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- ...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 des25 KB (3,934 words) - 15:07, 26 September 2016
- ...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 a14 KB (2,155 words) - 23:49, 12 November 2014
- #[[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
- ...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 {{PlanckPapers20 KB (2,907 words) - 13:28, 19 September 2016
- 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
- ...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
- ...(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 compo25 KB (3,718 words) - 15:37, 18 July 2014
- ...in very stable conditions during the whole mission, and practically all of the data were correctly recorded. ...an the required sensitivity. These numbers improved by about √2 when the whole mission data become available.2 KB (303 words) - 06:48, 10 December 2014
- ...channels using their nominal centre frequencies. A detailed description of the LFI instrument is given in {{PlanckPapers|bersanelli2010}}, and references ...nimize power dissipation in the focal plane unit, which is cooled to 20 K, the radiometers are split into two subassemblies connected by a set of waveguid3 KB (487 words) - 17:09, 4 February 2015
- = The 2015 Data Release = ...tions of Uranus and Neptune are used to obtain an absolute calibration for the 545 and 857 GHz channels.52 KB (8,515 words) - 12:52, 7 July 2015
- ;The Planck mission :[[The Planck mission]]2 KB (263 words) - 17:36, 25 March 2013
- ==The service module== On the list containing the different elements of the service module, in the case of components that have their own pages, it would be nice to have link1 KB (203 words) - 18:52, 27 November 2013
- ##[[The Planck mission_WiP|The Planck mission]] ##[[The satellite_WiP|The satellite]]5 KB (581 words) - 09:33, 31 March 2014
- {{DISPLAYTITLE:The Planck mission}} Planck is a space telescope of the European Space Agency designed to answer key cosmological questions.16 KB (2,511 words) - 18:59, 14 October 2014
- {{DISPLAYTITLE:The spacecraft}} The Planck spacecraft was designed, built and tested around two major modules.14 KB (2,136 words) - 09:37, 3 February 2015
- #[[The Planck mission|The Planck mission]] (<span style="color:red">Dupac</span>,<span style="color:b #[[The satellite|The satellite]](<span style="color:red">Dupac</span>,<span style="color:blue">M6 KB (744 words) - 09:45, 31 March 2014
- The template <tt>PlanckPapers</tt> produces references for papers cited in the text. T The syntax of <tt>PlanckPapers</tt> is126 KB (19,903 words) - 18:57, 15 December 2014
- ...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 a13 KB (2,128 words) - 15:29, 4 June 2014
