the recovery slewing is guaranteed to be in OCM. MOC carried out this analysis and decided whether they should perform the SGR accordingly.<br />
<br />
- The start and end times of the gap and the list of the pointing numbers (or just the numbers of the first and last pointings to be recovered) were then sent to MOC by E-mail, with the notification to start a Small-Gap Recovery.<br />
<br />
- MOC implemented the Small-Gap Recovery, provided the pointings could still be scheduled with respect to their latest start time, using the same scheme as described in the MOC-triggered SGR section<br />
<br />
Throughout the Planck mission, data losses were very rare. In fact Small-Gap Recovery was applied only a couple of times.<br />
<br />
==Special observations==<br />
The special observations are now described.<br />
<br />
* Normal scanning on Solar System objects for calibration purposes.<br />
<br />
[[File:Crab_Nebula.jpg|thumb|200px|The Crab Nebula (Messier 1, NGC 1952, Taurus A), here seen by the Hubble Space Telescope.]]<br />
<br />
[[File:Mars.jpg|thumb|200px|Mars as seen by the Hubble Space Telescope in 1999.]]<br />
<br />
This concerns the following objects (specifically planets): Mars; Jupiter; Saturn; Uranus; and Neptune. Their thermal emission in the far-infrared and the small angular sizes make them ideal calibrators for bolometers and radiometers.<br />
<br />
Mars is a particularly interesting calibrator for Planck, because of its proper motion.<br />
However this proper motion makes it difficult to observe it many times during the mission.<br />
<br />
Jupiter is the brightest source for (non-polarized) calibration. Saturn was also used significantly, with Uranus and Neptune being secondary calibrators.<br />
<br />
* Normal scanning on other (non-moving) sources for calibration purposes.<br />
<br />
This concerns mostly the Crab Nebula for polarization calibration purposes.<br />
This supernova remnant is highly polarized, and as such represents the main polarization calibrator for Planck.<br />
<br />
* Special pointings during the calibration phase, not relative to celestial sources.<br />
<br />
* "Deep rings," special observations that were performed on each passage of Jupiter and the Crab Nebula, from January 2012 onward.<br />
<br />
These consist of very deeply sampled observations (0.5') with the spin axis along the Ecliptic plane, typically lasting two to three weeks.<br />
<br />
Such observations benefit from special relaxing of the celestial constraints, with Solar Aspect Angles < 9 deg. rather than < 8 deg. during cycloidal surveying.<br />
<br />
* "Drift scans," special observations performed on Mars, making use of its proper motion.<br />
<br />
==Start and end of surveys==<br />
<br />
The completion of a given “survey” is declared when the logical AND of all frequency-coverage maps is greater than 95 %, OR the sky has been surveyed over a consecutive period of 7.5 months. Note that this definition is that of the Project Scientist and Planck Science Office. Data processing centres do not use exactly the same concept of surveys to create "survey" maps.<br />
<br />
In practice, since the gaps during the surveys have always been very small, this results in approximately 6 months per survey.<br />
<br />
[[File:PlanckMissionTimeline.JPG|thumb|300px|Planck mission timeline with the distribution of the "sky surveys".]]<br />
<br />
* '''Survey 1''': starts 13 August 2009, ends 13 February 2010.<br />
<br />
* '''Survey 2''': starts 14 February 2010, ends 13 August 2010.<br />
<br />
* '''Survey 3''': starts 14 August 2010, ends 13 February 2011.<br />
<br />
* '''Survey 4''': starts 14 February 2011, ends 29 July 2011.<br />
<br />
(This survey was shortened in ordered to start earlier with the new scanning strategy; see above).<br />
<br />
* '''Survey 5''': starts 29 July 2011, ends 30 January 2012.<br />
<br />
* '''Survey 6''' (LFI only): starts 30 January 2012, ends 31 July 2012.<br />
<br />
* '''Survey 7''' (LFI only): starts 31 July 2012, ends 31 January 2013.<br />
<br />
* '''Survey 8''' (LFI only): starts 1 February 2013, ends 1 August 2013.<br />
<br />
<br />
=== Completion of full sky coverage during Surveys 1-2 ===<br />
<br />
The picture gallery below exhibits the progress of sky coverage during the first months of survey (black colour = unobserved areas).<br />
<br />
<br />
<gallery widths=330 perrow=3 caption="HFI 353 GHz integration time after N months of survey. The units here are seconds per square degree, normalized to one detector."><br />
File:353_1month.png|After 1 month<br />
File:353_2month.png|After 2 months<br />
File:353_3month.png|After 3 months<br />
File:353_4month.png|After 4 months<br />
File:353_5month.png|After 5 months<br />
File:353_6month.png|After 6 months<br />
File:353_7month.png|After 7 months<br />
File:353_8month.png|After 8 months<br />
File:353_9months.png|After 9 months<br />
File:353_10months.png|After 10 months<br />
File:353_11months.png|After 11 months<br />
File:353_12months.png|After 12 months<br />
</gallery><br />
<br />
== Main planet and Crab observations ==<br />
<br />
Solar System objects and the Crab Nebula have been observed many times during the Planck surveys. Here is a list of these observations, with the ''deep rings'' (Jupiter and the Crab) and ''drift scans'' (Mars only) in '''boldface'''.<br />
<br />
* Crab: 16-22 September 2009<br />
<br />
* Mars: 17-29 October 2009<br />
<br />
* Jupiter: 25 October – 1 November 2009<br />
<br />
* Neptune: 1-8 November 2009<br />
<br />
* Uranus: 6-16 December 2009<br />
<br />
* Saturn: 2-8 January 2010<br />
<br />
* Crab: 6-12 March 2010<br />
<br />
* Mars: 9-18 April 2010<br />
<br />
* Neptune: 15-23 May 2010<br />
<br />
* Saturn: 13-22 June 2010<br />
<br />
* Uranus: 27 June – 5 July 2010<br />
<br />
* Jupiter: 1-9 July 2010<br />
<br />
* Crab: 15-21 September 2010<br />
<br />
* Neptune: 3-11 November 2010<br />
<br />
* Jupiter: 9-18 December 2010<br />
<br />
* Uranus: 12-21 December 2010<br />
<br />
* Saturn: 15-22 January 2011<br />
<br />
* Crab: 7-12 March 2011<br />
<br />
* Neptune: 18-26 May 2011<br />
<br />
* Saturn: 30 June - 9 July 2011<br />
<br />
* Uranus: 3-11 July 2011<br />
<br />
* Jupiter: 9-15 August 2011<br />
<br />
* Crab: 10-18 September 2011 (performed with the 250 deg. phase cycloidal strategy)<br />
<br />
* Crab: 20-23 September 2011 (performed with the 340 deg. phase cycloidal strategy)<br />
<br />
* '''Mars''': 8-16 December 2011 ("drift scan", Mars allowed to move through the Planck focal plane via its proper motion)<br />
<br />
* Mars: 17-26 December 2011 (normal scanning)<br />
<br />
* '''Jupiter''': 8-30 January 2012 (deep ring)<br />
<br />
* '''Crab''': 26 February - 16 March 2012 (deep ring)<br />
<br />
* '''Jupiter''': 1-14 September 2012 (deep ring)<br />
<br />
* '''Crab''': 14 September - 1 October 2012 (deep ring)<br />
<br />
* Neptune: 19-27 November 2012<br />
<br />
* Uranus: 24-30 December 2012<br />
<br />
* Saturn: 30 January - 5 February 2013<br />
<br />
* '''Jupiter''': February 2013 (deep ring)<br />
<br />
* '''Crab''': Feb. 28th - March 15th, 2013 (deep ring)<br />
<br />
* Neptune: June 4th - June 12th, 2013<br />
<br />
* Uranus: July 9-16th, 2013<br />
<br />
* Saturn: July 20-26th, 2013<br />
<br />
== Resulting integration time distribution ==<br />
<br />
The integration time after the end of HFI operations (January 2012) is shown in the following picture gallery.<br />
<br />
Units are seconds per square degree, normalized to one detector, for all maps. The projection is full-sky Mollweide centred on the Galactic centre.<br />
<br />
<br />
<br />
<gallery widths=330px perrow=3 caption="Integration time after the end of HFI operations (January 2012). The units here are seconds per square degree, normalized to one detector."><br />
File:HFI_fullmission_100GHz1-4.png|HFI 100 GHz 1,4<br />
File:HFI_fullmission_100GHz2-3.png|HFI 100 GHz 2,3<br />
File:HFI_fullmission_143GHz1-4.png|HFI 143 GHz 1-4<br />
File:HFI_fullmission_143GHz5-8.png|HFI 143 GHz 5-8<br />
File:HFI_fullmission_217GHz1-4.png|HFI 217 GHz 1-4<br />
File:HFI_fullmission_217GHz5-8.png|HFI 217 GHz 5-8<br />
File:HFI_fullmission_353GHz.png|HFI 353 GHz<br />
File:HFI_fullmission_545-857GHz.png|HFI 545 GHz / 857 GHz<br />
File:LFI25_coldmission.png|LFI-25 (44 GHz)<br />
File:LFI27_coldmission.png|LFI 30 GHz<br />
</gallery><br />
<br />
==References==<br />
<references /><br />
<br />
[[Category:Introduction|004]]<br />
[[Category:PSOBook]]</div>
Xdupac
https://wiki.cosmos.esa.int/planckpla2015/index.php?title=Survey_scanning_and_performance&diff=11015
Survey scanning and performance
2015-02-03T16:18:55Z
<p>Xdupac: /* Main planet and Crab observations */</p>
<hr />
<div>== The observation strategy ==<br />
<br />
The Planck ''observation strategy'', or ''scanning strategy'', made use of the characteristics of the Planck spacecraft {{PlanckPapers|planck2011-1-1}} and orbit in order to achieve the survey goals in terms of sky coverage and scanning directions.<br />
<br />
The Planck focal plane scanned the sky in the way explained in the figure below.<br />
<br />
[[file:FocalPlane.png|thumb|300px|Planck focal plane showing the direction of scanning. Polarization-sensitive detectors are drawn with crosses indicating the polarization orientation.]]<br />
<br />
The 353 GHz row scanned the sky in small circles with an 85 deg. bore-sight angle from the spin axis. 545 GHz, 857 GHz, and 143 GHz bolometers, as well as LFI radiometers 25 and 26 had a slightly smaller bore-sight angle, while the other part of the Planck focal plane had larger ones (up to about 89 deg.). The Planck spacecraft spun at a rate of 1 rpm.<br />
<br />
Planck, being at L2, moved along the Ecliptic at approximately one degree per day, and needed to keep the Solar aspect angle below about 9 degrees at all times. In practice, during the surveys, the limit considered was 8 deg. Another celestial constraint is that the angle between the Planck spin axis and the anti-Earth direction could not exceed 15 deg. (relaxed to 17 deg. from Survey 5 onward). These constraints had a very direct influence on the chosen scanning strategy.<br />
<br />
[[File:ScannStrategy.png|thumb|300px|Simplified illustration of the Planck scanning strategy, without additional motion of the spin axis.]]<br />
<br />
[[File:Observing_strat.png|thumb|300px|left|Planck scanning strategy, showing the additional motion of the spin axis.]]<br />
<br />
The path followed by the Planck spin axis was defined with respect to the Ecliptic plane. It corresponded to a motion in longitude which maintained an anti-Sun pointing (about one degree per day), to which was added a cycloidal motion (precession) of the spin axis around the anti-Sun position (fiducial point). The cycloidal path was defined by the functions: <br />
<br />
$ λ = θ sin((-1)^n ω (t-t_0)+φ) $ (eq. 1),<br />
<br />
$β = -θ cos((-1)^n ω(t-t_0) + φ) $ (eq. 2),<br />
<br />
where λ is the angular distance from the fiducial point in Ecliptic longitude, β the angular distance from the fiducial point in Ecliptic latitude, θ the spin axis precession amplitude, ω the pulsation of the precession, φ its phase, n the parameter which controls the motion direction of the precession, t is the time, and $t_0$ is the first time during the Planck survey at which the fiducial point crosses the Ecliptic longitude =0 line.<br />
<br />
[[File:Cycloidal_scanning.JPG|thumb|300px|Spin axis path with a 7 deg. amplitude cycloidal scanning, from Ref.{{BibCite|dupac2005}}]]<br />
<br />
The reasons to decide to use such a precession of the spin axis are the following.<br />
<br />
* An excursion of the spin axis from the anti-Sun direction is required to fully observe the whole sky (no excursion would leave a large area unobserved around the Ecliptic poles).<br />
<br />
* The precession motion keeps the Sun aspect angle constant during the whole survey, therefore minimizing the thermal constraint variations on the spacecraft.<br />
<br />
The following precession parameters were chosen for the BSS.<br />
<br />
* Amplitude θ = 7.5deg. (this value is the lowest possible which allows the whole sky to be covered with all detectors).<br />
<br />
* n = 1 (anti-clockwise motion as seen from the Sun).<br />
<br />
* Pulsation ω = 2π / (half a year), faster precession was considered, and has interesting advantages, but was not possible given the constraints if one wants to keep a 7.5 deg. amplitude (which is necessary to cover the whole sky).<br />
<br />
* The phase of the precession was decided according to this set of criteria (in order of importance):<br />
<br />
a) respecting the operational constraints;<br />
<br />
b) allowing the largest possible angle between two scans on the Crab Nebula (a polarization calibrator);<br />
<br />
c) avoiding null dipole amplitude for the whole mission;<br />
<br />
d) optimizing the position of the planets in the beginning of the survey and with respect to the feasibility of their recovery;<br />
<br />
e) placing the two “deep fields” where Galactic foregrounds are minimum;<br />
<br />
f) allowing a reasonable survey margin (i.e. the time allowed to recover lost pointings if a problem occurs).<br />
<br />
The phase is 340 deg. for Surveys 1 to 4, and 250 deg. for Surveys 5 to 8.<br />
<br />
The scanning strategy for the second year of Routine Operations (i.e. Surveys 3 and 4) was exactly the same as for the first year, except that all pointings were shifted by 1 arcmin along the cross-scanning direction, in order to provide finer sky sampling for the highest frequency detectors when combining two years of observations.<br />
<br />
The change of phase between Survey 4 and Survey 5 occurred because it was found essential (especially on the HFI side) that scanning direction crossings should be increased in the Planck survey. By choosing a phase 90 deg. away from the original one, one optimizes the scanning strategy in this respect.<br />
<br />
The details of the justifications for these parameters can be found in PL-WG9-TN-001.<br />
<br />
The scanning strategy parameters are input to the PSO Survey Planning and Performance Tool, which is the software which generates the series of pointing records to be sent out to MOC for implementation.<br />
<br />
An approximate visualization of the Planck scanning strategy can be found [http://www.youtube.com/watch?v=WwFXuZ0B3B8 here] and [http://www.youtube.com/watch?v=7Zu-aiEiDtY here].<br />
<br />
<br />
===Spin axis manoeuvres and exact pointings===<br />
The motion of the spin axis was not continuous. Every change in the spin axis position was initiated by a manoeuvre which required less than 5 minutes time to complete. <br />
<br />
The duration between spin-axis manoeuvres is hereafter referred to as the “dwelling time" and the angular distance between manoeuvres along the spin axis path is hereafter referred to as the “spacing”. <br />
<br />
The dwelling times and spacings are defined as follows:<br />
<br />
* the spacings are fixed to 2arcmin, which roughly corresponds to the Nyquist criterion for sampling the highest-frequency HFI detectors;<br />
<br />
* the dwell times vary from 2360 s to 3904 s.<br />
The exact series of coordinates and dwell times are set by Eqs. (1) and (2) when one has fixed the spacings.<br />
<br />
== Data gap recoveries ==<br />
<br />
Gaps in the data flow can occur for various reasons.<br />
<br />
Anomalies may occur at spacecraft or instrument level, but also due to failures in the ground-to-spacecraft link or the ground segment itself. The adverse effects of such anomalies may be the loss of scientific data corresponding to one or several planned pointings, which have not been acquired and/or stored in memory.<br />
<br />
Failure to acquire proper scientific data may occur to one or both instruments.<br />
<br />
When a gap occurred, scientific criteria were applied to decide whether to recover the data through the Small-Gap Recovery procedure.<br />
<br />
[[File:AHF_353_OD389.png|thumb|400px|Integration time of the 353 GHz detectors ({{PlanckPapers|lamarre2010}}) after 389 Operational Days (the unit is seconds per square degree, normalized to one detector). The first significant data gap and recovery are clearly visible.]]<br />
<br />
The Small-Gap Recovery (SGR) procedure could be applied by MOC or PSO.<br />
<br />
* '''MOC-triggered SGR''': Within its nominal scheduling procedure for an OD, the MOC searches the PPL for PREF corresponding to the OD being processed and any pointings which are the subject of a Small Gap Recovery. As the PREF are sorted in chronological order according to their nominal start time, those corresponding to a small gap will naturally be the earliest. After checking attitude constraints, all observable pointings are listed and their dwell times reduced (initially) to the Minimum Dwell Time (MDT), as given in the PPL.<br />
Having included all valid PREF the required slew times are calculated. With the required slew times and minimum dwell times for all pointings, the OD schedule may be under-populated; in this case the dwell times of all scheduled pointings will be increased equally to make use of all available time in the OD. If the resulting schedule is over-populated, even with MDT for all pointings, the recovery cannot be constrained to a single OD. The sequence of pointings for the ODs involved is optimized in PREF scheduling and dwell times determined in order to effect the recovery and revert to the nominal timeline as quickly as possible.<br />
<br />
* '''PSO-triggered SGR''':<br />
PSO declares a small gap when pointings that have been executed result in data of insufficient quality or inadequate frequency coverage. This assessment is based on data quality and instrument health information provided by the DPCs. The algorithm that was used by the PSO to check the scientific validity of a pointing was implemented within the SPPT software tool. The SPPT ingested on a weekly basis a Weekly Health Report (WHR) for the HFI and LFI containing information on the working status of each detector and their expected condition over the following four weeks. On a daily basis, a Daily Quality Report (DQR) provided by the DPCs for both instruments, included a set of parameters that described the quality of the detection achieved by each individual detector for every pointing executed.<br />
