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  • HFI design, qualification, and performance
    ...detail this information are available: {{PlanckPapers|lamarre2010}} and {{PlanckPapers|planck2011-1-5}}. Additional detailed information potentially useful for th
    5 KB (778 words) - 15:28, 22 July 2014
  • LFI design, qualification, and performance
    ...can be written as follows{{BibCite|seiffert2002}}{{BibCite|mennella2003}}{{PlanckPapers|bersanelli2010}}:: The gain modulation factor{{BibCite|mennella2003}}{{PlanckPapers|planck2011-1-6}}, <math>r</math>, is defined by:
    50 KB (7,790 words) - 10:04, 23 July 2014
  • The HFI DPC
    ...es of publications was described in {{PlanckPapers|planck2011-1-7}}. The {{PlanckPapers|planck2013-p03}} and its co-papers provide the reference for the processin ...other R&D groups in the HFI and LFI core teams. An overview was given in {{PlanckPapers|planck2011-1-7}}. In particular:
    4 KB (619 words) - 13:50, 23 July 2014
  • The LFI DPC
    ...nckPapers|planck2013-p02b}}, and instrument performances are reported in {{PlanckPapers|planck2013-p02a}}.
    7 KB (1,004 words) - 15:06, 23 July 2014
  • Simulation data
    ...t decorrelation observed in the Planck Early Paper on CIB power spectrum {{PlanckPapers|planck2011-6-6}}. ...haracterisation of this lensing potential map are described in detail in {{PlanckPapers|planck2013-p12}}, which describes also the procedure used to generate the r
    28 KB (4,118 words) - 16:15, 15 October 2015
  • Specially processed maps
    ...e (MV) lens reconstruction which forms the basis for the main results of {{PlanckPapers|planck2013-p12}}. This map is produced using a combination of the 143 and 2 ...spectrum on the local noise level of the map, discussed in Appendix A of {{PlanckPapers|planck2013-p12}}. Note that the noise power spectrum estimate here is not s
    7 KB (921 words) - 17:34, 23 July 2014
  • Catalogues
    # The Planck beams are described in {{PlanckPapers|planck2013-p02d}} and {{PlanckPapers|planck2013-p03c}}. This table shows the values which were adopted for the P # In the extragalactic zone (48% of the sky; see Fig. 2 in {{PlanckPapers|planck2013-p05}}).
    30 KB (4,218 words) - 16:56, 23 July 2014
  • CMB spectrum & Likelihood Code
    .../math>, instead, the spectrum is derived from the ''CAMspec'' likelihood {{PlanckPapers|planck2013-p08}} by optimally combining the spectra in the frequency range ...nck best-fit primordial power spectrum (cf Planck+WP+highL in Table 5 of {{PlanckPapers|planck2013-p11}}).''']]
    17 KB (2,601 words) - 17:28, 23 July 2014
  • Pre-processing
    ...ience data is retrieved and reconstructed as described in section 3.1 of {{PlanckPapers|planck2011-1-7|5}}. ...using a spherical linear interpolation as described in section 3.4 of of {{PlanckPapers|planck2011-1-7|6}}.
    13 KB (1,976 words) - 13:53, 23 July 2014
  • Sky temperature maps
    ...sting them to astrophysical values is given in the HFI Calibration paper {{PlanckPapers|planck2013-p03b}}. ...vel monopole by applying an offset correction, see LFI Calibration paper {{PlanckPapers|planck2013-p02b}} section 3.4 "Setting the zero levels in the maps". Note t
    35 KB (5,220 words) - 13:00, 24 July 2014
  • Map-making
    ...nd its performances are described in {{PlanckPapers|planck2013-p03}} and {{PlanckPapers|planck2013-p03b}}. ...on is removed from the 353, 545 and 857 GHz channels. It is described in {{PlanckPapers|planck2013-p03}}, but a synopsis of the procedure is as follows:
    11 KB (1,710 words) - 14:31, 23 July 2014
  • The RIMO
    ...passes of the detectors that are used to build the map. For details see {{PlanckPapers|planck2013-p03d}}. The bandpasses are given as 4-column tables containing: ...ssist in CO component separation efforts {{PlanckPapers|planck2013-p03a}}{{PlanckPapers|planck2013-p03d}}.
    12 KB (1,821 words) - 16:42, 23 July 2014
  • TOI processing
    ...tures of the pipeline which are given in the HFI Data Processing article {{PlanckPapers|planck2013-p03}}. Here we give complementary explanations on some details. ...glitch rate per channel is shown in this figure. For details, see copap. {{PlanckPapers|planck2013-p03e}}.
