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• Main Page3
  ##[[HFI design, qualification, and performance|HFI design, qualification, and performance]] <span style="color:red">(Lamarre/Pajot)</span> ##[[LFI design, qualification, and performance|LFI design, qualification, and performance]]<span style="color:red">(Gregorio)</span>
  6 KB (770 words) - 17:33, 29 January 2013
• List of acronyms
  * '''CPV''' : Calibration and Performance Verification * '''HFI''' : (Planck) High Frequency Instrument
  7 KB (738 words) - 22:33, 1 July 2018
• HFI operations timeline
  * '''HFI''', refers to HFI instrument operations (when this is during the commissioning of the CPV phases, labels [[Category:HFI design, qualification and performance|014]]
  27 KB (2,766 words) - 19:41, 11 December 2014
• References2
  ...ests of high sensitivity NTD Ge thermometers for the Planck-High Frequency Instrument}, title = {Thermal architecture design tests for the Planck/HFI instrument},
  39 KB (5,438 words) - 09:40, 20 May 2014
• LFIAppendix
  === Annexes: LFI Instrument === ...fly described in the main [[LFI design, qualification, and performance|LFI instrument]] page.
  60 KB (9,314 words) - 08:48, 2 January 2015
• LFI overview
  {{DISPLAYTITLE:LFI design, qualification and performance}} This section provides an overview of the Low-Frequency Instrument and of its different sub-systems.
  4 KB (551 words) - 12:13, 12 July 2018
• HFI instrument annexes
  This is a list of all annexes for the HFI instrument section. [[Category:HFI design, qualification and performance|006]]
  812 bytes (97 words) - 06:52, 10 December 2014
• TOC WorkInProgress
  ##[[HFI design, qualification, and performance|HFI design, qualification, and performance]] ###[[HFI_performance_summary | Performance summary]]
  5 KB (581 words) - 09:33, 31 March 2014
• The Planck mission WiP
  ...MB, with an accuracy set by fundamental astrophysical limits. Its level of performance enabled Planck to extract essentially all the information in the CMB temper Instrument (LFI), and a SAMBA-like High Frequency Instrument (HFI),
  15 KB (2,330 words) - 12:43, 17 July 2018
• The satellite WiP
  |Instrument part: 685 W (Begining of Life); 780 W (End of Life) ...f detector feedhorns, designed, manufactured and tested by the LFI and HFI instrument teams ({{PlanckPapers|villa2010}}, {{PlanckPapers|sandri2010}}, {{PlanckPap
  30 KB (4,647 words) - 09:23, 10 July 2018
• TOCV1 BackUp
  ##[[HFI design, qualification, and performance|HFI design, qualification, and performance]] ###[[HFI_performance_summary | Performance summary]]
  6 KB (744 words) - 09:45, 31 March 2014
• TestReplace2
  thermometer. The instrument Flight Model total number of bolometers is 52, split into 6 ...minimised to limit the photon noise contribution on the detectors from the instrument.
  13 KB (2,128 words) - 15:29, 4 June 2014
• Terminology
  ...icable to the data processing. IMO does not represent the knowledge of the instrument. It is a knowledge of its response, (e.g. how photons are gathered and tran ...: The RIMO, or Reduced Instrument Model is a FITS file containing selected instrument characteristics that are needed by users who work with the released data pr
  10 KB (1,542 words) - 09:41, 2 February 2018
• Frequency maps
  ...es and noise weights as they are recorded in the accompanying [[NPIPE RIMO|instrument model]]. Inverse variance noise weights in each horn are symmetrized: ...ctors, as the positions depend on their location in the focal plane of the instrument. As a result, when data from different detectors are combined to build a f
  133 KB (19,918 words) - 11:57, 14 December 2022

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