<br />
The scheme for declaring a Small-Gap Recovery from PSO is the following.<br />
<br />
- If a pointing fails to meet the chosen requirement, it becomes an SGR candidate.<br />
<br />
- If there are at least 12 consecutive pointings which are declared SGR candidates, and the problem has been identified and solved, then an SGR is triggered.<br />
Recoveries are only carried out if the recovery slewing is guaranteed to be in OCM. MOC carried out this analysis and decided whether they should perform the SGR accordingly.<br />
<br />
- The start and end times of the gap and the list of the pointing numbers (or just the numbers of the first and last pointings to be recovered) were then sent to MOC by E-mail, with the notification to start a Small-Gap Recovery.<br />
<br />
- MOC implemented the Small-Gap Recovery, provided the pointings could still be scheduled with respect to their latest start time, using the same scheme as described in the MOC-triggered SGR section<br />
<br />
Throughout the Planck mission, data losses were very rare. In fact Small-Gap Recovery was applied only a couple of times.<br />
<br />
==Special observations==<br />
The special observations are now described.<br />
<br />
* Normal scanning on Solar System objects for calibration purposes.<br />
<br />
[[File:Crab_Nebula.jpg|thumb|200px|The Crab Nebula (Messier 1, NGC 1952, Taurus A), here seen by the Hubble Space Telescope.]]<br />
<br />
[[File:Mars.jpg|thumb|200px|Mars as seen by the Hubble Space Telescope in 1999.]]<br />
<br />
This concerns the following objects (specifically planets): Mars; Jupiter; Saturn; Uranus; and Neptune. Their thermal emission in the far-infrared and the small angular sizes make them ideal calibrators for bolometers and radiometers.<br />
<br />
Mars is a particularly interesting calibrator for Planck, because of its proper motion.<br />
However this proper motion makes it difficult to observe it many times during the mission.<br />
<br />
Jupiter is the brightest source for (non-polarized) calibration. Saturn was also used significantly, with Uranus and Neptune being secondary calibrators.<br />
<br />
* Normal scanning on other (non-moving) sources for calibration purposes.<br />
<br />
This concerns mostly the Crab Nebula for polarization calibration purposes.<br />
This supernova remnant is highly polarized, and as such represents the main polarization calibrator for Planck.<br />
<br />
* Special pointings during the calibration phase, not relative to celestial sources.<br />
<br />
* "Deep rings," special observations that were performed on each passage of Jupiter and the Crab Nebula, from January 2012 onward.<br />
<br />
These consist of very deeply sampled observations (0.5') with the spin axis along the Ecliptic plane, typically lasting two to three weeks.<br />
<br />
Such observations benefit from special relaxing of the celestial constraints, with Solar Aspect Angles < 9 deg. rather than < 8 deg. during cycloidal surveying.<br />
<br />
* "Drift scans," special observations performed on Mars, making use of its proper motion.<br />
<br />
==Start and end of surveys==<br />
<br />
The completion of a given “survey” is declared when the logical AND of all frequency-coverage maps is greater than 95 %, OR the sky has been surveyed over a consecutive period of 7.5 months. Note that this definition is that of the Project Scientist and Planck Science Office. Data processing centres do not use exactly the same concept of surveys to create "survey" maps.<br />
<br />
In practice, since the gaps during the surveys have always been very small, this results in approximately 6 months per survey.<br />
<br />
[[File:PlanckMissionTimeline.JPG|thumb|300px|Planck mission timeline with the distribution of the "sky surveys".]]<br />
<br />
* '''Survey 1''': starts 13 August 2009, ends 13 February 2010.<br />
<br />
* '''Survey 2''': starts 14 February 2010, ends 13 August 2010.<br />
<br />
* '''Survey 3''': starts 14 August 2010, ends 13 February 2011.<br />
<br />
* '''Survey 4''': starts 14 February 2011, ends 29 July 2011.<br />
<br />
(This survey was shortened in ordered to start earlier with the new scanning strategy; see above).<br />
<br />
* '''Survey 5''': starts 29 July 2011, ends 30 January 2012.<br />
<br />
* '''Survey 6''' (LFI only): starts 30 January 2012, ends 31 July 2012.<br />
<br />
* '''Survey 7''' (LFI only): starts 31 July 2012, ends 31 January 2013.<br />
<br />
* '''Survey 8''' (LFI only): starts 1 February 2013, ends 1 August 2013.<br />
<br />
<br />
=== Completion of full sky coverage during Surveys 1-2 ===<br />
<br />
The picture gallery below exhibits the progress of sky coverage during the first months of survey (black colour = unobserved areas).<br />
<br />
<br />
<gallery widths=330 perrow=3 caption="HFI 353 GHz integration time after N months of survey. The units here are seconds per square degree, normalized to one detector."><br />
File:353_1month.png|After 1 month<br />
File:353_2month.png|After 2 months<br />
File:353_3month.png|After 3 months<br />
File:353_4month.png|After 4 months<br />
File:353_5month.png|After 5 months<br />
File:353_6month.png|After 6 months<br />
File:353_7month.png|After 7 months<br />
File:353_8month.png|After 8 months<br />
File:353_9months.png|After 9 months<br />
File:353_10months.png|After 10 months<br />
File:353_11months.png|After 11 months<br />
File:353_12months.png|After 12 months<br />
</gallery><br />
<br />
== Main planet and Crab observations ==<br />
<br />
Solar System objects and the Crab Nebula have been observed many times during the Planck surveys. Here is a list of these observations, with the ''deep rings'' (Jupiter and the Crab) and ''drift scans'' (Mars only) in '''boldface'''.<br />
<br />
* Crab: 16-22 September 2009<br />
<br />
* Mars: 17-29 October 2009<br />
<br />
* Jupiter: 25 October – 1 November 2009<br />
<br />
* Neptune: 1-8 November 2009<br />
<br />
* Uranus: 6-16 December 2009<br />
<br />
* Saturn: 2-8 January 2010<br />
<br />
* Crab: 6-12 March 2010<br />
<br />
* Mars: 9-18 April 2010<br />
<br />
* Neptune: 15-23 May 2010<br />
<br />
* Saturn: 13-22 June 2010<br />
<br />
* Uranus: 27 June – 5 July 2010<br />
<br />
* Jupiter: 1-9 July 2010<br />
<br />
* Crab: 15-21 September 2010<br />
<br />
* Neptune: 3-11 November 2010<br />
<br />
* Jupiter: 9-18 December 2010<br />
<br />
* Uranus: 12-21 December 2010<br />
<br />
* Saturn: 15-22 January 2011<br />
<br />
* Crab: 7-12 March 2011<br />
<br />
* Neptune: 18-26 May 2011<br />
<br />
* Saturn: 30 June - 9 July 2011<br />
<br />
* Uranus: 3-11 July 2011<br />
<br />
* Jupiter: 9-15 August 2011<br />
<br />
* Crab: 10-18 September 2011 (performed with the 250 deg. phase cycloidal strategy)<br />
<br />
* Crab: 20-23 September 2011 (performed with the 340 deg. phase cycloidal strategy)<br />
<br />
* '''Mars''': 8-16 December 2011 ("drift scan", Mars allowed to move through the Planck focal plane via its proper motion)<br />
<br />
* Mars: 17-26 December 2011 (normal scanning)<br />
<br />
* '''Jupiter''': 8-30 January 2012 (deep ring)<br />
<br />
* '''Crab''': 26 February - 16 March 2012 (deep ring)<br />
<br />
* '''Jupiter''': 1-14 September 2012 (deep ring)<br />
<br />
* '''Crab''': 14 September - 1 October 2012 (deep ring)<br />
<br />
* Neptune: 19-27 November 2012<br />
<br />
* Uranus: 24-30 December 2012<br />
<br />
* Saturn: 30 January - 5 February 2013<br />
<br />
* '''Jupiter''': February 2013 (deep ring)<br />
<br />
* '''Crab''': Feb. 28th - March 15th, 2013 (deep ring)<br />
<br />
* Neptune: June 4th - June 12th, 2013<br />
<br />
* Uranus: July 9-16th, 2013<br />
<br />
== Resulting integration time distribution ==<br />
<br />
The integration time after the end of HFI operations (January 2012) is shown in the following picture gallery.<br />
<br />
Units are seconds per square degree, normalized to one detector, for all maps. The projection is full-sky Mollweide centred on the Galactic centre.<br />
<br />
<br />
<br />
<gallery widths=330px perrow=3 caption="Integration time after the end of HFI operations (January 2012). The units here are seconds per square degree, normalized to one detector."><br />
File:HFI_fullmission_100GHz1-4.png|HFI 100 GHz 1,4<br />
File:HFI_fullmission_100GHz2-3.png|HFI 100 GHz 2,3<br />
File:HFI_fullmission_143GHz1-4.png|HFI 143 GHz 1-4<br />
File:HFI_fullmission_143GHz5-8.png|HFI 143 GHz 5-8<br />
File:HFI_fullmission_217GHz1-4.png|HFI 217 GHz 1-4<br />
File:HFI_fullmission_217GHz5-8.png|HFI 217 GHz 5-8<br />
File:HFI_fullmission_353GHz.png|HFI 353 GHz<br />
File:HFI_fullmission_545-857GHz.png|HFI 545 GHz / 857 GHz<br />
File:LFI25_coldmission.png|LFI-25 (44 GHz)<br />
File:LFI27_coldmission.png|LFI 30 GHz<br />
</gallery><br />
<br />
==References==<br />
<references /><br />
<br />
[[Category:Introduction|004]]<br />
[[Category:PSOBook]]</div>
Xdupac
https://wiki.cosmos.esa.int/planckpla2015/index.php?title=Survey_scanning_and_performance&diff=11014
Survey scanning and performance
2015-02-03T16:17:16Z
<p>Xdupac: /* Main planet and Crab observations */</p>
<hr />
<div>== The observation strategy ==<br />
<br />
The Planck ''observation strategy'', or ''scanning strategy'', made use of the characteristics of the Planck spacecraft {{PlanckPapers|planck2011-1-1}} and orbit in order to achieve the survey goals in terms of sky coverage and scanning directions.<br />
<br />
The Planck focal plane scanned the sky in the way explained in the figure below.<br />
<br />
[[file:FocalPlane.png|thumb|300px|Planck focal plane showing the direction of scanning. Polarization-sensitive detectors are drawn with crosses indicating the polarization orientation.]]<br />
<br />
The 353 GHz row scanned the sky in small circles with an 85 deg. bore-sight angle from the spin axis. 545 GHz, 857 GHz, and 143 GHz bolometers, as well as LFI radiometers 25 and 26 had a slightly smaller bore-sight angle, while the other part of the Planck focal plane had larger ones (up to about 89 deg.). The Planck spacecraft spun at a rate of 1 rpm.<br />
<br />
Planck, being at L2, moved along the Ecliptic at approximately one degree per day, and needed to keep the Solar aspect angle below about 9 degrees at all times. In practice, during the surveys, the limit considered was 8 deg. Another celestial constraint is that the angle between the Planck spin axis and the anti-Earth direction could not exceed 15 deg. (relaxed to 17 deg. from Survey 5 onward). These constraints had a very direct influence on the chosen scanning strategy.<br />
<br />
[[File:ScannStrategy.png|thumb|300px|Simplified illustration of the Planck scanning strategy, without additional motion of the spin axis.]]<br />
<br />
[[File:Observing_strat.png|thumb|300px|left|Planck scanning strategy, showing the additional motion of the spin axis.]]<br />
<br />
The path followed by the Planck spin axis was defined with respect to the Ecliptic plane. It corresponded to a motion in longitude which maintained an anti-Sun pointing (about one degree per day), to which was added a cycloidal motion (precession) of the spin axis around the anti-Sun position (fiducial point). The cycloidal path was defined by the functions: <br />
<br />
$ λ = θ sin((-1)^n ω (t-t_0)+φ) $ (eq. 1),<br />
<br />
$β = -θ cos((-1)^n ω(t-t_0) + φ) $ (eq. 2),<br />
<br />
where λ is the angular distance from the fiducial point in Ecliptic longitude, β the angular distance from the fiducial point in Ecliptic latitude, θ the spin axis precession amplitude, ω the pulsation of the precession, φ its phase, n the parameter which controls the motion direction of the precession, t is the time, and $t_0$ is the first time during the Planck survey at which the fiducial point crosses the Ecliptic longitude =0 line.<br />
<br />
[[File:Cycloidal_scanning.JPG|thumb|300px|Spin axis path with a 7 deg. amplitude cycloidal scanning, from Ref.{{BibCite|dupac2005}}]]<br />
<br />
The reasons to decide to use such a precession of the spin axis are the following.<br />
<br />
* An excursion of the spin axis from the anti-Sun direction is required to fully observe the whole sky (no excursion would leave a large area unobserved around the Ecliptic poles).<br />
<br />
* The precession motion keeps the Sun aspect angle constant during the whole survey, therefore minimizing the thermal constraint variations on the spacecraft.<br />
<br />
The following precession parameters were chosen for the BSS.<br />
<br />
* Amplitude θ = 7.5deg. (this value is the lowest possible which allows the whole sky to be covered with all detectors).<br />
<br />
* n = 1 (anti-clockwise motion as seen from the Sun).<br />
<br />
* Pulsation ω = 2π / (half a year), faster precession was considered, and has interesting advantages, but was not possible given the constraints if one wants to keep a 7.5 deg. amplitude (which is necessary to cover the whole sky).<br />
<br />
* The phase of the precession was decided according to this set of criteria (in order of importance):<br />
<br />
a) respecting the operational constraints;<br />
<br />
b) allowing the largest possible angle between two scans on the Crab Nebula (a polarization calibrator);<br />
<br />
c) avoiding null dipole amplitude for the whole mission;<br />
<br />
d) optimizing the position of the planets in the beginning of the survey and with respect to the feasibility of their recovery;<br />
<br />
e) placing the two “deep fields” where Galactic foregrounds are minimum;<br />
<br />
f) allowing a reasonable survey margin (i.e. the time allowed to recover lost pointings if a problem occurs).<br />
<br />
The phase is 340 deg. for Surveys 1 to 4, and 250 deg. for Surveys 5 to 8.<br />
<br />
The scanning strategy for the second year of Routine Operations (i.e. Surveys 3 and 4) was exactly the same as for the first year, except that all pointings were shifted by 1 arcmin along the cross-scanning direction, in order to provide finer sky sampling for the highest frequency detectors when combining two years of observations.<br />
<br />
The change of phase between Survey 4 and Survey 5 occurred because it was found essential (especially on the HFI side) that scanning direction crossings should be increased in the Planck survey. By choosing a phase 90 deg. away from the original one, one optimizes the scanning strategy in this respect.<br />
<br />
The details of the justifications for these parameters can be found in PL-WG9-TN-001.<br />
<br />
The scanning strategy parameters are input to the PSO Survey Planning and Performance Tool, which is the software which generates the series of pointing records to be sent out to MOC for implementation.<br />
<br />
An approximate visualization of the Planck scanning strategy can be found [http://www.youtube.com/watch?v=WwFXuZ0B3B8 here] and [http://www.youtube.com/watch?v=7Zu-aiEiDtY here].<br />
<br />
<br />
===Spin axis manoeuvres and exact pointings===<br />
The motion of the spin axis was not continuous. Every change in the spin axis position was initiated by a manoeuvre which required less than 5 minutes time to complete. <br />
<br />
The duration between spin-axis manoeuvres is hereafter referred to as the “dwelling time" and the angular distance between manoeuvres along the spin axis path is hereafter referred to as the “spacing”. <br />
<br />
The dwelling times and spacings are defined as follows:<br />
<br />
* the spacings are fixed to 2arcmin, which roughly corresponds to the Nyquist criterion for sampling the highest-frequency HFI detectors;<br />
<br />
* the dwell times vary from 2360 s to 3904 s.<br />
The exact series of coordinates and dwell times are set by Eqs. (1) and (2) when one has fixed the spacings.<br />
<br />
== Data gap recoveries ==<br />
<br />
Gaps in the data flow can occur for various reasons.<br />
<br />
Anomalies may occur at spacecraft or instrument level, but also due to failures in the ground-to-spacecraft link or the ground segment itself. The adverse effects of such anomalies may be the loss of scientific data corresponding to one or several planned pointings, which have not been acquired and/or stored in memory.<br />
<br />
Failure to acquire proper scientific data may occur to one or both instruments.<br />
<br />
When a gap occurred, scientific criteria were applied to decide whether to recover the data through the Small-Gap Recovery procedure.<br />
<br />
[[File:AHF_353_OD389.png|thumb|400px|Integration time of the 353 GHz detectors ({{PlanckPapers|lamarre2010}}) after 389 Operational Days (the unit is seconds per square degree, normalized to one detector). The first significant data gap and recovery are clearly visible.]]<br />
<br />
The Small-Gap Recovery (SGR) procedure could be applied by MOC or PSO.<br />
<br />
* '''MOC-triggered SGR''': Within its nominal scheduling procedure for an OD, the MOC searches the PPL for PREF corresponding to the OD being processed and any pointings which are the subject of a Small Gap Recovery. As the PREF are sorted in chronological order according to their nominal start time, those corresponding to a small gap will naturally be the earliest. After checking attitude constraints, all observable pointings are listed and their dwell times reduced (initially) to the Minimum Dwell Time (MDT), as given in the PPL.<br />
Having included all valid PREF the required slew times are calculated. With the required slew times and minimum dwell times for all pointings, the OD schedule may be under-populated; in this case the dwell times of all scheduled pointings will be increased equally to make use of all available time in the OD. If the resulting schedule is over-populated, even with MDT for all pointings, the recovery cannot be constrained to a single OD. The sequence of pointings for the ODs involved is optimized in PREF scheduling and dwell times determined in order to effect the recovery and revert to the nominal timeline as quickly as possible.<br />
<br />
* '''PSO-triggered SGR''':<br />
