Search results

Jump to: navigation, search

Create the page "Pointing LFI" on this wiki! See also the search results found.

  • Main Page
    ##[[LFI overview|LFI design, qualification, and performance]]<span style="color:red"></span> ###[[LFI design, qualification, and performance#LFIDescription| Instrument descripti
    6 KB (669 words) - 21:21, 6 August 2018
  • LFI design, qualification, and performance
    The Low-Frequency Instrument (see Fig. 1 in the [[LFI overview]]) consists of a 20 K focal plane unit hosting the corrugated feed Best LFI noise performance is obtained with receivers based on InP High Electron Mob
    50 KB (7,826 words) - 22:29, 4 February 2015
  • Operational history
    *the LFI; *pointing performance.
    11 KB (1,616 words) - 12:31, 26 March 2014
  • Survey scanning and performance
    ...e 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 ot ...ane. 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 (precessi
    17 KB (2,543 words) - 16:31, 3 February 2015
  • The HFI DPC
    * timing and pointing interpolation. * pointing and beam construction of each detector (see sections [[Detector pointing]] and [[Beams]]);
    4 KB (627 words) - 13:09, 7 July 2015
  • The LFI DPC
    ...telemetry handling|Housekeeping telemetry handling]] • [[Pre-processing LFI#Auxiliary data handling|Auxiliary data handling]]'' ...Calibration]] • [[TOI_processing LFI#Noise|Noise]] • [[TOI_processing LFI#References|References]] ''
    8 KB (1,072 words) - 20:27, 4 February 2015
  • Simulation data
    ...al (detector beam, bandpass, and correlated noise properties), scanning (pointing and flags), and analysis (map-making algorithm and implementation) eff ...n {{PlanckPapers|planck2014-a03}} and {{PlanckPapers|planck2014-a08}} for LFI and HFI, respectively.
    46 KB (7,032 words) - 12:02, 29 March 2016
  • Product Table for PLAv2
    |rowspan="3" align="center" | LFI | rowspan="6" align="center"| LFI
    83 KB (8,209 words) - 12:21, 5 February 2015
  • Glossary
    ...rs to the component of the calibration that varies from pointing period to pointing period. * '''DMC''': Data Management Component, the databases used at the HFI and LFI DPCs.
    7 KB (1,093 words) - 13:07, 7 July 2015
  • Planck Collaboration
    *The LFI Consortium, Principal Investigator N. Mandolesi of the Istituto di Astrofis ...tested and delivered to ESA by dedicated teams under the direction of the LFI and HFI Principal Investigators and Project Managers.
    9 KB (1,372 words) - 08:30, 21 September 2012
  • Timelines
    ...the value of that quantity as a function of time during the mission. For LFI, refer to {{PlanckPapers|planck2014-a03}}, and for HFI, to {{PlanckPapers|p ...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
    28 KB (4,415 words) - 18:43, 21 August 2015
  • Sky temperature maps
    ...ps are in Healpix format, with Nside of 1024 (LFI 30, 44 and 70) and 2048 (LFI 70 and HFI), in Galactic coordinates, and Nested ordering. ! Range || ODs || HFI rings || pointing-IDs || Comment
    45 KB (6,681 words) - 11:55, 16 May 2017
  • The RIMO
    ...th the released data products. It is described in detail in ''The HFI and LFI RIMO ICD'' (ref). See also {{PlanckPapers|planck2014-a03}} and {{PlanckPap ; LFI 2015 RIMO: {{PLASingleFile|fileType=rimo|name=LFI_RIMO_R2.50.fits|link=LFI_
    14 KB (2,168 words) - 09:15, 8 March 2017
  • The Planck mission
    LFI and HFI. It started with the FLS on 13 August of 2009, at of LFI science data and 72 kbps of HFI science data. The data
    13 KB (2,044 words) - 09:08, 21 August 2013
  • The satellite
    ...ssing radiation from the sky onto a focal plane shared by detectors of the LFI and HFI, operating at 20K and 0.1K respectively; a telescope baffle that si |Planck operated for 32 months with both instruments; the LFI continues surveying the sky
    14 KB (2,170 words) - 09:29, 21 May 2014
  • Ground Segment and Operations
    * providing MOC with a detailed pointing plan with a periodicity of about one month; === The LFI instrument operations and data-processing centre ===
    4 KB (599 words) - 09:38, 3 February 2015
  • TOI processing LFI
    ...l2 Pipeline analyzes data from each horn of the instrument separately, one pointing period at time, and stores the results in an object the length of an OD. Ea ...g maneuver, start OBT of the stable pointing, OBT of the end of the stable pointing, and spin axis ecliptic longitude and latitude.
    34 KB (5,468 words) - 15:34, 4 February 2015
  • Pre-processing LFI
    The first processing level of the LFI DPC is the so called Level 1. The source data of the Level 1 software inclu ...eping telemetry packets retrieved from different satellite subsystems: the LFI instrument, the Sorption cooler, the HFI instrument and the Central Data Ma
    14 KB (2,299 words) - 20:58, 17 March 2013
  • Map-making LFI
    ...rocedure consist of the calibrated timelines, along with the corresponding pointing information. LFI maps were constructed with the MADAM mapmaking code, version 3.7.4.
    26 KB (3,949 words) - 15:33, 1 March 2017
  • Beams LFI
    LFI observed the sky with 11 pairs of beams associated with the 22 pseudo-corre ...} (see also [[LFI design, qualification, and performance#Naming Convention|LFI naming convention]]).
    24 KB (3,748 words) - 10:02, 26 September 2016
  • LFI-Validation
    ...validation is critical at each step of the analysis pipeline. Much of the LFI data validation is based on null tests. Here we present some examples from Three things are worth pointing out generally about these maps.
    10 KB (1,699 words) - 13:37, 19 September 2016
  • HL-sims
