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• HFI design, qualification, and performance
  This section provides an overview of the High-Frequency Instrument and of its different sub-systems. Two papers that ...L_TheElectronicsAndServiceModule.png|thumb|500px|center|HFI electronics in the satellite]]
  5 KB (758 words) - 09:41, 3 February 2015
• LFI design, qualification, and performance
  ...ng a further radio frequency amplification stage, detector diodes, and all the electronics for data acquisition and bias supply. ...ng to the HFI helium J-T cooler. Two sorption cooler units are included in the flight hardware.
  50 KB (7,826 words) - 22:29, 4 February 2015
• Operational history
  The major operational phases and milestones are: ...o follow the scanning strategy require about 2.6 ms−1 per year. Overall, the excellent performance of launch and orbit manoeuvres will lead to a large a
  11 KB (1,616 words) - 12:31, 26 March 2014
• Survey scanning and performance
  == The observation strategy == ...k spacecraft {{PlanckPapers|planck2011-1-1}} and orbit in order to achieve the survey goals in terms of sky coverage and scanning directions.
  17 KB (2,543 words) - 16:31, 3 February 2015
• Catalogues
  ...S]] and in section 2 of {{PlanckPapers|planck2014-a35}}. The validation of the catalogues is described in section 3 of {{PlanckPapers|planck2014-a35}}. ...nal catalogues; PCCS2, here the detected sources are located in regions of the sky where it is not possible to make an estimate of their reliability.
  72 KB (10,038 words) - 08:40, 24 October 2016
• Planck Collaboration
  ...le:Planck_Logos.jpg | 500px | center | thumb | '''A pictorial overview of the major participating funding agencies and scientific institutes.''']] ...after launch, i.e. in January 2013. A complete database of all members of the Planck Collaboration can be searched [http://www.rssd.esa.int/index.php?pro
  9 KB (1,372 words) - 08:30, 21 September 2012
• LoadTest2
  ...August of 2012 at 11:00 am CET. This sentence was written by Rodrigo for the ES Wiki test load on 27 of August of 2012 at ...August of 2012 at 11:00 am CET. This sentence was written by Rodrigo for the ES Wiki test load on 27 of August of 2012 at 11:00 am CET.
  42 KB (7,697 words) - 16:43, 4 October 2012
• The RIMO
  {{DISPLAYTITLE:The 2015 instrument model}} ...me overall structure, but will differ in the details. The type of data in the RIMO can be:
  14 KB (2,168 words) - 09:15, 8 March 2017
• The Planck mission
  Planck is a space telescope of the European Space Agency designed to answer key cosmological ...the Universe are correct. To achieve this ambitious objective, it observed the Cosmic Microwave Background radiation (CMB), emitted about 14
  13 KB (2,044 words) - 09:08, 21 August 2013
• The satellite
  The Planck satellite was designed, built and tested around two major modules: ...rmal and radiative insulation between the warm service module and the cold telescope and instruments.
  14 KB (2,170 words) - 09:29, 21 May 2014
• Beams LFI
  LFI observed the sky with 11 pairs of beams associated with the 22 pseudo-correlation radiometers. ...28; M and S are the two polarizations, namely the main-arm and side-arm of the Orthomode transducers {{BibCite|darcangelo2009b}} (see also [[LFI design, q
  24 KB (3,748 words) - 10:02, 26 September 2016
• References
  title = {Planck 2013 results: The Low Frequency Instrument data processing (p02)}, title = {Planck 2013 results: Consistency of the data (p01a)},
  173 KB (25,381 words) - 15:29, 4 June 2014
• HFI cold optics
  The cold optics are described in {{PlanckPapers|ade2010}}. ..._JML_ColdOptics.png|thumb|500px|center|Mechanical and thermal structure of the HFI focal plane unit.]]
  25 KB (3,795 words) - 22:54, 12 November 2014
• Compact Source catalogues
  ...requency lists of sources, both Galactic and extragalactic, extracted from the Planck maps. ...The second public version of the catalogue (PCCS2) has been produced using the full mission data obtained between August 13 2009 and August 3 2013, as des
  25 KB (3,934 words) - 15:07, 26 September 2016
• HFI detection chain
  ...of the HFI - the detectors - are bolometers, solid-state devices in which the incoming radiation dissipates its energy as heat that increases the temperature of a
  14 KB (2,155 words) - 23:49, 12 November 2014
• Main Page3
  #[[The Planck mission|The Planck mission]] <span style="color:red">(Dupac)</span> #[[The satellite|The satellite]]
  6 KB (770 words) - 17:33, 29 January 2013
• LFI systematic effect uncertainties
  ...are dependent on the sky and that cannot be considered independently from the observation strategy. Here we report a brief summary of these effects, all the details can be found in {{PlanckPapers|planck2013-p02a}} and {{PlanckPapers
  20 KB (2,907 words) - 13:28, 19 September 2016
• References2
  adsnote = {Provided by the SAO/NASA Astrophysics Data System} title = {Simulation of the Planck-HFI thermal control system},
  39 KB (5,438 words) - 09:40, 20 May 2014
• LFIAppendix
  ...h component of the LFI instrument, which were already briefly described in the main [[LFI design, qualification, and performance|LFI instrument]] page. ...mposed of a sine-squared profiled section, and an exponential profile near the aperture plane.
  60 KB (9,314 words) - 08:48, 2 January 2015
• Frequency maps angular power spectra
  ...(detset) maps at 100, 143 and 217 GHz, all analyzed on the same 42.8% of the sky, are provided. ...large scale to small scale (see input section). Except for the removal of the most contaminated pixels through masking, no attempt at astrophysical compo
  25 KB (3,718 words) - 15:37, 18 July 2014

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