PSO declares a small gap when pointings that have been executed result in data of insufficient quality or inadequate frequency coverage. This assessment is based on data quality and instrument health information provided by the DPCs. The algorithm that was used by the PSO to check the scientific validity of a pointing was implemented within the SPPT software tool. The SPPT ingested on a weekly basis a Weekly Health Report (WHR) for the HFI and LFI containing information on the working status of each detector and their expected condition over the following four weeks. On a daily basis, a Daily Quality Report (DQR) provided by the DPCs for both instruments, included a set of parameters that described the quality of the detection achieved by each individual detector for every pointing executed.<br />
<br />
The scheme for declaring a Small-Gap Recovery from PSO is the following.<br />
<br />
- If a pointing fails to meet the chosen requirement, it becomes an SGR candidate.<br />
<br />
- If there are at least 12 consecutive pointings which are declared SGR candidates, and the problem has been identified and solved, then an SGR is triggered.<br />
Recoveries are only carried out if the recovery slewing is guaranteed to be in OCM. MOC carried out this analysis and decided whether they should perform the SGR accordingly.<br />
<br />
- The start and end times of the gap and the list of the pointing numbers (or just the numbers of the first and last pointings to be recovered) were then sent to MOC by E-mail, with the notification to start a Small-Gap Recovery.<br />
<br />
- MOC implemented the Small-Gap Recovery, provided the pointings could still be scheduled with respect to their latest start time, using the same scheme as described in the MOC-triggered SGR section<br />
<br />
Throughout the Planck mission, data losses were very rare. In fact Small-Gap Recovery was applied only a couple of times.<br />
<br />
==Special observations==<br />
The special observations are now described.<br />
<br />
* Normal scanning on Solar System objects for calibration purposes.<br />
<br />
[[File:Crab_Nebula.jpg|thumb|200px|The Crab Nebula (Messier 1, NGC 1952, Taurus A), here seen by the Hubble Space Telescope.]]<br />
<br />
[[File:Mars.jpg|thumb|200px|Mars as seen by the Hubble Space Telescope in 1999.]]<br />
<br />
This concerns the following objects (specifically planets): Mars; Jupiter; Saturn; Uranus; and Neptune. Their thermal emission in the far-infrared and the small angular sizes make them ideal calibrators for bolometers and radiometers.<br />
<br />
Mars is a particularly interesting calibrator for Planck, because of its proper motion.<br />
However this proper motion makes it difficult to observe it many times during the mission.<br />
<br />
Jupiter is the brightest source for (non-polarized) calibration. Saturn was also used significantly, with Uranus and Neptune being secondary calibrators.<br />
<br />
* Normal scanning on other (non-moving) sources for calibration purposes.<br />
<br />
This concerns mostly the Crab Nebula for polarization calibration purposes.<br />
This supernova remnant is highly polarized, and as such represents the main polarization calibrator for Planck.<br />
<br />
* Special pointings during the calibration phase, not relative to celestial sources.<br />
<br />
* "Deep rings," special observations that were performed on each passage of Jupiter and the Crab Nebula, from January 2012 onward.<br />
<br />
These consist of very deeply sampled observations (0.5') with the spin axis along the Ecliptic plane, typically lasting two to three weeks.<br />
<br />
Such observations benefit from special relaxing of the celestial constraints, with Solar Aspect Angles < 9 deg. rather than < 8 deg. during cycloidal surveying.<br />
<br />
* "Drift scans," special observations performed on Mars, making use of its proper motion.<br />
<br />
==Start and end of surveys==<br />
<br />
The completion of a given “survey” is declared when the logical AND of all frequency-coverage maps is greater than 95 %, OR the sky has been surveyed over a consecutive period of 7.5 months. Note that this definition is that of the Project Scientist and Planck Science Office. Data processing centres do not use exactly the same concept of surveys to create "survey" maps.<br />
<br />
In practice, since the gaps during the surveys have always been very small, this results in approximately 6 months per survey.<br />
<br />
[[File:PlanckMissionTimeline.JPG|thumb|300px|Planck mission timeline with the distribution of the "sky surveys".]]<br />
<br />
* '''Survey 1''': starts 13 August 2009, ends 13 February 2010.<br />
<br />
* '''Survey 2''': starts 14 February 2010, ends 13 August 2010.<br />
<br />
* '''Survey 3''': starts 14 August 2010, ends 13 February 2011.<br />
<br />
* '''Survey 4''': starts 14 February 2011, ends 29 July 2011.<br />
<br />
(This survey was shortened in ordered to start earlier with the new scanning strategy; see above).<br />
<br />
* '''Survey 5''': starts 29 July 2011, ends 30 January 2012.<br />
<br />
* '''Survey 6''' (LFI only): starts 30 January 2012, ends 31 July 2012.<br />
<br />
* '''Survey 7''' (LFI only): starts 31 July 2012, ends 31 January 2013.<br />
<br />
* '''Survey 8''' (LFI only): starts 1 February 2013, ends 1 August 2013.<br />
<br />
<br />
=== Completion of full sky coverage during Surveys 1-2 ===<br />
<br />
The picture gallery below exhibits the progress of sky coverage during the first months of survey (black colour = unobserved areas).<br />
<br />
<br />
<gallery widths=330 perrow=3 caption="HFI 353 GHz integration time after N months of survey. The units here are seconds per square degree, normalized to one detector."><br />
File:353_1month.png|After 1 month<br />
File:353_2month.png|After 2 months<br />
File:353_3month.png|After 3 months<br />
File:353_4month.png|After 4 months<br />
File:353_5month.png|After 5 months<br />
File:353_6month.png|After 6 months<br />
File:353_7month.png|After 7 months<br />
File:353_8month.png|After 8 months<br />
File:353_9months.png|After 9 months<br />
File:353_10months.png|After 10 months<br />
File:353_11months.png|After 11 months<br />
File:353_12months.png|After 12 months<br />
</gallery><br />
<br />
== Main planet and Crab observations ==<br />
<br />
Solar System objects and the Crab Nebula have been observed many times during the Planck surveys. Here is a list of these observations, with the ''deep rings'' (Jupiter and the Crab) and ''drift scans'' (Mars only) in '''boldface'''.<br />
<br />
* Crab: 16-22 September 2009<br />
<br />
* Mars: 17-29 October 2009<br />
<br />
* Jupiter: 25 October – 1 November 2009<br />
<br />
* Neptune: 1-8 November 2009<br />
<br />
* Uranus: 6-16 December 2009<br />
<br />
* Saturn: 2-8 January 2010<br />
<br />
* Crab: 6-12 March 2010<br />
<br />
* Mars: 9-18 April 2010<br />
<br />
* Neptune: 15-23 May 2010<br />
<br />
* Saturn: 13-22 June 2010<br />
<br />
* Uranus: 27 June – 5 July 2010<br />
<br />
* Jupiter: 1-9 July 2010<br />
<br />
* Crab: 15-21 September 2010<br />
<br />
* Neptune: 3-11 November 2010<br />
<br />
* Jupiter: 9-18 December 2010<br />
<br />
* Uranus: 12-21 December 2010<br />
<br />
* Saturn: 15-22 January 2011<br />
<br />
* Crab: 7-12 March 2011<br />
<br />
* Neptune: 18-26 May 2011<br />
<br />
* Saturn: 30 June - 9 July 2011<br />
<br />
* Uranus: 3-11 July 2011<br />
<br />
* Jupiter: 9-15 August 2011<br />
<br />
* Crab: 10-18 September 2011 (performed with the 250 deg. phase cycloidal strategy)<br />
<br />
* Crab: 20-23 September 2011 (performed with the 340 deg. phase cycloidal strategy)<br />
<br />
* '''Mars''': 8-16 December 2011 ("drift scan", Mars allowed to move through the Planck focal plane via its proper motion)<br />
<br />
* Mars: 17-26 December 2011 (normal scanning)<br />
<br />
* '''Jupiter''': 8-30 January 2012 (deep ring)<br />
<br />
* '''Crab''': 26 February - 16 March 2012 (deep ring)<br />
<br />
* '''Jupiter''': 1-14 September 2012 (deep ring)<br />
<br />
* '''Crab''': 14 September - 1 October 2012 (deep ring)<br />
<br />
* Neptune: 19-27 November 2012<br />
<br />
* Uranus: 24-30 December 2012<br />
<br />
* Saturn: 30 January - 5 February 2013<br />
<br />
* '''Jupiter''': February 2013 (deep ring)<br />
<br />
* '''Crab''': Feb. 28th - March 15th, 2013 (deep ring)<br />
<br />
* Neptune: June 4th - June 12th, 2013<br />
<br />
== Resulting integration time distribution ==<br />
<br />
The integration time after the end of HFI operations (January 2012) is shown in the following picture gallery.<br />
<br />
Units are seconds per square degree, normalized to one detector, for all maps. The projection is full-sky Mollweide centred on the Galactic centre.<br />
<br />
<br />
<br />
<gallery widths=330px perrow=3 caption="Integration time after the end of HFI operations (January 2012). The units here are seconds per square degree, normalized to one detector."><br />
File:HFI_fullmission_100GHz1-4.png|HFI 100 GHz 1,4<br />
File:HFI_fullmission_100GHz2-3.png|HFI 100 GHz 2,3<br />
File:HFI_fullmission_143GHz1-4.png|HFI 143 GHz 1-4<br />
File:HFI_fullmission_143GHz5-8.png|HFI 143 GHz 5-8<br />
File:HFI_fullmission_217GHz1-4.png|HFI 217 GHz 1-4<br />
File:HFI_fullmission_217GHz5-8.png|HFI 217 GHz 5-8<br />
File:HFI_fullmission_353GHz.png|HFI 353 GHz<br />
File:HFI_fullmission_545-857GHz.png|HFI 545 GHz / 857 GHz<br />
File:LFI25_coldmission.png|LFI-25 (44 GHz)<br />
File:LFI27_coldmission.png|LFI 30 GHz<br />
</gallery><br />
<br />
==References==<br />
<references /><br />
<br />
[[Category:Introduction|004]]<br />
[[Category:PSOBook]]</div>
Xdupac
https://wiki.cosmos.esa.int/planckpla2015/index.php?title=Survey_scanning_and_performance&diff=11013
Survey scanning and performance
2015-02-03T16:16:45Z
<p>Xdupac: /* Main planet and Crab observations */</p>
<hr />
<div>== The observation strategy ==<br />
<br />
The Planck ''observation strategy'', or ''scanning strategy'', made use of the characteristics of the Planck spacecraft {{PlanckPapers|planck2011-1-1}} and orbit in order to achieve the survey goals in terms of sky coverage and scanning directions.<br />
<br />
The Planck focal plane scanned the sky in the way explained in the figure below.<br />
<br />
[[file:FocalPlane.png|thumb|300px|Planck focal plane showing the direction of scanning. Polarization-sensitive detectors are drawn with crosses indicating the polarization orientation.]]<br />
<br />
The 353 GHz row scanned the sky in small circles with an 85 deg. bore-sight angle from the spin axis. 545 GHz, 857 GHz, and 143 GHz bolometers, as well as LFI radiometers 25 and 26 had a slightly smaller bore-sight angle, while the other part of the Planck focal plane had larger ones (up to about 89 deg.). The Planck spacecraft spun at a rate of 1 rpm.<br />
<br />
Planck, being at L2, moved along the Ecliptic at approximately one degree per day, and needed to keep the Solar aspect angle below about 9 degrees at all times. In practice, during the surveys, the limit considered was 8 deg. Another celestial constraint is that the angle between the Planck spin axis and the anti-Earth direction could not exceed 15 deg. (relaxed to 17 deg. from Survey 5 onward). These constraints had a very direct influence on the chosen scanning strategy.<br />
<br />
[[File:ScannStrategy.png|thumb|300px|Simplified illustration of the Planck scanning strategy, without additional motion of the spin axis.]]<br />
<br />
[[File:Observing_strat.png|thumb|300px|left|Planck scanning strategy, showing the additional motion of the spin axis.]]<br />
<br />
The path followed by the Planck spin axis was defined with respect to the Ecliptic plane. It corresponded to a motion in longitude which maintained an anti-Sun pointing (about one degree per day), to which was added a cycloidal motion (precession) of the spin axis around the anti-Sun position (fiducial point). The cycloidal path was defined by the functions: <br />
<br />
$ λ = θ sin((-1)^n ω (t-t_0)+φ) $ (eq. 1),<br />
<br />
$β = -θ cos((-1)^n ω(t-t_0) + φ) $ (eq. 2),<br />
<br />
where λ is the angular distance from the fiducial point in Ecliptic longitude, β the angular distance from the fiducial point in Ecliptic latitude, θ the spin axis precession amplitude, ω the pulsation of the precession, φ its phase, n the parameter which controls the motion direction of the precession, t is the time, and $t_0$ is the first time during the Planck survey at which the fiducial point crosses the Ecliptic longitude =0 line.<br />
<br />
[[File:Cycloidal_scanning.JPG|thumb|300px|Spin axis path with a 7 deg. amplitude cycloidal scanning, from Ref.{{BibCite|dupac2005}}]]<br />
<br />
The reasons to decide to use such a precession of the spin axis are the following.<br />
<br />
* An excursion of the spin axis from the anti-Sun direction is required to fully observe the whole sky (no excursion would leave a large area unobserved around the Ecliptic poles).<br />
<br />
* The precession motion keeps the Sun aspect angle constant during the whole survey, therefore minimizing the thermal constraint variations on the spacecraft.<br />
<br />
The following precession parameters were chosen for the BSS.<br />
<br />
* Amplitude θ = 7.5deg. (this value is the lowest possible which allows the whole sky to be covered with all detectors).<br />
<br />
* n = 1 (anti-clockwise motion as seen from the Sun).<br />
<br />
* Pulsation ω = 2π / (half a year), faster precession was considered, and has interesting advantages, but was not possible given the constraints if one wants to keep a 7.5 deg. amplitude (which is necessary to cover the whole sky).<br />
<br />
* The phase of the precession was decided according to this set of criteria (in order of importance):<br />
<br />
a) respecting the operational constraints;<br />
<br />
b) allowing the largest possible angle between two scans on the Crab Nebula (a polarization calibrator);<br />
<br />
c) avoiding null dipole amplitude for the whole mission;<br />
<br />
d) optimizing the position of the planets in the beginning of the survey and with respect to the feasibility of their recovery;<br />
<br />
e) placing the two “deep fields” where Galactic foregrounds are minimum;<br />
<br />
f) allowing a reasonable survey margin (i.e. the time allowed to recover lost pointings if a problem occurs).<br />
<br />
The phase is 340 deg. for Surveys 1 to 4, and 250 deg. for Surveys 5 to 8.<br />
<br />
The scanning strategy for the second year of Routine Operations (i.e. Surveys 3 and 4) was exactly the same as for the first year, except that all pointings were shifted by 1 arcmin along the cross-scanning direction, in order to provide finer sky sampling for the highest frequency detectors when combining two years of observations.<br />
<br />
The change of phase between Survey 4 and Survey 5 occurred because it was found essential (especially on the HFI side) that scanning direction crossings should be increased in the Planck survey. By choosing a phase 90 deg. away from the original one, one optimizes the scanning strategy in this respect.<br />
<br />
The details of the justifications for these parameters can be found in PL-WG9-TN-001.<br />
<br />
The scanning strategy parameters are input to the PSO Survey Planning and Performance Tool, which is the software which generates the series of pointing records to be sent out to MOC for implementation.<br />
<br />
An approximate visualization of the Planck scanning strategy can be found [http://www.youtube.com/watch?v=WwFXuZ0B3B8 here] and [http://www.youtube.com/watch?v=7Zu-aiEiDtY here].<br />
<br />
<br />
===Spin axis manoeuvres and exact pointings===<br />
The motion of the spin axis was not continuous. Every change in the spin axis position was initiated by a manoeuvre which required less than 5 minutes time to complete. <br />
<br />
The duration between spin-axis manoeuvres is hereafter referred to as the “dwelling time" and the angular distance between manoeuvres along the spin axis path is hereafter referred to as the “spacing”. <br />
<br />
The dwelling times and spacings are defined as follows:<br />
<br />
* the spacings are fixed to 2arcmin, which roughly corresponds to the Nyquist criterion for sampling the highest-frequency HFI detectors;<br />
<br />
* the dwell times vary from 2360 s to 3904 s.<br />
The exact series of coordinates and dwell times are set by Eqs. (1) and (2) when one has fixed the spacings.<br />
<br />
== Data gap recoveries ==<br />
<br />
Gaps in the data flow can occur for various reasons.<br />
<br />
Anomalies may occur at spacecraft or instrument level, but also due to failures in the ground-to-spacecraft link or the ground segment itself. The adverse effects of such anomalies may be the loss of scientific data corresponding to one or several planned pointings, which have not been acquired and/or stored in memory.<br />
<br />
Failure to acquire proper scientific data may occur to one or both instruments.<br />
<br />
When a gap occurred, scientific criteria were applied to decide whether to recover the data through the Small-Gap Recovery procedure.<br />
<br />
[[File:AHF_353_OD389.png|thumb|400px|Integration time of the 353 GHz detectors ({{PlanckPapers|lamarre2010}}) after 389 Operational Days (the unit is seconds per square degree, normalized to one detector). The first significant data gap and recovery are clearly visible.]]<br />
<br />
The Small-Gap Recovery (SGR) procedure could be applied by MOC or PSO.<br />
<br />
* '''MOC-triggered SGR''': Within its nominal scheduling procedure for an OD, the MOC searches the PPL for PREF corresponding to the OD being processed and any pointings which are the subject of a Small Gap Recovery. As the PREF are sorted in chronological order according to their nominal start time, those corresponding to a small gap will naturally be the earliest. After checking attitude constraints, all observable pointings are listed and their dwell times reduced (initially) to the Minimum Dwell Time (MDT), as given in the PPL.<br />
Having included all valid PREF the required slew times are calculated. With the required slew times and minimum dwell times for all pointings, the OD schedule may be under-populated; in this case the dwell times of all scheduled pointings will be increased equally to make use of all available time in the OD. If the resulting schedule is over-populated, even with MDT for all pointings, the recovery cannot be constrained to a single OD. The sequence of pointings for the ODs involved is optimized in PREF scheduling and dwell times determined in order to effect the recovery and revert to the nominal timeline as quickly as possible.<br />