    ...[[ref to the old LS paper]]. It can take in input the output of the PSM, a pointing and beam description in order to generate the infalling power on detectors ...or, no 4K nor glitch residuals, no noise correlation, etc). But the actual pointing, spectral banpasses, beams, noise determinations were used.
    5 KB (779 words) - 16:03, 21 May 2014
  • Mission products
    * '''signal and pointing timelines''', accompanied by the relevant flags, which can be used to build ...ng are given in the [[The HFI DPC| HFI Data Processing]] and [[The LFI DPC|LFI Data Processing]] chapters. Each section also lists any known problems wit
    3 KB (438 words) - 10:45, 5 February 2015
  • Main Page2
    ##[[LFI design, qualification, and performance|LFI design, qualification, and performance]]<span style="color:red">(Gregorio)< ##[[Pointing performance|Pointing performance]] <span style="color:red">(Dupac)</span>
    2 KB (265 words) - 17:39, 25 January 2013
  • Effective Beams
    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 ...essing are given in the respective pages for [[Beams|HFI]] and [[Beams_LFI|LFI]].
    22 KB (3,180 words) - 10:37, 5 February 2015
  • Main Page3
    ##[[LFI design, qualification, and performance|LFI design, qualification, and performance]]<span style="color:red">(Gregorio)< ##[[Pointing performance|Pointing performance]] <span style="color:red">(Dupac)</span>
    6 KB (770 words) - 17:33, 29 January 2013
  • List of acronyms
    * '''APPL''' : Augmented Preprogrammed Pointing List * '''ASW''' : (LFI REBA) Application SoftWare
    6 KB (650 words) - 23:43, 1 February 2015
  • LFI systematic effect uncertainties
    Known systematic effects in the Planck-LFI data can be divided into two broad categories: effects independent of the s ...evel overview of the uncertainties due to systematic effects in the Planck-LFI CMB temperature maps and power spectra. Table 1 provides a list of these ef
    20 KB (2,907 words) - 13:28, 19 September 2016
  • Beams
    ...asonal brightness. This is achieved by determining a scaling factor and a pointing offset by fitting the time-ordered data to a template from a previous estim ...>\Delta\Omega _\mathrm{MC}</math>) including noise, residual glitches, and pointing uncertainty.'''</small>
    52 KB (8,515 words) - 12:52, 7 July 2015
  • Changelog
    * 2013-04-12, Zacchei, [[Frequency Maps | Sky temperature maps]] : Added LFI 70 GHz 2048 product and caveats on the use of effective beam with those map * 2013-04-12, Zacchei, [[Map-making_LFI | Map-making]] : Added LFI 70 GHz 2048 product. <span style="color:Green">Moved to public ES.</span>
    12 KB (1,788 words) - 08:42, 25 September 2014
  • Detector pointing
    ...e full advantage of the Planck beams, we must know the individual detector pointing positions to a precision of better than several arcseconds, over the course ...te for convenience. We must then further rotate this focal-plane boresight pointing to the individual detector locations. Because neither the rotations from th
    5 KB (744 words) - 13:20, 12 January 2018
  • TOC WorkInProgress
    ##[[LFI overview|LFI design, qualification, and performance]]<span style="color:red"></span> ###[[LFI design, qualification, and performance#LFIDescription| Instrument descripti
    5 KB (581 words) - 09:33, 31 March 2014
  • The Planck mission WiP
    about five times for the HFI and eight times for the LFI. LFI and HFI. It started with the FLS on 13 August 2009.
    16 KB (2,511 words) - 18:59, 14 October 2014
  • The satellite WiP
    ...ssing radiation from the sky onto a focal plane shared by detectors of the LFI and HFI, operating at 20K and 0.1K, respectively; a telescope baffle that s |Planck operated for 32 months with both instruments; the LFI continued surveying the sky for an additional 20 months
    14 KB (2,136 words) - 09:37, 3 February 2015
  • TOCV1 BackUp
    ##[[LFI overview|LFI design, qualification, and performance]]<span style="color:red"></span> ###[[LFI design, qualification, and performance#LFIDescription| Instrument descripti
    6 KB (744 words) - 09:45, 31 March 2014
  • TestMassEditing
    ...built using the first and second half of the stable pointing part in each pointing period. These maps are used extensively to investigate the (high frequency) ...lpix format, with Nside of 2048 for HFI and of 1024 for LFI (note that the LFI 70 GHz has been delivered also at Nside of 2048 to be directly comparable w
    35 KB (5,146 words) - 17:59, 3 July 2014
  • Terminology
    ...refers to the component of the calibration that varies pointing period by pointing period. ...difference : difference between the map built using the first half of each pointing period (typically 20 minutes of contiguous data) and the one built with th
    10 KB (1,539 words) - 15:11, 21 July 2014
  • NoiseCovarMatrices
    The noise PSDs feed into two noise covariance estimation codes. The LFI noise covariance is estimated using a module integrated in the Madam mapmak ...N</math> depend on the mapmaking method and the features of the noise PSD. LFI uses short baselines and a noise prior to reduce correlated noise up to rou
    6 KB (1,020 words) - 18:38, 19 December 2014
  • Planck Added Value Tools
    ...corresponding uncertainty values; only the HFI bandpasses has this, so for LFI bandpasses this functionality is disabled. The uncertainty is estimated by ...measurement. This is the algorithm that was used in the generation of the LFI masks. The exact equation that is used is
    30 KB (5,022 words) - 16:55, 16 March 2018
Retrieved from ‘https://wiki.cosmos.esa.int/planckpla2015/index.php/Special:Search’