    18 KB (2,712 words) - 13:55, 23 July 2014
  • The Planck mission
    For more information, see {{PlanckPapers|planck2011-1-1}}. For a complete list of operational events, including cont More details on the Planck mission performance can be found in {{PlanckPapers|planck2011-1-1}}.
    16 KB (2,489 words) - 13:19, 22 July 2014
  • Ground Segment and Operations
    More information about the Planck Ground Segment may be found in {{PlanckPapers|tauber2010a}}.
    4 KB (601 words) - 14:24, 22 July 2014
  • TOI processing LFI
    ...ogic/Digital Converter on board. More on {{PlanckPapers|planck2013-p02}},{{PlanckPapers|planck2013-p02a}}. ...lines. More information can be found in {{PlanckPapers|planck2013-p02}}, {{PlanckPapers|planck2013-p02a}}.
    31 KB (4,941 words) - 15:14, 23 July 2014
  • HFI cryogenics
    ...constant. The dilution cooler is described in detail in section 2.3.3 of {{PlanckPapers|planck2011-1-3|7}}. 5.4 of {{PlanckPapers|planck2011-1-3|23}}.
    5 KB (747 words) - 15:36, 22 July 2014
  • HFI-Validation
    ...tics]] and in [[#Cosmic_Rays|the section on cosmic rays]], as well as in {{PlanckPapers|planck2013-p03e|1|the 2013 HFI Cosmic Ray Removal paper}}. ...y specific frequency signatures, which is filtered. This is described in {{PlanckPapers|planck2013-p03|1|the 2013 HFI DPC Paper}}, [[#4K_lines_Residuals|the sectio
    25 KB (4,008 words) - 15:01, 23 July 2014
  • Map-making LFI
    A detailed description of the map-making procedure is given in {{PlanckPapers|planck2013-p02}}. See also section [[Frequency Maps]]. ...}. We chose to downgrade the maps using the inverse noise weighting. See {{PlanckPapers|planck2013-p02}} for discussion.
    23 KB (3,368 words) - 15:56, 23 July 2014
  • Beams LFI
    ...fit as in {{PlanckPapers|planck2011-1-6}} with modification explained in {{PlanckPapers|planck2013-p02d}}. This method is used to determine ...cs code) by appropriately tuning the Radio Frequency Flight Model (RFFM) {{PlanckPapers|tauber2010b}}. The Radio Frequency Tuned Model, called RFTM, was implemente
    23 KB (3,650 words) - 15:53, 23 July 2014
  • LFI-Validation
    All the details can be found in {{PlanckPapers|planck2013-p02}}.
    13 KB (1,992 words) - 16:09, 23 July 2014
  • HFI cold optics
    The cold optics is described in {{PlanckPapers|ade2010}}}. ...description of the HFI optical design and beam performances is given in {{PlanckPapers|maffei2010}}.
    25 KB (3,767 words) - 15:43, 22 July 2014
  • Spectral response
    ...Further details on the definition of these parameters are available in {{PlanckPapers|planck2013-p03d}}.
    18 KB (805 words) - 14:32, 23 July 2014
  • Compact Source catalogues
    ...from each of Planck's nine frequency channels. It is fully described in {{PlanckPapers|planck2013-p05}}. ...are based on aperture photometry, PSF fitting and Gaussian fitting (see {{PlanckPapers|planck2013-p05}} for a detailed description of these additional photometrie
    12 KB (1,879 words) - 16:37, 23 July 2014
  • HFI detection chain
    {{PlanckPapers|rosset2010}}. The thermometers are ...e the Q and U Stokes parameters with minimal correction for the pointing {{PlanckPapers|rosset2010}}. Residual systematics will come from the differences between t
    13 KB (2,126 words) - 15:54, 22 July 2014
  • Effective Beams
    ...is given in the appropriate LFI {{PlanckPapers|planck2013-p02d}} and HFI {{PlanckPapers|planck2013-p03c}} papers. Relevant details of the processing steps are give
    23 KB (3,381 words) - 12:28, 28 August 2014
  • Cosmological Parameters
    ...arameter tables. Definitions, conventions and reference are contained in {{PlanckPapers|planck2013-p11}}. ...n into account when comparing with BBN results reported in Sect. 6.4. of {{PlanckPapers|planck2013-p11}}, which use an updated version for the neutron lifetime (an
    10 KB (1,566 words) - 17:32, 23 July 2014
  • Summary of HFI data characteristics
    ...contains the information from the summary section of the HFI DPC paper {{PlanckPapers|planck2013-p03}} which describes the most important characteristics of the
    449 bytes (64 words) - 15:03, 23 July 2014
  • Survey scanning and performance
    ...ng strategy'', makes use of the characteristics of the Planck spacecraft {{PlanckPapers|planck2011-1-1}} and orbit in order to achieve the survey goals in terms of [[File:AHF_353_OD389.png|thumb|400px|The 353 GHz detectors {{PlanckPapers|lamarre2010}} integration time after 389 Operational Days (the unit is seco
    16 KB (2,501 words) - 14:28, 22 July 2014
  • Summary LFI
    ...e 1 below. All the details can be found in the LFI data processing paper {{PlanckPapers|planck2013-p02}}. ...ective beam. Those are the values used in the source extraction pipeline {{PlanckPapers|planck2013-p05}}.