<br />
* '''PSO-triggered SGR''':<br />
PSO declares a small gap when pointings that have been executed result in data of insufficient quality or inadequate frequency coverage. This assessment is based on data quality and instrument health information provided by the DPCs. The algorithm that was used by the PSO to check the scientific validity of a pointing was implemented within the SPPT software tool. The SPPT ingested on a weekly basis a Weekly Health Report (WHR) for the HFI and LFI containing information on the working status of each detector and their expected condition over the following four weeks. On a daily basis, a Daily Quality Report (DQR) provided by the DPCs for both instruments, included a set of parameters that described the quality of the detection achieved by each individual detector for every pointing executed.<br />
<br />
The scheme for declaring a Small-Gap Recovery from PSO is the following.<br />
<br />
- If a pointing fails to meet the chosen requirement, it becomes an SGR candidate.<br />
<br />
- If there are at least 12 consecutive pointings which are declared SGR candidates, and the problem has been identified and solved, then an SGR is triggered.<br />
Recoveries are only carried out if the recovery slewing is guaranteed to be in OCM. MOC carried out this analysis and decided whether they should perform the SGR accordingly.<br />
<br />
- The start and end times of the gap and the list of the pointing numbers (or just the numbers of the first and last pointings to be recovered) were then sent to MOC by E-mail, with the notification to start a Small-Gap Recovery.<br />
<br />
- MOC implemented the Small-Gap Recovery, provided the pointings could still be scheduled with respect to their latest start time, using the same scheme as described in the MOC-triggered SGR section<br />
<br />
Throughout the Planck mission, data losses were very rare. In fact Small-Gap Recovery was applied only a couple of times.<br />
<br />
==Special observations==<br />
The special observations are now described.<br />
<br />
* Normal scanning on Solar System objects for calibration purposes.<br />
<br />
[[File:Crab_Nebula.jpg|thumb|200px|The Crab Nebula (Messier 1, NGC 1952, Taurus A), here seen by the Hubble Space Telescope.]]<br />
<br />
[[File:Mars.jpg|thumb|200px|Mars as seen by the Hubble Space Telescope in 1999.]]<br />
<br />
This concerns the following objects (specifically planets): Mars; Jupiter; Saturn; Uranus; and Neptune. Their thermal emission in the far-infrared and the small angular sizes make them ideal calibrators for bolometers and radiometers.<br />
<br />
Mars is a particularly interesting calibrator for Planck, because of its proper motion.<br />
However this proper motion makes it difficult to observe it many times during the mission.<br />
<br />
Jupiter is the brightest source for (non-polarized) calibration. Saturn was also used significantly, with Uranus and Neptune being secondary calibrators.<br />
<br />
* Normal scanning on other (non-moving) sources for calibration purposes.<br />
<br />
This concerns mostly the Crab Nebula for polarization calibration purposes.<br />
This supernova remnant is highly polarized, and as such represents the main polarization calibrator for Planck.<br />
<br />
* Special pointings during the calibration phase, not relative to celestial sources.<br />
<br />
* "Deep rings," special observations that were performed on each passage of Jupiter and the Crab Nebula, from January 2012 onward.<br />
<br />
These consist of very deeply sampled observations (0.5') with the spin axis along the Ecliptic plane, typically lasting two to three weeks.<br />
<br />
Such observations benefit from special relaxing of the celestial constraints, with Solar Aspect Angles < 9 deg. rather than < 8 deg. during cycloidal surveying.<br />
<br />
* "Drift scans," special observations performed on Mars, making use of its proper motion.<br />
<br />
==Start and end of surveys==<br />
<br />
The completion of a given “survey” is declared when the logical AND of all frequency-coverage maps is greater than 95 %, OR the sky has been surveyed over a consecutive period of 7.5 months. Note that this definition is that of the Project Scientist and Planck Science Office. Data processing centres do not use exactly the same concept of surveys to create "survey" maps.<br />
<br />
In practice, since the gaps during the surveys have always been very small, this results in approximately 6 months per survey.<br />
<br />
[[File:PlanckMissionTimeline.JPG|thumb|300px|Planck mission timeline with the distribution of the "sky surveys".]]<br />
<br />
* '''Survey 1''': starts 13 August 2009, ends 13 February 2010.<br />
<br />
* '''Survey 2''': starts 14 February 2010, ends 13 August 2010.<br />
<br />
* '''Survey 3''': starts 14 August 2010, ends 13 February 2011.<br />
<br />
* '''Survey 4''': starts 14 February 2011, ends 29 July 2011.<br />
<br />
(This survey was shortened in ordered to start earlier with the new scanning strategy; see above).<br />
<br />
* '''Survey 5''': starts 29 July 2011, ends 30 January 2012.<br />
<br />
* '''Survey 6''' (LFI only): starts 30 January 2012, ends 31 July 2012.<br />
<br />
* '''Survey 7''' (LFI only): starts 31 July 2012, ends 31 January 2013.<br />
<br />
* '''Survey 8''' (LFI only): starts 1 February 2013, ends 1 August 2013.<br />
<br />
<br />
=== Completion of full sky coverage during Surveys 1-2 ===<br />
<br />
The picture gallery below exhibits the progress of sky coverage during the first months of survey (black colour = unobserved areas).<br />
<br />
<br />
<gallery widths=330 perrow=3 caption="HFI 353 GHz integration time after N months of survey. The units here are seconds per square degree, normalized to one detector."><br />
File:353_1month.png|After 1 month<br />
File:353_2month.png|After 2 months<br />
File:353_3month.png|After 3 months<br />
File:353_4month.png|After 4 months<br />
File:353_5month.png|After 5 months<br />
File:353_6month.png|After 6 months<br />
File:353_7month.png|After 7 months<br />
File:353_8month.png|After 8 months<br />
File:353_9months.png|After 9 months<br />
File:353_10months.png|After 10 months<br />
File:353_11months.png|After 11 months<br />
File:353_12months.png|After 12 months<br />
</gallery><br />
<br />
== Main planet and Crab observations ==<br />
<br />
Solar System objects and the Crab Nebula have been observed many times during the Planck surveys. Here is a list of these observations, with the ''deep rings'' (Jupiter and the Crab) and ''drift scans'' (Mars only) in '''boldface'''.<br />
<br />
* Crab: 16-22 September 2009<br />
<br />
* Mars: 17-29 October 2009<br />
<br />
* Jupiter: 25 October – 1 November 2009<br />
<br />
* Neptune: 1-8 November 2009<br />
<br />
* Uranus: 6-16 December 2009<br />
<br />
* Saturn: 2-8 January 2010<br />
<br />
* Crab: 6-12 March 2010<br />
<br />
* Mars: 9-18 April 2010<br />
<br />
* Neptune: 15-23 May 2010<br />
<br />
* Saturn: 13-22 June 2010<br />
<br />
* Uranus: 27 June – 5 July 2010<br />
<br />
* Jupiter: 1-9 July 2010<br />
<br />
* Crab: 15-21 September 2010<br />
<br />
* Neptune: 3-11 November 2010<br />
<br />
* Jupiter: 9-18 December 2010<br />
<br />
* Uranus: 12-21 December 2010<br />
<br />
* Saturn: 15-22 January 2011<br />
<br />
* Crab: 7-12 March 2011<br />
<br />
* Neptune: 18-26 May 2011<br />
<br />
* Saturn: 30 June - 9 July 2011<br />
<br />
* Uranus: 3-11 July 2011<br />
<br />
* Jupiter: 9-15 August 2011<br />
<br />
* Crab: 10-18 September 2011 (performed with the 250 deg. phase cycloidal strategy)<br />
<br />
* Crab: 20-23 September 2011 (performed with the 340 deg. phase cycloidal strategy)<br />
<br />
* '''Mars''': 8-16 December 2011 ("drift scan", Mars allowed to move through the Planck focal plane via its proper motion)<br />
<br />
* Mars: 17-26 December 2011 (normal scanning)<br />
<br />
* '''Jupiter''': 8-30 January 2012 (deep ring)<br />
<br />
* '''Crab''': 26 February - 16 March 2012 (deep ring)<br />
<br />
* '''Jupiter''': 1-14 September 2012 (deep ring)<br />
<br />
* '''Crab''': 14 September - 1 October 2012 (deep ring)<br />
<br />
* Neptune: 19-27 November 2012<br />
<br />
* Uranus: 24-30 December 2012<br />
<br />
* Saturn: 30 January - 5 February 2013<br />
<br />
* '''Jupiter''': February 2013 (deep ring)<br />
<br />
* '''Crab''': Feb. 28th - March 15th, 2013<br />
<br />
* Neptune: June 4th - June 12th, 2013<br />
<br />
== Resulting integration time distribution ==<br />
<br />
The integration time after the end of HFI operations (January 2012) is shown in the following picture gallery.<br />
<br />
Units are seconds per square degree, normalized to one detector, for all maps. The projection is full-sky Mollweide centred on the Galactic centre.<br />
<br />
<br />
<br />
<gallery widths=330px perrow=3 caption="Integration time after the end of HFI operations (January 2012). The units here are seconds per square degree, normalized to one detector."><br />
File:HFI_fullmission_100GHz1-4.png|HFI 100 GHz 1,4<br />
File:HFI_fullmission_100GHz2-3.png|HFI 100 GHz 2,3<br />
File:HFI_fullmission_143GHz1-4.png|HFI 143 GHz 1-4<br />
File:HFI_fullmission_143GHz5-8.png|HFI 143 GHz 5-8<br />
File:HFI_fullmission_217GHz1-4.png|HFI 217 GHz 1-4<br />
File:HFI_fullmission_217GHz5-8.png|HFI 217 GHz 5-8<br />
File:HFI_fullmission_353GHz.png|HFI 353 GHz<br />
File:HFI_fullmission_545-857GHz.png|HFI 545 GHz / 857 GHz<br />
File:LFI25_coldmission.png|LFI-25 (44 GHz)<br />
File:LFI27_coldmission.png|LFI 30 GHz<br />
</gallery><br />
<br />
==References==<br />
<references /><br />
<br />
[[Category:Introduction|004]]<br />
[[Category:PSOBook]]</div>
Xdupac
https://wiki.cosmos.esa.int/planckpla2015/index.php?title=Survey_scanning_and_performance&diff=11012
Survey scanning and performance
2015-02-03T16:16:05Z
<p>Xdupac: /* Main planet and Crab observations */</p>
<hr />
<div>== The observation strategy ==<br />
<br />
The Planck ''observation strategy'', or ''scanning strategy'', made use of the characteristics of the Planck spacecraft {{PlanckPapers|planck2011-1-1}} and orbit in order to achieve the survey goals in terms of sky coverage and scanning directions.<br />
<br />
The Planck focal plane scanned the sky in the way explained in the figure below.<br />
<br />
[[file:FocalPlane.png|thumb|300px|Planck focal plane showing the direction of scanning. Polarization-sensitive detectors are drawn with crosses indicating the polarization orientation.]]<br />
<br />
The 353 GHz row scanned the sky in small circles with an 85 deg. bore-sight angle from the spin axis. 545 GHz, 857 GHz, and 143 GHz bolometers, as well as LFI radiometers 25 and 26 had a slightly smaller bore-sight angle, while the other part of the Planck focal plane had larger ones (up to about 89 deg.). The Planck spacecraft spun at a rate of 1 rpm.<br />
<br />
Planck, being at L2, moved along the Ecliptic at approximately one degree per day, and needed to keep the Solar aspect angle below about 9 degrees at all times. In practice, during the surveys, the limit considered was 8 deg. Another celestial constraint is that the angle between the Planck spin axis and the anti-Earth direction could not exceed 15 deg. (relaxed to 17 deg. from Survey 5 onward). These constraints had a very direct influence on the chosen scanning strategy.<br />
<br />
[[File:ScannStrategy.png|thumb|300px|Simplified illustration of the Planck scanning strategy, without additional motion of the spin axis.]]<br />
<br />
[[File:Observing_strat.png|thumb|300px|left|Planck scanning strategy, showing the additional motion of the spin axis.]]<br />
<br />
The path followed by the Planck spin axis was defined with respect to the Ecliptic plane. It corresponded to a motion in longitude which maintained an anti-Sun pointing (about one degree per day), to which was added a cycloidal motion (precession) of the spin axis around the anti-Sun position (fiducial point). The cycloidal path was defined by the functions: <br />
<br />
$ λ = θ sin((-1)^n ω (t-t_0)+φ) $ (eq. 1),<br />
<br />
$β = -θ cos((-1)^n ω(t-t_0) + φ) $ (eq. 2),<br />
<br />
where λ is the angular distance from the fiducial point in Ecliptic longitude, β the angular distance from the fiducial point in Ecliptic latitude, θ the spin axis precession amplitude, ω the pulsation of the precession, φ its phase, n the parameter which controls the motion direction of the precession, t is the time, and $t_0$ is the first time during the Planck survey at which the fiducial point crosses the Ecliptic longitude =0 line.<br />
<br />
[[File:Cycloidal_scanning.JPG|thumb|300px|Spin axis path with a 7 deg. amplitude cycloidal scanning, from Ref.{{BibCite|dupac2005}}]]<br />
<br />
The reasons to decide to use such a precession of the spin axis are the following.<br />
<br />
* An excursion of the spin axis from the anti-Sun direction is required to fully observe the whole sky (no excursion would leave a large area unobserved around the Ecliptic poles).<br />
<br />
* The precession motion keeps the Sun aspect angle constant during the whole survey, therefore minimizing the thermal constraint variations on the spacecraft.<br />
<br />
The following precession parameters were chosen for the BSS.<br />
<br />
* Amplitude θ = 7.5deg. (this value is the lowest possible which allows the whole sky to be covered with all detectors).<br />
<br />
* n = 1 (anti-clockwise motion as seen from the Sun).<br />
<br />
* Pulsation ω = 2π / (half a year), faster precession was considered, and has interesting advantages, but was not possible given the constraints if one wants to keep a 7.5 deg. amplitude (which is necessary to cover the whole sky).<br />
<br />
* The phase of the precession was decided according to this set of criteria (in order of importance):<br />
<br />
a) respecting the operational constraints;<br />
<br />
b) allowing the largest possible angle between two scans on the Crab Nebula (a polarization calibrator);<br />
<br />
c) avoiding null dipole amplitude for the whole mission;<br />
<br />
d) optimizing the position of the planets in the beginning of the survey and with respect to the feasibility of their recovery;<br />
<br />
e) placing the two “deep fields” where Galactic foregrounds are minimum;<br />
<br />
f) allowing a reasonable survey margin (i.e. the time allowed to recover lost pointings if a problem occurs).<br />
<br />
The phase is 340 deg. for Surveys 1 to 4, and 250 deg. for Surveys 5 to 8.<br />
<br />
The scanning strategy for the second year of Routine Operations (i.e. Surveys 3 and 4) was exactly the same as for the first year, except that all pointings were shifted by 1 arcmin along the cross-scanning direction, in order to provide finer sky sampling for the highest frequency detectors when combining two years of observations.<br />
<br />
The change of phase between Survey 4 and Survey 5 occurred because it was found essential (especially on the HFI side) that scanning direction crossings should be increased in the Planck survey. By choosing a phase 90 deg. away from the original one, one optimizes the scanning strategy in this respect.<br />
<br />
The details of the justifications for these parameters can be found in PL-WG9-TN-001.<br />
<br />
The scanning strategy parameters are input to the PSO Survey Planning and Performance Tool, which is the software which generates the series of pointing records to be sent out to MOC for implementation.<br />
<br />
An approximate visualization of the Planck scanning strategy can be found [http://www.youtube.com/watch?v=WwFXuZ0B3B8 here] and [http://www.youtube.com/watch?v=7Zu-aiEiDtY here].<br />
<br />
<br />
===Spin axis manoeuvres and exact pointings===<br />
The motion of the spin axis was not continuous. Every change in the spin axis position was initiated by a manoeuvre which required less than 5 minutes time to complete. <br />
<br />
The duration between spin-axis manoeuvres is hereafter referred to as the “dwelling time" and the angular distance between manoeuvres along the spin axis path is hereafter referred to as the “spacing”. <br />
<br />
The dwelling times and spacings are defined as follows:<br />
<br />
* the spacings are fixed to 2arcmin, which roughly corresponds to the Nyquist criterion for sampling the highest-frequency HFI detectors;<br />
<br />
* the dwell times vary from 2360 s to 3904 s.<br />
The exact series of coordinates and dwell times are set by Eqs. (1) and (2) when one has fixed the spacings.<br />
<br />
== Data gap recoveries ==<br />
<br />
Gaps in the data flow can occur for various reasons.<br />
<br />
Anomalies may occur at spacecraft or instrument level, but also due to failures in the ground-to-spacecraft link or the ground segment itself. The adverse effects of such anomalies may be the loss of scientific data corresponding to one or several planned pointings, which have not been acquired and/or stored in memory.<br />
<br />
Failure to acquire proper scientific data may occur to one or both instruments.<br />
<br />
When a gap occurred, scientific criteria were applied to decide whether to recover the data through the Small-Gap Recovery procedure.<br />
<br />
[[File:AHF_353_OD389.png|thumb|400px|Integration time of the 353 GHz detectors ({{PlanckPapers|lamarre2010}}) after 389 Operational Days (the unit is seconds per square degree, normalized to one detector). The first significant data gap and recovery are clearly visible.]]<br />
<br />
The Small-Gap Recovery (SGR) procedure could be applied by MOC or PSO.<br />
<br />
* '''MOC-triggered SGR''': Within its nominal scheduling procedure for an OD, the MOC searches the PPL for PREF corresponding to the OD being processed and any pointings which are the subject of a Small Gap Recovery. As the PREF are sorted in chronological order according to their nominal start time, those corresponding to a small gap will naturally be the earliest. After checking attitude constraints, all observable pointings are listed and their dwell times reduced (initially) to the Minimum Dwell Time (MDT), as given in the PPL.<br />
