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• Astrophysical component separation
  ...s, a simpler model is employed, in which only a single joint power-law low-frequency foreground model is included in the fit, accouting simultaneously for synch ...h accounts explicitly for the specific instrumental beam of each frequency channel. Furthermore, by processing the data at full angular resolution Commander2
  16 KB (2,572 words) - 10:22, 10 July 2018
• CMB Maps test
  ...ption of the product, including e.g. figures related to the contents (e.g. maps, tables), and some explanation of its scientific meaning. If there are scie ...for the CMB channels, and MJy/sr for the Galactic channels). As usual, all maps are in Galactic coordinate and use Nested ordering scheme.
  7 KB (1,103 words) - 18:38, 1 March 2013
• Astrophysical component maps test
  ====Low frequency foreground component==== ...uced to Nside=256 first. Parameters related to the foreground scaling with frequency are estimated at that resolution
  22 KB (2,713 words) - 18:48, 1 March 2013
• Unit conversion and Color correction
  ...in this release contains only the updated bandpass profiles concerning the maps included in this release. <span style="color:#ff0000">'''It is therefore n ...>: a routine to get the desired detector level spectral transmission data (HFI) and output in a structure format used by the other routines.
  29 KB (4,821 words) - 09:34, 10 July 2018
• Beams
  ...truction of the spatial response for the Planck High Frequency Instrument (HFI) is informed by observation of planets. Furthermore, observations of Uranus ...ts used for the 2015 (PR2) release of ''Planck'' data, can be found in the HFI DPC Paper 1 {{PlanckPapers|planck2014-a08}}.
  53 KB (8,689 words) - 15:07, 2 July 2018
• CMB and astrophysical component maps
  {{DISPLAYTITLE:2015 CMB maps}} ...These products are derived from some or all of the nine frequency channel maps described above using different techniques and, in some cases, using other
  73 KB (10,660 words) - 08:15, 21 August 2016
• Changelog
  * 2013-03-27, Moneti/Cardoso, [[CMB and astrophysical component maps]]: update to correct product description, add figures, remove commented tex * 2013-04-03, Mendes. [[Sky temperature maps]]: fixed incorrect links (Ticket ID DTX-918825). <span style="color:Green">
  12 KB (1,788 words) - 08:42, 25 September 2014
• Terminology
  ;calibration [HFI meaning]: For a single detector, the absolute calibration is gain factor be ...eaning]: absolute calibration refers to the 0th order calibration for each channel, 1 single number, while the relative calibration refers to the component of
  10 KB (1,542 words) - 09:41, 2 February 2018
• Frequency maps
  {{DISPLAYTITLE:Frequency maps in Temperature and Polarization}} ...the zodiacal light). The Planck Collaboration has made three releases of maps, in 2013, 2015 and 2018. This section describes the 2018 release. For descr
  133 KB (19,918 words) - 11:57, 14 December 2022
• Astrophysical component maps
  ...These products are derived from some or all of the nine frequency channel maps described above using different techniques and, in some cases, using other ...vey by Haslam et al. (1982). This allows a direct decomposition of the low-frequency foregrounds into separate synchrotron, free-free and spinning dust componen
  23 KB (3,241 words) - 08:49, 31 May 2016
• Foreground maps
  ...These products are derived from some or all of the nine frequency channel maps described above using different techniques and, in some cases, using other == Commander-derived astrophysical foreground maps ==
  107 KB (15,543 words) - 17:33, 22 October 2021
• Planck high dynamic range colour palette
  We are displaying the microwave frequency maps over the frequency span of 22-353 GHz. Our principal target --- the ...data where the dynamic range of signal varies considerably from channel to channel, precisely as in the case at hand.
  2 KB (388 words) - 09:01, 21 June 2016
• Planck Added Value Tools
  ...above functionalities are available both for map cutouts and for full sky maps. ...nous format (see next section), due to the size and the multiple number of maps selected.
  61 KB (9,846 words) - 08:09, 27 August 2019
• Subpixel HFI
  ...frequency map of the bias for the frequency. Those frequency averaged bias maps are displayed in the table ''(a)''. For convenience, we also provide ''(b)'' the maps of the logarithm of the ratio of the bias variance, in each N<sub>side</sub
  6 KB (904 words) - 13:03, 30 May 2018
• BeyondPLANCK
  ...ssive efforts, several known outstanding issues regarding the final Planck maps remained unresolved at the end of the funded analysis phase, and several ex * M denotes the component-frequency mixing matrix, which depends on both astrophysical foreground spectral para
  25 KB (3,590 words) - 09:35, 15 February 2023

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