    2 KB (296 words) - 16:20, 23 July 2014
  • LFI systematic effect uncertainties
    ...report a brief summary of these effects, all the details can be found in{{PlanckPapers|planck2013-p02a}}. ...aps. The CMB curve corresponds to the Planck best-fit model presented in {{PlanckPapers|planck2013-p08}}.'''
    16 KB (2,578 words) - 16:05, 23 July 2014
  • L3 LFI
    ...sked Galactic plane and point sources using masks described in Sec. 3 of {{PlanckPapers|planck2013-p06}}. In particular, we have used the 70% Galactic mask for 44 ...ment between the observed spectra and the Planck Likelihood Code bestfit {{PlanckPapers|planck2013-p08}} when adding a simple foreground component to account for u
    2 KB (270 words) - 16:19, 23 July 2014
  • LFIAppendix
    ...nels. Details about the definition of colour corrections are provided in {{PlanckPapers|planck2011-1-6}}. As detailed in {{PlanckPapers|planck2011-1-4}}, one effect detected during the first survey was the daily
    59 KB (9,067 words) - 10:10, 23 July 2014
  • Frequency maps angular power spectra
    ...h-<math>\ell</math> likelihoods are described, discussed and compared in {{PlanckPapers|planck2013-p08}}. ...Y}(\ell)</math> of the relative error on <math>B^{XY}_{\ell}</math> (see {{PlanckPapers|planck2013-p03c|1|HFI time response and beams paper}}), defined for <math>p
    25 KB (3,721 words) - 17:10, 23 July 2014
  • Astrophysical component separation
    See the Component Separation paper {{PlanckPapers|planck2013-p06}} for details.
    12 KB (1,894 words) - 16:38, 23 July 2014
  • LFI overview
    ...ntre frequency. A detailed description of the LFI instrument is given in {{PlanckPapers|bersanelli2010}}, and references therein.
    3 KB (479 words) - 16:15, 22 July 2014
  • Unit conversion and Color correction
    ...t (i.e. 2.2.1.2, 4.4.5, and 4.6), as well as the Spectral Response Paper {{PlanckPapers|planck2013-p03d}} for details of the derivation of the detector spectra and ...dpass routine. Details of the unit conversion equations are available in {{PlanckPapers|planck2013-p03d}}.
    28 KB (4,680 words) - 10:21, 2 October 2014
  • Beams
    In {{PlanckPapers|planck2013-p03c}} we consider two models of the beam in order to better und ...cessing (see [[Frequency_Maps#HFI_processing | here]] or Section 3.11 of {{PlanckPapers|planck2013-p03}} for more info). We use JPL Horizons ephemerides to determi
    33 KB (5,387 words) - 14:27, 23 July 2014
  • CMB and astrophysical component maps
    All the details can be found in {{PlanckPapers|planck2013-p06}}. ...isotropy map. These are the maps used in the component separation paper {{PlanckPapers|planck2013-p06}}.
    55 KB (8,302 words) - 09:26, 20 June 2016
  • Detector pointing
    ...detector transfer function, which is complex in the Fourier domain (see {{PlanckPapers|planck2013-p03c}}). This phase shift was not measured during normal operati ...e radiometer electronics box assembly (REBA) as discussed more fully in {{PlanckPapers|planck2013-p03}}.
    17 KB (2,628 words) - 16:32, 23 July 2014
  • The spacecraft
    For more information, see {{PlanckPapers|planck2011-1-1}}. For more information, see {{PlanckPapers|tauber2010a}}.
    14 KB (2,142 words) - 14:23, 22 July 2014
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