Having included all valid PREF the required slew times are calculated. With the required slew times and minimum dwell times for all pointings, the OD schedule may be under-populated; in this case the dwell times of all scheduled pointings will be increased equally to make use of all available time in the OD. If the resulting schedule is over-populated, even with MDT for all pointings, the recovery cannot be constrained to a single OD. The sequence of pointings for the ODs involved is optimized in PREF scheduling and dwell times determined in order to effect the recovery and revert to the nominal timeline as quickly as possible.<br />
<br />
* '''PSO-triggered SGR''':<br />
PSO declares a small gap when pointings that have been executed result in data of insufficient quality or inadequate frequency coverage. This assessment is based on data quality and instrument health information provided by the DPCs. The algorithm that was used by the PSO to check the scientific validity of a pointing was implemented within the SPPT software tool. The SPPT ingested on a weekly basis a Weekly Health Report (WHR) for the HFI and LFI containing information on the working status of each detector and their expected condition over the following four weeks. On a daily basis, a Daily Quality Report (DQR) provided by the DPCs for both instruments, included a set of parameters that described the quality of the detection achieved by each individual detector for every pointing executed.<br />
<br />
The scheme for declaring a Small-Gap Recovery from PSO is the following.<br />
<br />
- If a pointing fails to meet the chosen requirement, it becomes an SGR candidate.<br />
<br />
- If there are at least 12 consecutive pointings which are declared SGR candidates, and the problem has been identified and solved, then an SGR is triggered.<br />
Recoveries are only carried out if the recovery slewing is guaranteed to be in OCM. MOC carried out this analysis and decided whether they should perform the SGR accordingly.<br />
<br />
- The start and end times of the gap and the list of the pointing numbers (or just the numbers of the first and last pointings to be recovered) were then sent to MOC by E-mail, with the notification to start a Small-Gap Recovery.<br />
<br />
- MOC implemented the Small-Gap Recovery, provided the pointings could still be scheduled with respect to their latest start time, using the same scheme as described in the MOC-triggered SGR section<br />
<br />
Throughout the Planck mission, data losses were very rare. In fact Small-Gap Recovery was applied only a couple of times.<br />
<br />
==Special observations==<br />
The special observations are now described.<br />
<br />
* Normal scanning on Solar System objects for calibration purposes.<br />
<br />
[[File:Crab_Nebula.jpg|thumb|200px|The Crab Nebula (Messier 1, NGC 1952, Taurus A), here seen by the Hubble Space Telescope.]]<br />
<br />
[[File:Mars.jpg|thumb|200px|Mars as seen by the Hubble Space Telescope in 1999.]]<br />
<br />
This concerns the following objects (specifically planets): Mars; Jupiter; Saturn; Uranus; and Neptune. Their thermal emission in the far-infrared and the small angular sizes make them ideal calibrators for bolometers and radiometers.<br />
<br />
Mars is a particularly interesting calibrator for Planck, because of its proper motion.<br />
However this proper motion makes it difficult to observe it many times during the mission.<br />
<br />
Jupiter is the brightest source for (non-polarized) calibration. Saturn was also used significantly, with Uranus and Neptune being secondary calibrators.<br />
<br />
* Normal scanning on other (non-moving) sources for calibration purposes.<br />
<br />
This concerns mostly the Crab Nebula for polarization calibration purposes.<br />
This supernova remnant is highly polarized, and as such represents the main polarization calibrator for Planck.<br />
<br />
* Special pointings during the calibration phase, not relative to celestial sources.<br />
<br />
* "Deep rings," special observations that were performed on each passage of Jupiter and the Crab Nebula, from January 2012 onward.<br />
<br />
These consist of very deeply sampled observations (0.5') with the spin axis along the Ecliptic plane, typically lasting two to three weeks.<br />
<br />
Such observations benefit from special relaxing of the celestial constraints, with Solar Aspect Angles < 9 deg. rather than < 8 deg. during cycloidal surveying.<br />
<br />
* "Drift scans," special observations performed on Mars, making use of its proper motion.<br />
<br />
==Start and end of surveys==<br />
<br />
The completion of a given “survey” is declared when the logical AND of all frequency-coverage maps is greater than 95 %, OR the sky has been surveyed over a consecutive period of 7.5 months. Note that this definition is that of the Project Scientist and Planck Science Office. Data processing centres do not use exactly the same concept of surveys to create "survey" maps.<br />
<br />
In practice, since the gaps during the surveys have always been very small, this results in approximately 6 months per survey.<br />
<br />
[[File:PlanckMissionTimeline.JPG|thumb|300px|Planck mission timeline with the distribution of the "sky surveys".]]<br />
<br />
* '''Survey 1''': starts 13 August 2009, ends 13 February 2010.<br />
<br />
* '''Survey 2''': starts 14 February 2010, ends 13 August 2010.<br />
<br />
* '''Survey 3''': starts 14 August 2010, ends 13 February 2011.<br />
<br />
* '''Survey 4''': starts 14 February 2011, ends 29 July 2011.<br />
<br />
(This survey was shortened in ordered to start earlier with the new scanning strategy; see above).<br />
<br />
* '''Survey 5''': starts 29 July 2011, ends 30 January 2012.<br />
<br />
* '''Survey 6''' (LFI only): starts 30 January 2012, ends 31 July 2012.<br />
<br />
* '''Survey 7''' (LFI only): starts 31 July 2012, ends 31 January 2013.<br />
<br />
* '''Survey 8''' (LFI only): starts 1 February 2013, ends 1 August 2013.<br />
<br />
<br />
=== Completion of full sky coverage during Surveys 1-2 ===<br />
<br />
The picture gallery below exhibits the progress of sky coverage during the first months of survey (black colour = unobserved areas).<br />
<br />
<br />
<gallery widths=330 perrow=3 caption="HFI 353 GHz integration time after N months of survey. The units here are seconds per square degree, normalized to one detector."><br />
File:353_1month.png|After 1 month<br />
File:353_2month.png|After 2 months<br />
File:353_3month.png|After 3 months<br />
File:353_4month.png|After 4 months<br />
File:353_5month.png|After 5 months<br />
File:353_6month.png|After 6 months<br />
File:353_7month.png|After 7 months<br />
File:353_8month.png|After 8 months<br />
File:353_9months.png|After 9 months<br />
File:353_10months.png|After 10 months<br />
File:353_11months.png|After 11 months<br />
File:353_12months.png|After 12 months<br />
</gallery><br />
<br />
== Main planet and Crab observations ==<br />
<br />
Solar System objects and the Crab Nebula have been observed many times during the Planck surveys. Here is a list of these observations, with the ''deep rings'' (Jupiter and the Crab) and ''drift scans'' (Mars only) in '''boldface'''.<br />
<br />
* Crab: 16-22 September 2009<br />
<br />
* Mars: 17-29 October 2009<br />
<br />
* Jupiter: 25 October – 1 November 2009<br />
<br />
* Neptune: 1-8 November 2009<br />
<br />
* Uranus: 6-16 December 2009<br />
<br />
* Saturn: 2-8 January 2010<br />
<br />
* Crab: 6-12 March 2010<br />
<br />
* Mars: 9-18 April 2010<br />
<br />
* Neptune: 15-23 May 2010<br />
<br />
* Saturn: 13-22 June 2010<br />
<br />
* Uranus: 27 June – 5 July 2010<br />
<br />
* Jupiter: 1-9 July 2010<br />
<br />
* Crab: 15-21 September 2010<br />
<br />
* Neptune: 3-11 November 2010<br />
<br />
* Jupiter: 9-18 December 2010<br />
<br />
* Uranus: 12-21 December 2010<br />
<br />
* Saturn: 15-22 January 2011<br />
<br />
* Crab: 7-12 March 2011<br />
<br />
* Neptune: 18-26 May 2011<br />
<br />
* Saturn: 30 June - 9 July 2011<br />
<br />
* Uranus: 3-11 July 2011<br />
<br />
* Jupiter: 9-15 August 2011<br />
<br />
* Crab: 10-18 September 2011 (performed with the 250 deg. phase cycloidal strategy)<br />
<br />
* Crab: 20-23 September 2011 (performed with the 340 deg. phase cycloidal strategy)<br />
<br />
* '''Mars''': 8-16 December 2011 ("drift scan", Mars allowed to move through the Planck focal plane via its proper motion)<br />
<br />
* Mars: 17-26 December 2011 (normal scanning)<br />
<br />
* '''Jupiter''': 8-30 January 2012 (deep ring)<br />
<br />
* '''Crab''': 26 February - 16 March 2012 (deep ring)<br />
<br />
* '''Jupiter''': 1-14 September 2012 (deep ring)<br />
<br />
* '''Crab''': 14 September - 1 October 2012 (deep ring)<br />
<br />
* Neptune: 19-27 November 2012<br />
<br />
* Uranus: 24-30 December 2012<br />
<br />
* Saturn: 30 January - 5 February 2013<br />
<br />
* '''Jupiter''': February 2013 (deep ring)<br />
<br />
* '''Crab''': Feb. 28th - March 15th<br />
<br />
* Neptune: June 4th - June 12th<br />
<br />
== Resulting integration time distribution ==<br />
<br />
The integration time after the end of HFI operations (January 2012) is shown in the following picture gallery.<br />
<br />
Units are seconds per square degree, normalized to one detector, for all maps. The projection is full-sky Mollweide centred on the Galactic centre.<br />
<br />
<br />
<br />
<gallery widths=330px perrow=3 caption="Integration time after the end of HFI operations (January 2012). The units here are seconds per square degree, normalized to one detector."><br />
File:HFI_fullmission_100GHz1-4.png|HFI 100 GHz 1,4<br />
File:HFI_fullmission_100GHz2-3.png|HFI 100 GHz 2,3<br />
File:HFI_fullmission_143GHz1-4.png|HFI 143 GHz 1-4<br />
File:HFI_fullmission_143GHz5-8.png|HFI 143 GHz 5-8<br />
File:HFI_fullmission_217GHz1-4.png|HFI 217 GHz 1-4<br />
File:HFI_fullmission_217GHz5-8.png|HFI 217 GHz 5-8<br />
File:HFI_fullmission_353GHz.png|HFI 353 GHz<br />
File:HFI_fullmission_545-857GHz.png|HFI 545 GHz / 857 GHz<br />
File:LFI25_coldmission.png|LFI-25 (44 GHz)<br />
File:LFI27_coldmission.png|LFI 30 GHz<br />
</gallery><br />
<br />
==References==<br />
<references /><br />
<br />
[[Category:Introduction|004]]<br />
[[Category:PSOBook]]</div>
Xdupac
https://wiki.cosmos.esa.int/planckpla2015/index.php?title=Survey_scanning_and_performance&diff=11009
Survey scanning and performance
2015-02-03T16:07:23Z
<p>Xdupac: /* Main planet and Crab observations */</p>
<hr />
<div>== The observation strategy ==<br />
<br />
The Planck ''observation strategy'', or ''scanning strategy'', made use of the characteristics of the Planck spacecraft {{PlanckPapers|planck2011-1-1}} and orbit in order to achieve the survey goals in terms of sky coverage and scanning directions.<br />
<br />
The Planck focal plane scanned the sky in the way explained in the figure below.<br />
<br />
[[file:FocalPlane.png|thumb|300px|Planck focal plane showing the direction of scanning. Polarization-sensitive detectors are drawn with crosses indicating the polarization orientation.]]<br />
<br />
The 353 GHz row scanned the sky in small circles with an 85 deg. bore-sight angle from the spin axis. 545 GHz, 857 GHz, and 143 GHz bolometers, as well as LFI radiometers 25 and 26 had a slightly smaller bore-sight angle, while the other part of the Planck focal plane had larger ones (up to about 89 deg.). The Planck spacecraft spun at a rate of 1 rpm.<br />
<br />
Planck, being at L2, moved along the Ecliptic at approximately one degree per day, and needed to keep the Solar aspect angle below about 9 degrees at all times. In practice, during the surveys, the limit considered was 8 deg. Another celestial constraint is that the angle between the Planck spin axis and the anti-Earth direction could not exceed 15 deg. (relaxed to 17 deg. from Survey 5 onward). These constraints had a very direct influence on the chosen scanning strategy.<br />
<br />
[[File:ScannStrategy.png|thumb|300px|Simplified illustration of the Planck scanning strategy, without additional motion of the spin axis.]]<br />
<br />
[[File:Observing_strat.png|thumb|300px|left|Planck scanning strategy, showing the additional motion of the spin axis.]]<br />
<br />
The path followed by the Planck spin axis was defined with respect to the Ecliptic plane. It corresponded to a motion in longitude which maintained an anti-Sun pointing (about one degree per day), to which was added a cycloidal motion (precession) of the spin axis around the anti-Sun position (fiducial point). The cycloidal path was defined by the functions: <br />
<br />
$ λ = θ sin((-1)^n ω (t-t_0)+φ) $ (eq. 1),<br />
<br />
$β = -θ cos((-1)^n ω(t-t_0) + φ) $ (eq. 2),<br />
<br />
where λ is the angular distance from the fiducial point in Ecliptic longitude, β the angular distance from the fiducial point in Ecliptic latitude, θ the spin axis precession amplitude, ω the pulsation of the precession, φ its phase, n the parameter which controls the motion direction of the precession, t is the time, and $t_0$ is the first time during the Planck survey at which the fiducial point crosses the Ecliptic longitude =0 line.<br />
<br />
[[File:Cycloidal_scanning.JPG|thumb|300px|Spin axis path with a 7 deg. amplitude cycloidal scanning, from Ref.{{BibCite|dupac2005}}]]<br />
<br />
The reasons to decide to use such a precession of the spin axis are the following.<br />
<br />
* An excursion of the spin axis from the anti-Sun direction is required to fully observe the whole sky (no excursion would leave a large area unobserved around the Ecliptic poles).<br />
<br />
* The precession motion keeps the Sun aspect angle constant during the whole survey, therefore minimizing the thermal constraint variations on the spacecraft.<br />
<br />
The following precession parameters were chosen for the BSS.<br />
<br />
* Amplitude θ = 7.5deg. (this value is the lowest possible which allows the whole sky to be covered with all detectors).<br />
<br />
* n = 1 (anti-clockwise motion as seen from the Sun).<br />
<br />
* Pulsation ω = 2π / (half a year), faster precession was considered, and has interesting advantages, but was not possible given the constraints if one wants to keep a 7.5 deg. amplitude (which is necessary to cover the whole sky).<br />
<br />
* The phase of the precession was decided according to this set of criteria (in order of importance):<br />
<br />
a) respecting the operational constraints;<br />
<br />
b) allowing the largest possible angle between two scans on the Crab Nebula (a polarization calibrator);<br />
<br />
c) avoiding null dipole amplitude for the whole mission;<br />
<br />
d) optimizing the position of the planets in the beginning of the survey and with respect to the feasibility of their recovery;<br />
<br />
e) placing the two “deep fields” where Galactic foregrounds are minimum;<br />
<br />
f) allowing a reasonable survey margin (i.e. the time allowed to recover lost pointings if a problem occurs).<br />
<br />
The phase is 340 deg. for Surveys 1 to 4, and 250 deg. for Surveys 5 to 8.<br />
<br />
The scanning strategy for the second year of Routine Operations (i.e. Surveys 3 and 4) was exactly the same as for the first year, except that all pointings were shifted by 1 arcmin along the cross-scanning direction, in order to provide finer sky sampling for the highest frequency detectors when combining two years of observations.<br />
<br />
The change of phase between Survey 4 and Survey 5 occurred because it was found essential (especially on the HFI side) that scanning direction crossings should be increased in the Planck survey. By choosing a phase 90 deg. away from the original one, one optimizes the scanning strategy in this respect.<br />
<br />
The details of the justifications for these parameters can be found in PL-WG9-TN-001.<br />
<br />
The scanning strategy parameters are input to the PSO Survey Planning and Performance Tool, which is the software which generates the series of pointing records to be sent out to MOC for implementation.<br />
<br />
An approximate visualization of the Planck scanning strategy can be found [http://www.youtube.com/watch?v=WwFXuZ0B3B8 here] and [http://www.youtube.com/watch?v=7Zu-aiEiDtY here].<br />
<br />
<br />
===Spin axis manoeuvres and exact pointings===<br />
The motion of the spin axis was not continuous. Every change in the spin axis position was initiated by a manoeuvre which required less than 5 minutes time to complete. <br />
<br />
The duration between spin-axis manoeuvres is hereafter referred to as the “dwelling time" and the angular distance between manoeuvres along the spin axis path is hereafter referred to as the “spacing”. <br />
<br />
The dwelling times and spacings are defined as follows:<br />
<br />
* the spacings are fixed to 2arcmin, which roughly corresponds to the Nyquist criterion for sampling the highest-frequency HFI detectors;<br />
<br />
* the dwell times vary from 2360 s to 3904 s.<br />
The exact series of coordinates and dwell times are set by Eqs. (1) and (2) when one has fixed the spacings.<br />
<br />
== Data gap recoveries ==<br />
<br />
Gaps in the data flow can occur for various reasons.<br />
<br />
Anomalies may occur at spacecraft or instrument level, but also due to failures in the ground-to-spacecraft link or the ground segment itself. The adverse effects of such anomalies may be the loss of scientific data corresponding to one or several planned pointings, which have not been acquired and/or stored in memory.<br />
<br />
Failure to acquire proper scientific data may occur to one or both instruments.<br />
<br />
When a gap occurred, scientific criteria were applied to decide whether to recover the data through the Small-Gap Recovery procedure.<br />
<br />
[[File:AHF_353_OD389.png|thumb|400px|Integration time of the 353 GHz detectors ({{PlanckPapers|lamarre2010}}) after 389 Operational Days (the unit is seconds per square degree, normalized to one detector). The first significant data gap and recovery are clearly visible.]]<br />
<br />
The Small-Gap Recovery (SGR) procedure could be applied by MOC or PSO.<br />
<br />
