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- ##[[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
- * '''CPV''' : Calibration and Performance Verification * '''HFI''' : (Planck) High Frequency Instrument7 KB (738 words) - 22:33, 1 July 2018
- * '''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
- ...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
- === 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
- {{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
- 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
- ##[[HFI design, qualification, and performance|HFI design, qualification, and performance]] ###[[HFI_performance_summary | Performance summary]]5 KB (581 words) - 09:33, 31 March 2014
- ...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
- |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}}, {{PlanckPap30 KB (4,647 words) - 09:23, 10 July 2018
- ##[[HFI design, qualification, and performance|HFI design, qualification, and performance]] ###[[HFI_performance_summary | Performance summary]]6 KB (744 words) - 09:45, 31 March 2014
- 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
- ...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 pr10 KB (1,542 words) - 09:41, 2 February 2018
- ...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 f133 KB (19,918 words) - 11:57, 14 December 2022