* '''MOC-triggered SGR''': Within its nominal scheduling procedure for an OD, the MOC searches the PPL for PREF corresponding to the OD being processed and any pointings which are the subject of a Small Gap Recovery. As the PREF are sorted in chronological order according to their nominal start time, those corresponding to a small gap will naturally be the earliest. After checking attitude constraints, all observable pointings are listed and their dwell times reduced (initially) to the Minimum Dwell Time (MDT), as given in the PPL.<br />
Having included all valid PREF the required slew times are calculated. With the required slew times and minimum dwell times for all pointings, the OD schedule may be under-populated; in this case the dwell times of all scheduled pointings will be increased equally to make use of all available time in the OD. If the resulting schedule is over-populated, even with MDT for all pointings, the recovery cannot be constrained to a single OD. The sequence of pointings for the ODs involved is optimized in PREF scheduling and dwell times determined in order to effect the recovery and revert to the nominal timeline as quickly as possible.<br />
<br />
* '''PSO-triggered SGR''':<br />
PSO declares a small gap when pointings that have been executed result in data of insufficient quality or inadequate frequency coverage. This assessment is based on data quality and instrument health information provided by the DPCs. The algorithm that was used by the PSO to check the scientific validity of a pointing was implemented within the SPPT software tool. The SPPT ingested on a weekly basis a Weekly Health Report (WHR) for the HFI and LFI containing information on the working status of each detector and their expected condition over the following four weeks. On a daily basis, a Daily Quality Report (DQR) provided by the DPCs for both instruments, included a set of parameters that described the quality of the detection achieved by each individual detector for every pointing executed.<br />
<br />
The scheme for declaring a Small-Gap Recovery from PSO is the following.<br />
<br />
- If a pointing fails to meet the chosen requirement, it becomes an SGR candidate.<br />
<br />
- If there are at least 12 consecutive pointings which are declared SGR candidates, and the problem has been identified and solved, then an SGR is triggered.<br />
Recoveries are only carried out if the recovery slewing is guaranteed to be in OCM. MOC carried out this analysis and decided whether they should perform the SGR accordingly.<br />
<br />
- The start and end times of the gap and the list of the pointing numbers (or just the numbers of the first and last pointings to be recovered) were then sent to MOC by E-mail, with the notification to start a Small-Gap Recovery.<br />
<br />
- MOC implemented the Small-Gap Recovery, provided the pointings could still be scheduled with respect to their latest start time, using the same scheme as described in the MOC-triggered SGR section<br />
<br />
Throughout the Planck mission, data losses were very rare. In fact Small-Gap Recovery was applied only a couple of times.<br />
<br />
==Special observations==<br />
The special observations are now described.<br />
<br />
* Normal scanning on Solar System objects for calibration purposes.<br />
<br />
[[File:Crab_Nebula.jpg|thumb|200px|The Crab Nebula (Messier 1, NGC 1952, Taurus A), here seen by the Hubble Space Telescope.]]<br />
<br />
[[File:Mars.jpg|thumb|200px|Mars as seen by the Hubble Space Telescope in 1999.]]<br />
<br />
This concerns the following objects (specifically planets): Mars; Jupiter; Saturn; Uranus; and Neptune. Their thermal emission in the far-infrared and the small angular sizes make them ideal calibrators for bolometers and radiometers.<br />
<br />
Mars is a particularly interesting calibrator for Planck, because of its proper motion.<br />
However this proper motion makes it difficult to observe it many times during the mission.<br />
<br />
Jupiter is the brightest source for (non-polarized) calibration. Saturn was also used significantly, with Uranus and Neptune being secondary calibrators.<br />
<br />
* Normal scanning on other (non-moving) sources for calibration purposes.<br />
<br />
This concerns mostly the Crab Nebula for polarization calibration purposes.<br />
This supernova remnant is highly polarized, and as such represents the main polarization calibrator for Planck.<br />
<br />
* Special pointings during the calibration phase, not relative to celestial sources.<br />
<br />
* "Deep rings," special observations that were performed on each passage of Jupiter and the Crab Nebula, from January 2012 onward.<br />
<br />
These consist of very deeply sampled observations (0.5') with the spin axis along the Ecliptic plane, typically lasting two to three weeks.<br />
<br />
Such observations benefit from special relaxing of the celestial constraints, with Solar Aspect Angles < 9 deg. rather than < 8 deg. during cycloidal surveying.<br />
<br />
* "Drift scans," special observations performed on Mars, making use of its proper motion.<br />
<br />
==Start and end of surveys==<br />
<br />
The completion of a given “survey” is declared when the logical AND of all frequency-coverage maps is greater than 95 %, OR the sky has been surveyed over a consecutive period of 7.5 months. Note that this definition is that of the Project Scientist and Planck Science Office. Data processing centres do not use exactly the same concept of surveys to create "survey" maps.<br />
<br />
In practice, since the gaps during the surveys have always been very small, this results in approximately 6 months per survey.<br />
<br />
[[File:PlanckMissionTimeline.JPG|thumb|300px|Planck mission timeline with the distribution of the "sky surveys".]]<br />
<br />
* '''Survey 1''': starts 13 August 2009, ends 13 February 2010.<br />
<br />
* '''Survey 2''': starts 14 February 2010, ends 13 August 2010.<br />
<br />
* '''Survey 3''': starts 14 August 2010, ends 13 February 2011.<br />
<br />
* '''Survey 4''': starts 14 February 2011, ends 29 July 2011.<br />
<br />
(This survey was shortened in ordered to start earlier with the new scanning strategy; see above).<br />
<br />
* '''Survey 5''': starts 29 July 2011, ends 30 January 2012.<br />
<br />
* '''Survey 6''' (LFI only): starts 30 January 2012, ends 31 July 2012.<br />
<br />
* '''Survey 7''' (LFI only): starts 31 July 2012, ends 31 January 2013.<br />
<br />
* '''Survey 8''' (LFI only): starts 1 February 2013, ends 1 August 2013.<br />
<br />
<br />
=== Completion of full sky coverage during Surveys 1-2 ===<br />
<br />
The picture gallery below exhibits the progress of sky coverage during the first months of survey (black colour = unobserved areas).<br />
<br />
<br />
<gallery widths=330 perrow=3 caption="HFI 353 GHz integration time after N months of survey. The units here are seconds per square degree, normalized to one detector."><br />
File:353_1month.png|After 1 month<br />
File:353_2month.png|After 2 months<br />
File:353_3month.png|After 3 months<br />
File:353_4month.png|After 4 months<br />
File:353_5month.png|After 5 months<br />
File:353_6month.png|After 6 months<br />
File:353_7month.png|After 7 months<br />
File:353_8month.png|After 8 months<br />
File:353_9months.png|After 9 months<br />
File:353_10months.png|After 10 months<br />
File:353_11months.png|After 11 months<br />
File:353_12months.png|After 12 months<br />
</gallery><br />
<br />
== Main planet and Crab observations ==<br />
<br />
Solar System objects and the Crab Nebula have been observed many times during the Planck surveys. Here is a list of these observations, with the ''deep rings'' (Jupiter and the Crab) and ''drift scans'' (Mars only) in '''boldface'''.<br />
<br />
* Crab: 16-22 September 2009<br />
<br />
* Mars: 17-29 October 2009<br />
<br />
* Jupiter: 25 October – 1 November 2009<br />
<br />
* Neptune: 1-8 November 2009<br />
<br />
* Uranus: 6-16 December 2009<br />
<br />
* Saturn: 2-8 January 2010<br />
<br />
* Crab: 6-12 March 2010<br />
<br />
* Mars: 9-18 April 2010<br />
<br />
* Neptune: 15-23 May 2010<br />
<br />
* Saturn: 13-22 June 2010<br />
<br />
* Uranus: 27 June – 5 July 2010<br />
<br />
* Jupiter: 1-9 July 2010<br />
<br />
* Crab: 15-21 September 2010<br />
<br />
* Neptune: 3-11 November 2010<br />
<br />
* Jupiter: 9-18 December 2010<br />
<br />
* Uranus: 12-21 December 2010<br />
<br />
* Saturn: 15-22 January 2011<br />
<br />
* Crab: 7-12 March 2011<br />
<br />
* Neptune: 18-26 May 2011<br />
<br />
* Saturn: 30 June - 9 July 2011<br />
<br />
* Uranus: 3-11 July 2011<br />
<br />
* Jupiter: 9-15 August 2011<br />
<br />
* Crab: 10-18 September 2011 (performed with the 250 deg. phase cycloidal strategy)<br />
<br />
* Crab: 20-23 September 2011 (performed with the 340 deg. phase cycloidal strategy)<br />
<br />
* '''Mars''': 8-16 December 2011 ("drift scan", Mars allowed to move through the Planck focal plane via its proper motion)<br />
<br />
* Mars: 17-26 December 2011 (normal scanning)<br />
<br />
* '''Jupiter''': 8-30 January 2012 (deep ring)<br />
<br />
* '''Crab''': 26 February - 16 March 2012 (deep ring)<br />
<br />
* '''Jupiter''': 1-14 September 2012 (deep ring)<br />
<br />
* '''Crab''': 14 September - 1 October 2012 (deep ring)<br />
<br />
* Neptune: 19-27 November 2012<br />
<br />
* Uranus: 24-30 December 2012<br />
<br />
* Saturn: 30 January - 5 February 2013<br />
<br />
* '''Jupiter''': February 2013 (deep ring)<br />
<br />
== Resulting integration time distribution ==<br />
<br />
The integration time after the end of HFI operations (January 2012) is shown in the following picture gallery.<br />
<br />
Units are seconds per square degree, normalized to one detector, for all maps. The projection is full-sky Mollweide centred on the Galactic centre.<br />
<br />
<br />
<br />
<gallery widths=330px perrow=3 caption="Integration time after the end of HFI operations (January 2012). The units here are seconds per square degree, normalized to one detector."><br />
File:HFI_fullmission_100GHz1-4.png|HFI 100 GHz 1,4<br />
File:HFI_fullmission_100GHz2-3.png|HFI 100 GHz 2,3<br />
File:HFI_fullmission_143GHz1-4.png|HFI 143 GHz 1-4<br />
File:HFI_fullmission_143GHz5-8.png|HFI 143 GHz 5-8<br />
File:HFI_fullmission_217GHz1-4.png|HFI 217 GHz 1-4<br />
File:HFI_fullmission_217GHz5-8.png|HFI 217 GHz 5-8<br />
File:HFI_fullmission_353GHz.png|HFI 353 GHz<br />
File:HFI_fullmission_545-857GHz.png|HFI 545 GHz / 857 GHz<br />
File:LFI25_coldmission.png|LFI-25 (44 GHz)<br />
File:LFI27_coldmission.png|LFI 30 GHz<br />
</gallery><br />
<br />
==References==<br />
<references /><br />
<br />
[[Category:Introduction|004]]<br />
[[Category:PSOBook]]</div>
Xdupac
https://wiki.cosmos.esa.int/planckpla2015/index.php?title=Survey_scanning_and_performance&diff=11008
Survey scanning and performance
2015-02-03T16:06:45Z
<p>Xdupac: /* Main planet and Crab observations during Surveys 1-7 */</p>
<hr />
<div>== The observation strategy ==<br />
<br />
The Planck ''observation strategy'', or ''scanning strategy'', made use of the characteristics of the Planck spacecraft {{PlanckPapers|planck2011-1-1}} and orbit in order to achieve the survey goals in terms of sky coverage and scanning directions.<br />
<br />
The Planck focal plane scanned the sky in the way explained in the figure below.<br />
<br />
[[file:FocalPlane.png|thumb|300px|Planck focal plane showing the direction of scanning. Polarization-sensitive detectors are drawn with crosses indicating the polarization orientation.]]<br />
<br />
The 353 GHz row scanned the sky in small circles with an 85 deg. bore-sight angle from the spin axis. 545 GHz, 857 GHz, and 143 GHz bolometers, as well as LFI radiometers 25 and 26 had a slightly smaller bore-sight angle, while the other part of the Planck focal plane had larger ones (up to about 89 deg.). The Planck spacecraft spun at a rate of 1 rpm.<br />
<br />
Planck, being at L2, moved along the Ecliptic at approximately one degree per day, and needed to keep the Solar aspect angle below about 9 degrees at all times. In practice, during the surveys, the limit considered was 8 deg. Another celestial constraint is that the angle between the Planck spin axis and the anti-Earth direction could not exceed 15 deg. (relaxed to 17 deg. from Survey 5 onward). These constraints had a very direct influence on the chosen scanning strategy.<br />
<br />
[[File:ScannStrategy.png|thumb|300px|Simplified illustration of the Planck scanning strategy, without additional motion of the spin axis.]]<br />
<br />
[[File:Observing_strat.png|thumb|300px|left|Planck scanning strategy, showing the additional motion of the spin axis.]]<br />
<br />
The path followed by the Planck spin axis was defined with respect to the Ecliptic plane. It corresponded to a motion in longitude which maintained an anti-Sun pointing (about one degree per day), to which was added a cycloidal motion (precession) of the spin axis around the anti-Sun position (fiducial point). The cycloidal path was defined by the functions: <br />
<br />
$ λ = θ sin((-1)^n ω (t-t_0)+φ) $ (eq. 1),<br />
<br />
$β = -θ cos((-1)^n ω(t-t_0) + φ) $ (eq. 2),<br />
<br />
where λ is the angular distance from the fiducial point in Ecliptic longitude, β the angular distance from the fiducial point in Ecliptic latitude, θ the spin axis precession amplitude, ω the pulsation of the precession, φ its phase, n the parameter which controls the motion direction of the precession, t is the time, and $t_0$ is the first time during the Planck survey at which the fiducial point crosses the Ecliptic longitude =0 line.<br />
<br />
[[File:Cycloidal_scanning.JPG|thumb|300px|Spin axis path with a 7 deg. amplitude cycloidal scanning, from Ref.{{BibCite|dupac2005}}]]<br />
<br />
The reasons to decide to use such a precession of the spin axis are the following.<br />
<br />
* An excursion of the spin axis from the anti-Sun direction is required to fully observe the whole sky (no excursion would leave a large area unobserved around the Ecliptic poles).<br />
<br />
* The precession motion keeps the Sun aspect angle constant during the whole survey, therefore minimizing the thermal constraint variations on the spacecraft.<br />
<br />
The following precession parameters were chosen for the BSS.<br />
<br />
* Amplitude θ = 7.5deg. (this value is the lowest possible which allows the whole sky to be covered with all detectors).<br />
<br />
* n = 1 (anti-clockwise motion as seen from the Sun).<br />
<br />
* Pulsation ω = 2π / (half a year), faster precession was considered, and has interesting advantages, but was not possible given the constraints if one wants to keep a 7.5 deg. amplitude (which is necessary to cover the whole sky).<br />
<br />
* The phase of the precession was decided according to this set of criteria (in order of importance):<br />
<br />
a) respecting the operational constraints;<br />
<br />
b) allowing the largest possible angle between two scans on the Crab Nebula (a polarization calibrator);<br />
<br />
c) avoiding null dipole amplitude for the whole mission;<br />
<br />
d) optimizing the position of the planets in the beginning of the survey and with respect to the feasibility of their recovery;<br />
<br />
e) placing the two “deep fields” where Galactic foregrounds are minimum;<br />
<br />
f) allowing a reasonable survey margin (i.e. the time allowed to recover lost pointings if a problem occurs).<br />
<br />
The phase is 340 deg. for Surveys 1 to 4, and 250 deg. for Surveys 5 to 8.<br />
<br />
The scanning strategy for the second year of Routine Operations (i.e. Surveys 3 and 4) was exactly the same as for the first year, except that all pointings were shifted by 1 arcmin along the cross-scanning direction, in order to provide finer sky sampling for the highest frequency detectors when combining two years of observations.<br />
<br />
The change of phase between Survey 4 and Survey 5 occurred because it was found essential (especially on the HFI side) that scanning direction crossings should be increased in the Planck survey. By choosing a phase 90 deg. away from the original one, one optimizes the scanning strategy in this respect.<br />
<br />
The details of the justifications for these parameters can be found in PL-WG9-TN-001.<br />
<br />
The scanning strategy parameters are input to the PSO Survey Planning and Performance Tool, which is the software which generates the series of pointing records to be sent out to MOC for implementation.<br />
<br />
An approximate visualization of the Planck scanning strategy can be found [http://www.youtube.com/watch?v=WwFXuZ0B3B8 here] and [http://www.youtube.com/watch?v=7Zu-aiEiDtY here].<br />
<br />
<br />
===Spin axis manoeuvres and exact pointings===<br />
The motion of the spin axis was not continuous. Every change in the spin axis position was initiated by a manoeuvre which required less than 5 minutes time to complete. <br />
<br />
The duration between spin-axis manoeuvres is hereafter referred to as the “dwelling time" and the angular distance between manoeuvres along the spin axis path is hereafter referred to as the “spacing”. <br />
<br />
The dwelling times and spacings are defined as follows:<br />
<br />
* the spacings are fixed to 2arcmin, which roughly corresponds to the Nyquist criterion for sampling the highest-frequency HFI detectors;<br />
<br />
* the dwell times vary from 2360 s to 3904 s.<br />
The exact series of coordinates and dwell times are set by Eqs. (1) and (2) when one has fixed the spacings.<br />
<br />
== Data gap recoveries ==<br />
<br />
Gaps in the data flow can occur for various reasons.<br />
<br />
Anomalies may occur at spacecraft or instrument level, but also due to failures in the ground-to-spacecraft link or the ground segment itself. The adverse effects of such anomalies may be the loss of scientific data corresponding to one or several planned pointings, which have not been acquired and/or stored in memory.<br />
<br />
Failure to acquire proper scientific data may occur to one or both instruments.<br />
<br />
When a gap occurred, scientific criteria were applied to decide whether to recover the data through the Small-Gap Recovery procedure.<br />
<br />
[[File:AHF_353_OD389.png|thumb|400px|Integration time of the 353 GHz detectors ({{PlanckPapers|lamarre2010}}) after 389 Operational Days (the unit is seconds per square degree, normalized to one detector). The first significant data gap and recovery are clearly visible.]]<br />
<br />
The Small-Gap Recovery (SGR) procedure could be applied by MOC or PSO.<br />
<br />
* '''MOC-triggered SGR''': Within its nominal scheduling procedure for an OD, the MOC searches the PPL for PREF corresponding to the OD being processed and any pointings which are the subject of a Small Gap Recovery. As the PREF are sorted in chronological order according to their nominal start time, those corresponding to a small gap will naturally be the earliest. After checking attitude constraints, all observable pointings are listed and their dwell times reduced (initially) to the Minimum Dwell Time (MDT), as given in the PPL.<br />
Having included all valid PREF the required slew times are calculated. With the required slew times and minimum dwell times for all pointings, the OD schedule may be under-populated; in this case the dwell times of all scheduled pointings will be increased equally to make use of all available time in the OD. If the resulting schedule is over-populated, even with MDT for all pointings, the recovery cannot be constrained to a single OD. The sequence of pointings for the ODs involved is optimized in PREF scheduling and dwell times determined in order to effect the recovery and revert to the nominal timeline as quickly as possible.<br />
<br />
* '''PSO-triggered SGR''':<br />
PSO declares a small gap when pointings that have been executed result in data of insufficient quality or inadequate frequency coverage. This assessment is based on data quality and instrument health information provided by the DPCs. The algorithm that was used by the PSO to check the scientific validity of a pointing was implemented within the SPPT software tool. The SPPT ingested on a weekly basis a Weekly Health Report (WHR) for the HFI and LFI containing information on the working status of each detector and their expected condition over the following four weeks. On a daily basis, a Daily Quality Report (DQR) provided by the DPCs for both instruments, included a set of parameters that described the quality of the detection achieved by each individual detector for every pointing executed.<br />
<br />
The scheme for declaring a Small-Gap Recovery from PSO is the following.<br />
<br />
- If a pointing fails to meet the chosen requirement, it becomes an SGR candidate.<br />
<br />
- If there are at least 12 consecutive pointings which are declared SGR candidates, and the problem has been identified and solved, then an SGR is triggered.<br />
Recoveries are only carried out if the recovery slewing is guaranteed to be in OCM. MOC carried out this analysis and decided whether they should perform the SGR accordingly.<br />
<br />
- The start and end times of the gap and the list of the pointing numbers (or just the numbers of the first and last pointings to be recovered) were then sent to MOC by E-mail, with the notification to start a Small-Gap Recovery.<br />
<br />
- MOC implemented the Small-Gap Recovery, provided the pointings could still be scheduled with respect to their latest start time, using the same scheme as described in the MOC-triggered SGR section<br />
<br />
Throughout the Planck mission, data losses were very rare. In fact Small-Gap Recovery was applied only a couple of times.<br />
<br />
==Special observations==<br />
The special observations are now described.<br />
<br />
* Normal scanning on Solar System objects for calibration purposes.<br />
<br />
[[File:Crab_Nebula.jpg|thumb|200px|The Crab Nebula (Messier 1, NGC 1952, Taurus A), here seen by the Hubble Space Telescope.]]<br />
<br />
[[File:Mars.jpg|thumb|200px|Mars as seen by the Hubble Space Telescope in 1999.]]<br />
<br />
This concerns the following objects (specifically planets): Mars; Jupiter; Saturn; Uranus; and Neptune. Their thermal emission in the far-infrared and the small angular sizes make them ideal calibrators for bolometers and radiometers.<br />
<br />
Mars is a particularly interesting calibrator for Planck, because of its proper motion.<br />
However this proper motion makes it difficult to observe it many times during the mission.<br />
<br />
Jupiter is the brightest source for (non-polarized) calibration. Saturn was also used significantly, with Uranus and Neptune being secondary calibrators.<br />
<br />
* Normal scanning on other (non-moving) sources for calibration purposes.<br />
<br />
This concerns mostly the Crab Nebula for polarization calibration purposes.<br />
This supernova remnant is highly polarized, and as such represents the main polarization calibrator for Planck.<br />
<br />
* Special pointings during the calibration phase, not relative to celestial sources.<br />
<br />
* "Deep rings," special observations that were performed on each passage of Jupiter and the Crab Nebula, from January 2012 onward.<br />
<br />
These consist of very deeply sampled observations (0.5') with the spin axis along the Ecliptic plane, typically lasting two to three weeks.<br />
<br />
Such observations benefit from special relaxing of the celestial constraints, with Solar Aspect Angles < 9 deg. rather than < 8 deg. during cycloidal surveying.<br />
<br />
* "Drift scans," special observations performed on Mars, making use of its proper motion.<br />
<br />
==Start and end of surveys==<br />
<br />
The completion of a given “survey” is declared when the logical AND of all frequency-coverage maps is greater than 95 %, OR the sky has been surveyed over a consecutive period of 7.5 months. Note that this definition is that of the Project Scientist and Planck Science Office. Data processing centres do not use exactly the same concept of surveys to create "survey" maps.<br />
<br />
In practice, since the gaps during the surveys have always been very small, this results in approximately 6 months per survey.<br />
<br />
[[File:PlanckMissionTimeline.JPG|thumb|300px|Planck mission timeline with the distribution of the "sky surveys".]]<br />
<br />
* '''Survey 1''': starts 13 August 2009, ends 13 February 2010.<br />
<br />
* '''Survey 2''': starts 14 February 2010, ends 13 August 2010.<br />
<br />
* '''Survey 3''': starts 14 August 2010, ends 13 February 2011.<br />
<br />
* '''Survey 4''': starts 14 February 2011, ends 29 July 2011.<br />
<br />
(This survey was shortened in ordered to start earlier with the new scanning strategy; see above).<br />
<br />
* '''Survey 5''': starts 29 July 2011, ends 30 January 2012.<br />
<br />
* '''Survey 6''' (LFI only): starts 30 January 2012, ends 31 July 2012.<br />
<br />
* '''Survey 7''' (LFI only): starts 31 July 2012, ends 31 January 2013.<br />
<br />
* '''Survey 8''' (LFI only): starts 1 February 2013, ends 1 August 2013.<br />
<br />
<br />
=== Completion of full sky coverage during Surveys 1-2 ===<br />
<br />
The picture gallery below exhibits the progress of sky coverage during the first months of survey (black colour = unobserved areas).<br />
<br />
<br />
<gallery widths=330 perrow=3 caption="HFI 353 GHz integration time after N months of survey. The units here are seconds per square degree, normalized to one detector."><br />
File:353_1month.png|After 1 month<br />
File:353_2month.png|After 2 months<br />
File:353_3month.png|After 3 months<br />
File:353_4month.png|After 4 months<br />
File:353_5month.png|After 5 months<br />
File:353_6month.png|After 6 months<br />
File:353_7month.png|After 7 months<br />
File:353_8month.png|After 8 months<br />
File:353_9months.png|After 9 months<br />
File:353_10months.png|After 10 months<br />
File:353_11months.png|After 11 months<br />
File:353_12months.png|After 12 months<br />
</gallery><br />
<br />
== Main planet and Crab observations ==<br />
<br />
Solar System objects and the Crab Nebula have been observed many times during the Planck surveys. Here is a complete list of these observations, with the ''deep rings'' (Jupiter and the Crab) and ''drift scans'' (Mars only) in '''boldface'''.<br />
<br />
* Crab: 16-22 September 2009<br />
<br />
* Mars: 17-29 October 2009<br />
<br />
* Jupiter: 25 October – 1 November 2009<br />
<br />
* Neptune: 1-8 November 2009<br />
<br />
* Uranus: 6-16 December 2009<br />
<br />
* Saturn: 2-8 January 2010<br />
<br />
* Crab: 6-12 March 2010<br />
<br />
* Mars: 9-18 April 2010<br />
<br />
* Neptune: 15-23 May 2010<br />
<br />
* Saturn: 13-22 June 2010<br />
<br />
* Uranus: 27 June – 5 July 2010<br />
<br />
* Jupiter: 1-9 July 2010<br />
<br />
* Crab: 15-21 September 2010<br />
<br />
* Neptune: 3-11 November 2010<br />
<br />
* Jupiter: 9-18 December 2010<br />
<br />
* Uranus: 12-21 December 2010<br />
<br />
* Saturn: 15-22 January 2011<br />
<br />
* Crab: 7-12 March 2011<br />
<br />
* Neptune: 18-26 May 2011<br />
<br />
* Saturn: 30 June - 9 July 2011<br />
<br />
* Uranus: 3-11 July 2011<br />
<br />
* Jupiter: 9-15 August 2011<br />
<br />
* Crab: 10-18 September 2011 (performed with the 250 deg. phase cycloidal strategy)<br />
<br />
* Crab: 20-23 September 2011 (performed with the 340 deg. phase cycloidal strategy)<br />
<br />
* '''Mars''': 8-16 December 2011 ("drift scan", Mars allowed to move through the Planck focal plane via its proper motion)<br />
<br />
* Mars: 17-26 December 2011 (normal scanning)<br />
<br />
* '''Jupiter''': 8-30 January 2012 (deep ring)<br />
<br />
* '''Crab''': 26 February - 16 March 2012 (deep ring)<br />
<br />
* '''Jupiter''': 1-14 September 2012 (deep ring)<br />
<br />
* '''Crab''': 14 September - 1 October 2012 (deep ring)<br />
<br />
* Neptune: 19-27 November 2012<br />
<br />
* Uranus: 24-30 December 2012<br />
<br />
* Saturn: 30 January - 5 February 2013<br />
<br />
* '''Jupiter''': February 2013 (deep ring)<br />
<br />
== Resulting integration time distribution ==<br />
<br />
The integration time after the end of HFI operations (January 2012) is shown in the following picture gallery.<br />
<br />
Units are seconds per square degree, normalized to one detector, for all maps. The projection is full-sky Mollweide centred on the Galactic centre.<br />
<br />
<br />
<br />
<gallery widths=330px perrow=3 caption="Integration time after the end of HFI operations (January 2012). The units here are seconds per square degree, normalized to one detector."><br />
File:HFI_fullmission_100GHz1-4.png|HFI 100 GHz 1,4<br />
File:HFI_fullmission_100GHz2-3.png|HFI 100 GHz 2,3<br />
File:HFI_fullmission_143GHz1-4.png|HFI 143 GHz 1-4<br />
File:HFI_fullmission_143GHz5-8.png|HFI 143 GHz 5-8<br />
File:HFI_fullmission_217GHz1-4.png|HFI 217 GHz 1-4<br />
File:HFI_fullmission_217GHz5-8.png|HFI 217 GHz 5-8<br />
File:HFI_fullmission_353GHz.png|HFI 353 GHz<br />
File:HFI_fullmission_545-857GHz.png|HFI 545 GHz / 857 GHz<br />
File:LFI25_coldmission.png|LFI-25 (44 GHz)<br />
File:LFI27_coldmission.png|LFI 30 GHz<br />
</gallery><br />
<br />
==References==<br />
<references /><br />
<br />
[[Category:Introduction|004]]<br />
[[Category:PSOBook]]</div>
Xdupac
https://wiki.cosmos.esa.int/planckpla2015/index.php?title=Specially_processed_maps&diff=11007
Specially processed maps
2015-02-03T16:05:48Z
<p>Xdupac: </p>
<hr />
<div>{{DISPLAYTITLE:Additional maps}}<br />
==Introduction==<br />
<br />
This section describes the products that required special processing.<br />
<br />
== Lensing map ==<br />
<br />
We distribute the minimum-variance (MV) lensing potential estimate presented in {{PlanckPapers|planck2014-xxx}} as part of the 2014 data release. This map represents an estimate of the CMB lensing potential on approximately 70% of the sky, and also forms the basis for the Planck 2014 lensing likelihood. It is produced using filtered temperature and polarization data from the SMICA DX11 CMB map; its construction is discussed in detail in {{PlanckPapers|planck2014-xxx}}.<br />
<br />
<br />
The estimate is contained in a single gzipped tarball named ''{{PLASingleFile|fileType=map|name=COM_CompMap_Lensing_2048_R2.00.tgz|link=COM_CompMap_Lensing_2048_R2.00.tgz}}''. Its contents are described below.<br />
<br />
<br />
<br />
{| border="1" cellpadding="3" cellspacing="0" align="center" style="text-align:left"<br />
|+ ''' Contents of Lensing package '''<br />
|- bgcolor="ffdead" <br />
! Filename || Format || Description<br />
|-<br />
| dat_klm.fits || HEALPIX FITS format alm, with <math> L_{\rm max} = 2048 </math> || Contains the estimated lensing convergence <math> \hat{\kappa}_{LM} = \frac{1}{2} L(L+1)\hat{\phi}_{LM} </math>.<br />
|-<br />
| mask.fits.gz || HEALPIX FITS format map, with <math> N_{\rm side} = 2048 </math> || Contains the lens reconstruction analysis mask.<br />
|-<br />
| nlkk.dat || ASCII text file, with columns = (<math>L</math>, <math>N_L </math>, <math>C_L+N_L</math>) || The approximate noise <math>N_L</math> (and signal+noise, <math>C_L+N_L</math>) power spectrum of <math> \hat{\kappa}_{LM} </math>, for the fiducial cosmology used in {{PlanckPapers|planck2014-xxx}}.<br />
|}<br />
<br />
<br />
== Compton parameter map ==<br />
<br />
We distribute here the Planck full mission Compton parameter maps (y-maps hereafter) obtained using the NILC and MILCA component separation algorithms as described in {{PlanckPapers|planck2014-xxii}}. We also provide the ILC weights per scale and per frequency that were used to produce these y-maps. IDL routines are also provide to allow the user to apply those weights. Compton parameters produced by keeping either the first or the second half of stable pointing periods are also provide and we call them FIRST and LAST y-maps. Additionally we construct a noise estimates of full mission Planck y-maps from the half difference of the FIRST and LAST y-maps. These estimates are used to construct standard deviation maps of the noise in the full mission Planck y-maps that are also provided. To complement this we also provide the power spectra of the noise estimate maps after correcting for inhomogeneities using the standard deviation maps. We also deliver foreground masks including point-source and galactic masks.<br />
<br />
The full data set is contained in a single gzipped tarball named ''{{PLASingleFile|fileType=map|name=ymap_R0.00.tgz|link=ymap_R0.00.tgz}}''. Its contents are described below.<br />
<br />
<br />
<br />
{| border="1" cellpadding="3" cellspacing="0" align="center" style="text-align:left"<br />
|+ ''' Contents of {{PLASingleFile|fileType=map|name=ymap_R0.00.tgz|link=ymap_R0.00.tgz}} '''<br />
|- bgcolor="ffdead" <br />
! Filename || Format || Description<br />
|-<br />
| nilc_ymaps.fits || HEALPIX FITS format map in Galactic coordinates with <math> N_{\rm side} = 2048 </math>|| Contains the NILC full mission, FIRST and LAST ymaps.<br />
|-<br />
| milca_ymaps.fits || HEALPIX FITS format map in Galactic coordinates with <math> N_{\rm side} = 2048 </math> || Contains the MILCA full mission, FIRST and LAST ymaps.<br />
|-<br />
| nilc_weights_BAND.fits || HEALPIX FITS format map in Galactic coordinates with <math> N_{\rm side} = 128 </math>|| Contains the NILC ILC weights for the full mission ymap for band BAND 0 to 9. For each band we provide a weight map per frequency.<br />
|-<br />
| milca_FREQ_Csz.fits || HEALPIX FITS format map in Galactic coordinates with <math> N_{\rm side} = 2048 </math> || Contains the MILCA ILC weights for the full mission ymap for frequency FREQ (100,143,217,353,545,857). For each frequency we provide a weight map per filter band.<br />
|-<br />
| nilc_stddev.fits || HEALPIX FITS format map in Galactic coordinates with <math> N_{\rm side} = 2048 </math>|| Contains the stddev map for the NILC full mission y-map.<br />
|-<br />
| milca_stddev.fits || HEALPIX FITS format map in Galactic coordinates with <math> N_{\rm side} = 2048 </math> || Contains the stddev maps for the MILCA full mission ymap.<br />
|-<br />
| nilc_homnoise_spect.fits || ASCII table FITS format || Contains the angular power spectrum of the homogeneous noise in the NILC full mission ymap.<br />
|-<br />
| milca_homnoise_spect.fits || ASCII table FITS format || Contains the angular power spectrum of the homogeneous noise in the MILCA full mission ymap.<br />
|-<br />
| masks.fits || HEALPIX FITS format map, with <math> N_{\rm side} = 2048 </math> || Contains foreground masks.<br />
|-<br />
| nilc_bands.fits || ASCII table FITS format || Contains NILC wavelet bands in multipole space<br />
|}<br />
<!---<br />
== IRAM Maps of the Crab nebula ==<br />
<br />
Maps of the Crab nebula at 89.189 GHz (HCO+(1-0) transition) in both temperature and polarization, prodouced from observations performed at the IRAM 30m telescope from January 9th to January 12th 2009, are delivered as a tarball of 416 KB in the file<br />
<br />
: [[File:Crab_IRAM_2010.zip]]<br />
<br />
See README in the tarball for full details. These data were used in{{BibCite|aumont2010}}<br />
---><br />
<br />
<br />
==References==<br />
<References /><br />
<br />
<br />
<br />
<br />
<br />
[[Category:Mission products|010]]</div>
Xdupac
https://wiki.cosmos.esa.int/planckpla2015/index.php?title=SREM&diff=11006
SREM
2015-02-03T16:04:34Z
<p>Xdupac: /* Product description */</p>
<hr />
<div>==Product description==<br />
The SREM data files contain calibrated data for the different energy and particle species channels available in the SREM. Each data file contains 24 hours of data - from midnight to midnight UTC. (note that this is '''different from an Operational Day''') - with the date covered by the file easily identifiable through the file name.<br />
<br />
==Inputs==<br />
SREM calibrated data was produced from the SREM raw data acquired during the entire mission.<br />
<br />
==Related products==<br />
Data for the SREM on board other ESA missions can be retrieved from the Paul Scherrer Institute [http://www.psi.ch]. In order to retrieve the data you will need to register first.<br />
<br />
==Data files==<br />
The files containing the SREM calibrated data will have a name of the form SREMPlanck_PACC_YYYYMMDD.fits where PACC stands for Processed ACCumulated data and YYYYMMDD is the date the data in the file was acquired.<br />
<br />
The SREM processed data can be downloaded from the PLA interface: "Ancillary data" tab of the "Time-ordered information" section.<br />
<br />
A list of the files available can be found {{PLAProductsV2|product=opdata|link=here}}.<br />
<br />
===Data format===<br />
Each file contains three binary table extensions named CDFFITS1,CDFFITS2 and CDFFITS3. The first extension contains the accumulated counts data, the second extension the labels to identify the data in the first extension and the third extension the total radiation dosis. The contents of each extension are as follows.<br />
{| border="1" cellspacing="0" cellpadding="2" align="center"<br />
|+ '''CDFFITS1'''<br />
|-<br />
!scope="col"| Column Name<br />
!scope="col"| Contents<br />
!scope="col"| Format<br />
!scope="col"| Unit<br />
|-<br />
!scope="row" align="left" width="150"| EPOCH<br />
| width="550" | vector containing 1 string with UTC for center of accumulation interval in ISO format (YYYY-MM-DDTHH:MM:SS.MMMZ)<br />
|A24<br />
| NA<br />
|-<br />
!scope="row" align="left"| COUNTRATE<br />
| vector containing 15 elements (1 for each channel) with counts for accumulation period identified in the EPOCH column <br />
|E15.4<br />
| s<math>^{-1}</math><br />
|-<br />
!scope="row" align="left"| ORBIT<br />
| position (x,y,z) of the SREM in the ECI frame. Distance from center fo the Earth is <math>R=\sqrt(x^2+y^2+z^2)</math><br />
|E15.4<br />
| km<br />
|-<br />
!scope="row" align="left"| ATTITUDE<br />
| Not in use<br />
|E15.4<br />
| -<br />
|-<br />
!scope="row" align="left"| PROT FITQUAL<br />
| Not in use<br />
|I1<br />
| NA<br />
|-<br />
!scope="row" align="left"| ODPF<br />
| Not in use.<br />
|E15.4<br />
| -<br />
|-<br />
!scope="row" align="left"| ODPFERR<br />
| Not in use<br />
|E15.4<br />
| -<br />
|-<br />
!scope="row" align="left"| ELEC FITQUAL<br />
| Not in use<br />
|I1<br />
| -<br />
|-<br />
!scope="row" align="left"| ODEF<br />
| Not in use<br />
|E15.4<br />
| -<br />
|-<br />
!scope="row" align="left"| ODEFERR<br />
| Not in use<br />
|E15.4<br />
| -<br />
|-<br />
!scope="row" align="left"| ANISOTROPY<br />
| Not in use<br />
|E15.4<br />
| -<br />
|-<br />
!scope="row" align="left"| TEMPERATURE<br />
| 2 element vector containing temperature of the two detector heads at each EPOCH<br />
|E15.4<br />
| <math>^\circ</math>C<br />
|}<br />
<br />
<br />
{| border="1" cellspacing="0" cellpadding="2" align="center"<br />
|+ '''CDFFITS2'''<br />
|-<br />
!scope="col"| Column Name<br />
!scope="col"| Contents<br />
!scope="col"| Format<br />
!scope="col"| Unit<br />
|-<br />
!scope="row"| EPOCH<br />
| this is a keyword<br />
| NA<br />
| UTC<br />
|}<br />
<br />
<br />
{| border="1" cellspacing="0" cellpadding="2" align="center"<br />
|+ '''CDFFITS3'''<br />
|-<br />
!scope="col"| Column Name<br />
!scope="col"| Contents<br />
!scope="col"| Format<br />
!scope="col"| Unit<br />
|-<br />
!scope="row"| RADEPOCH<br />
| this is a keyword<br />
|A24<br />
| NA<br />
|-<br />
!scope="row"| RADFET<br />
| Value proportional to the absorbed dose on a diode mounted on the surface of SREM<br />
|E15.4<br />
| NA<br />
|}<br />
<br />
'''Note:''' SREM calibrated data files where initially provided in the [http://cdf.gsfc.nasa.gov/ Common Data Format (cdf) format]. This has traditionally been the preferred data format for SREM on board previous ESA missions. However, as cdf is not widely used in the astrophysics community it was later agreed with the provider that fits files should also be provided. This meant taking the original cdf format and converting it to fits. The original cdf files can be retrieved from the [http://srem.web.psi.ch/html/srem_home.shtml SREM site] at the PSI.<br />
<br />
[[Category:Operational data|007]]<br />
[[Category:PSOBook]]</div>
Xdupac
https://wiki.cosmos.esa.int/planckpla2015/index.php?title=SREM&diff=11005
SREM
2015-02-03T16:01:24Z
<p>Xdupac: /* Related products */</p>
<hr />
<div>==Product description==<br />
The SREM data files contain calibrated data for the different energy and particle species channels available in the SREM. Each data file contains 24 hours of data - from midnight to midnight UTC. (note this is '''not''' an Operational Day) - with the date covered by the file easily identifiable through the file name.<br />
<br />
==Inputs==<br />
SREM calibrated data was produced from the SREM raw data acquired during the entire mission.<br />
<br />
==Related products==<br />
Data for the SREM on board other ESA missions can be retrieved from the Paul Scherrer Institute [http://www.psi.ch]. In order to retrieve the data you will need to register first.<br />
<br />
==Data files==<br />
The files containing the SREM calibrated data will have a name of the form SREMPlanck_PACC_YYYYMMDD.fits where PACC stands for Processed ACCumulated data and YYYYMMDD is the date the data in the file was acquired.<br />
<br />
The SREM processed data can be downloaded from the PLA interface: "Ancillary data" tab of the "Time-ordered information" section.<br />
<br />
A list of the files available can be found {{PLAProductsV2|product=opdata|link=here}}.<br />
<br />
===Data format===<br />
Each file contains three binary table extensions named CDFFITS1,CDFFITS2 and CDFFITS3. The first extension contains the accumulated counts data, the second extension the labels to identify the data in the first extension and the third extension the total radiation dosis. The contents of each extension are as follows.<br />
{| border="1" cellspacing="0" cellpadding="2" align="center"<br />
|+ '''CDFFITS1'''<br />
|-<br />
!scope="col"| Column Name<br />
!scope="col"| Contents<br />
!scope="col"| Format<br />
!scope="col"| Unit<br />
|-<br />
!scope="row" align="left" width="150"| EPOCH<br />
| width="550" | vector containing 1 string with UTC for center of accumulation interval in ISO format (YYYY-MM-DDTHH:MM:SS.MMMZ)<br />
|A24<br />
| NA<br />
|-<br />
!scope="row" align="left"| COUNTRATE<br />
| vector containing 15 elements (1 for each channel) with counts for accumulation period identified in the EPOCH column <br />
|E15.4<br />
| s<math>^{-1}</math><br />
|-<br />
!scope="row" align="left"| ORBIT<br />
| position (x,y,z) of the SREM in the ECI frame. Distance from center fo the Earth is <math>R=\sqrt(x^2+y^2+z^2)</math><br />
|E15.4<br />
| km<br />
|-<br />
!scope="row" align="left"| ATTITUDE<br />
| Not in use<br />
|E15.4<br />
| -<br />
|-<br />
!scope="row" align="left"| PROT FITQUAL<br />
| Not in use<br />
|I1<br />
| NA<br />
|-<br />
!scope="row" align="left"| ODPF<br />
| Not in use.<br />
|E15.4<br />
| -<br />
|-<br />
!scope="row" align="left"| ODPFERR<br />
| Not in use<br />
|E15.4<br />
| -<br />
|-<br />
!scope="row" align="left"| ELEC FITQUAL<br />
| Not in use<br />
|I1<br />
| -<br />
|-<br />
!scope="row" align="left"| ODEF<br />
| Not in use<br />
|E15.4<br />
| -<br />
|-<br />
!scope="row" align="left"| ODEFERR<br />
| Not in use<br />
|E15.4<br />
| -<br />
|-<br />
!scope="row" align="left"| ANISOTROPY<br />
| Not in use<br />
|E15.4<br />
| -<br />
|-<br />
!scope="row" align="left"| TEMPERATURE<br />
| 2 element vector containing temperature of the two detector heads at each EPOCH<br />
|E15.4<br />
| <math>^\circ</math>C<br />
|}<br />
<br />
<br />
{| border="1" cellspacing="0" cellpadding="2" align="center"<br />
|+ '''CDFFITS2'''<br />
|-<br />
!scope="col"| Column Name<br />
!scope="col"| Contents<br />
!scope="col"| Format<br />
!scope="col"| Unit<br />
|-<br />
!scope="row"| EPOCH<br />
| this is a keyword<br />
| NA<br />
| UTC<br />
|}<br />
<br />
<br />
{| border="1" cellspacing="0" cellpadding="2" align="center"<br />
|+ '''CDFFITS3'''<br />
|-<br />
!scope="col"| Column Name<br />
!scope="col"| Contents<br />
!scope="col"| Format<br />
!scope="col"| Unit<br />
|-<br />
!scope="row"| RADEPOCH<br />
| this is a keyword<br />
|A24<br />
| NA<br />
|-<br />
!scope="row"| RADFET<br />
| Value proportional to the absorbed dose on a diode mounted on the surface of SREM<br />
|E15.4<br />
| NA<br />
|}<br />
<br />
'''Note:''' SREM calibrated data files where initially provided in the [http://cdf.gsfc.nasa.gov/ Common Data Format (cdf) format]. This has traditionally been the preferred data format for SREM on board previous ESA missions. However, as cdf is not widely used in the astrophysics community it was later agreed with the provider that fits files should also be provided. This meant taking the original cdf format and converting it to fits. The original cdf files can be retrieved from the [http://srem.web.psi.ch/html/srem_home.shtml SREM site] at the PSI.<br />
<br />
[[Category:Operational data|007]]<br />
[[Category:PSOBook]]</div>
Xdupac
https://wiki.cosmos.esa.int/planckpla2015/index.php?title=SREM&diff=11004
SREM
2015-02-03T16:00:59Z
<p>Xdupac: /* Related products */</p>
<hr />
<div>==Product description==<br />
The SREM data files contain calibrated data for the different energy and particle species channels available in the SREM. Each data file contains 24 hours of data - from midnight to midnight UTC. (note this is '''not''' an Operational Day) - with the date covered by the file easily identifiable through the file name.<br />
<br />
==Inputs==<br />
SREM calibrated data was produced from the SREM raw data acquired during the entire mission.<br />
<br />
==Related products==<br />
Data for the SREM on board other ESA missions can be retrieved from the Paul Scherrer Institute [http://www.psi.ch]. In order to retrieve the data you will need to Register first.<br />
<br />
==Data files==<br />
The files containing the SREM calibrated data will have a name of the form SREMPlanck_PACC_YYYYMMDD.fits where PACC stands for Processed ACCumulated data and YYYYMMDD is the date the data in the file was acquired.<br />
<br />
The SREM processed data can be downloaded from the PLA interface: "Ancillary data" tab of the "Time-ordered information" section.<br />
<br />
A list of the files available can be found {{PLAProductsV2|product=opdata|link=here}}.<br />
<br />
===Data format===<br />
Each file contains three binary table extensions named CDFFITS1,CDFFITS2 and CDFFITS3. The first extension contains the accumulated counts data, the second extension the labels to identify the data in the first extension and the third extension the total radiation dosis. The contents of each extension are as follows.<br />
{| border="1" cellspacing="0" cellpadding="2" align="center"<br />
|+ '''CDFFITS1'''<br />
|-<br />
!scope="col"| Column Name<br />
!scope="col"| Contents<br />
!scope="col"| Format<br />
!scope="col"| Unit<br />
|-<br />
!scope="row" align="left" width="150"| EPOCH<br />
| width="550" | vector containing 1 string with UTC for center of accumulation interval in ISO format (YYYY-MM-DDTHH:MM:SS.MMMZ)<br />
|A24<br />
| NA<br />
|-<br />
!scope="row" align="left"| COUNTRATE<br />
| vector containing 15 elements (1 for each channel) with counts for accumulation period identified in the EPOCH column <br />
|E15.4<br />
| s<math>^{-1}</math><br />
|-<br />
!scope="row" align="left"| ORBIT<br />
| position (x,y,z) of the SREM in the ECI frame. Distance from center fo the Earth is <math>R=\sqrt(x^2+y^2+z^2)</math><br />
|E15.4<br />
| km<br />
|-<br />
!scope="row" align="left"| ATTITUDE<br />
| Not in use<br />
|E15.4<br />
| -<br />
|-<br />
!scope="row" align="left"| PROT FITQUAL<br />
| Not in use<br />
|I1<br />
| NA<br />
|-<br />
!scope="row" align="left"| ODPF<br />
| Not in use.<br />
|E15.4<br />
| -<br />
|-<br />
!scope="row" align="left"| ODPFERR<br />
| Not in use<br />
|E15.4<br />
| -<br />
|-<br />
!scope="row" align="left"| ELEC FITQUAL<br />
| Not in use<br />
|I1<br />
| -<br />
|-<br />
!scope="row" align="left"| ODEF<br />
| Not in use<br />
|E15.4<br />
| -<br />
|-<br />
!scope="row" align="left"| ODEFERR<br />
| Not in use<br />
|E15.4<br />
| -<br />
|-<br />
!scope="row" align="left"| ANISOTROPY<br />
| Not in use<br />
|E15.4<br />
| -<br />
|-<br />
!scope="row" align="left"| TEMPERATURE<br />
| 2 element vector containing temperature of the two detector heads at each EPOCH<br />
|E15.4<br />
| <math>^\circ</math>C<br />
|}<br />
<br />
<br />
{| border="1" cellspacing="0" cellpadding="2" align="center"<br />
|+ '''CDFFITS2'''<br />
|-<br />
!scope="col"| Column Name<br />
!scope="col"| Contents<br />
!scope="col"| Format<br />
!scope="col"| Unit<br />
|-<br />
!scope="row"| EPOCH<br />
| this is a keyword<br />
| NA<br />
| UTC<br />
|}<br />
<br />
<br />
{| border="1" cellspacing="0" cellpadding="2" align="center"<br />
|+ '''CDFFITS3'''<br />
|-<br />
!scope="col"| Column Name<br />
!scope="col"| Contents<br />
!scope="col"| Format<br />
!scope="col"| Unit<br />
|-<br />
!scope="row"| RADEPOCH<br />
| this is a keyword<br />
|A24<br />
| NA<br />
|-<br />
!scope="row"| RADFET<br />
| Value proportional to the absorbed dose on a diode mounted on the surface of SREM<br />
|E15.4<br />
| NA<br />
|}<br />
<br />
'''Note:''' SREM calibrated data files where initially provided in the [http://cdf.gsfc.nasa.gov/ Common Data Format (cdf) format]. This has traditionally been the preferred data format for SREM on board previous ESA missions. However, as cdf is not widely used in the astrophysics community it was later agreed with the provider that fits files should also be provided. This meant taking the original cdf format and converting it to fits. The original cdf files can be retrieved from the [http://srem.web.psi.ch/html/srem_home.shtml SREM site] at the PSI.<br />
<br />
[[Category:Operational data|007]]<br />
[[Category:PSOBook]]</div>
Xdupac
https://wiki.cosmos.esa.int/planckpla2015/index.php?title=SREM&diff=11003
SREM
2015-02-03T16:00:30Z
<p>Xdupac: /* Related products */</p>
<hr />
<div>==Product description==<br />
The SREM data files contain calibrated data for the different energy and particle species channels available in the SREM. Each data file contains 24 hours of data - from midnight to midnight UTC. (note this is '''not''' an Operational Day) - with the date covered by the file easily identifiable through the file name.<br />
<br />
==Inputs==<br />
SREM calibrated data was produced from the SREM raw data acquired during the entire mission.<br />
<br />
==Related products==<br />
Data for the SREM on board other ESA missions can be retrieved from the Paul Scherrer Institute [http://www.psi.ch]. In order to retrieve the data you will need to Register first. The registration link is immediately below the data access link.<br />
<br />
==Data files==<br />
The files containing the SREM calibrated data will have a name of the form SREMPlanck_PACC_YYYYMMDD.fits where PACC stands for Processed ACCumulated data and YYYYMMDD is the date the data in the file was acquired.<br />
<br />
The SREM processed data can be downloaded from the PLA interface: "Ancillary data" tab of the "Time-ordered information" section.<br />
<br />
A list of the files available can be found {{PLAProductsV2|product=opdata|link=here}}.<br />
<br />
===Data format===<br />
Each file contains three binary table extensions named CDFFITS1,CDFFITS2 and CDFFITS3. The first extension contains the accumulated counts data, the second extension the labels to identify the data in the first extension and the third extension the total radiation dosis. The contents of each extension are as follows.<br />
{| border="1" cellspacing="0" cellpadding="2" align="center"<br />
|+ '''CDFFITS1'''<br />
|-<br />
!scope="col"| Column Name<br />
!scope="col"| Contents<br />
!scope="col"| Format<br />
!scope="col"| Unit<br />
|-<br />
!scope="row" align="left" width="150"| EPOCH<br />
| width="550" | vector containing 1 string with UTC for center of accumulation interval in ISO format (YYYY-MM-DDTHH:MM:SS.MMMZ)<br />
|A24<br />
| NA<br />
|-<br />
!scope="row" align="left"| COUNTRATE<br />
| vector containing 15 elements (1 for each channel) with counts for accumulation period identified in the EPOCH column <br />
|E15.4<br />
| s<math>^{-1}</math><br />
|-<br />
!scope="row" align="left"| ORBIT<br />
| position (x,y,z) of the SREM in the ECI frame. Distance from center fo the Earth is <math>R=\sqrt(x^2+y^2+z^2)</math><br />
|E15.4<br />
| km<br />
|-<br />
!scope="row" align="left"| ATTITUDE<br />
| Not in use<br />
|E15.4<br />
| -<br />
|-<br />
!scope="row" align="left"| PROT FITQUAL<br />
| Not in use<br />
|I1<br />
| NA<br />
|-<br />
!scope="row" align="left"| ODPF<br />
| Not in use.<br />
|E15.4<br />
| -<br />
|-<br />
!scope="row" align="left"| ODPFERR<br />
| Not in use<br />
|E15.4<br />
| -<br />
|-<br />
!scope="row" align="left"| ELEC FITQUAL<br />
| Not in use<br />
|I1<br />
| -<br />
|-<br />
!scope="row" align="left"| ODEF<br />
| Not in use<br />
|E15.4<br />
| -<br />
|-<br />
!scope="row" align="left"| ODEFERR<br />
| Not in use<br />
|E15.4<br />
| -<br />
|-<br />
!scope="row" align="left"| ANISOTROPY<br />
| Not in use<br />
|E15.4<br />
| -<br />
|-<br />
!scope="row" align="left"| TEMPERATURE<br />
| 2 element vector containing temperature of the two detector heads at each EPOCH<br />
|E15.4<br />
| <math>^\circ</math>C<br />
|}<br />
<br />
<br />
{| border="1" cellspacing="0" cellpadding="2" align="center"<br />
|+ '''CDFFITS2'''<br />
|-<br />
!scope="col"| Column Name<br />
!scope="col"| Contents<br />
!scope="col"| Format<br />
!scope="col"| Unit<br />
|-<br />
!scope="row"| EPOCH<br />
| this is a keyword<br />
| NA<br />
| UTC<br />
|}<br />
<br />
<br />
{| border="1" cellspacing="0" cellpadding="2" align="center"<br />
|+ '''CDFFITS3'''<br />
|-<br />
!scope="col"| Column Name<br />
!scope="col"| Contents<br />
!scope="col"| Format<br />
!scope="col"| Unit<br />
|-<br />
!scope="row"| RADEPOCH<br />
| this is a keyword<br />
|A24<br />
| NA<br />
|-<br />
!scope="row"| RADFET<br />
| Value proportional to the absorbed dose on a diode mounted on the surface of SREM<br />
|E15.4<br />
| NA<br />
|}<br />
<br />
'''Note:''' SREM calibrated data files where initially provided in the [http://cdf.gsfc.nasa.gov/ Common Data Format (cdf) format]. This has traditionally been the preferred data format for SREM on board previous ESA missions. However, as cdf is not widely used in the astrophysics community it was later agreed with the provider that fits files should also be provided. This meant taking the original cdf format and converting it to fits. The original cdf files can be retrieved from the [http://srem.web.psi.ch/html/srem_home.shtml SREM site] at the PSI.<br />
<br />
[[Category:Operational data|007]]<br />
[[Category:PSOBook]]</div>
Xdupac