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• HFI data compression
  ==Data compression== ===Data compression scheme===
  8 KB (1,269 words) - 09:45, 10 December 2014
• HFI performance summary
  ...ery stable conditions during the whole mission, and practically all of the data were correctly recorded. ...from {{PlanckPapers|planck2014-a07}}) applies to the 2015 and 2018 release products.
  5 KB (674 words) - 14:36, 2 July 2018
• CMB Maps test
  The CMB data are in thermodynamic temperature units (uK_cmb), and the residuals are in t ...applied to Planck simulations Leach et al., 2008 and to WMAP polarisation data Fernandez-cobos et al., 2012. In the cleaning process, no assumptions about
  7 KB (1,103 words) - 18:38, 1 March 2013
• Astrophysical component maps test
  We describe diffuse foreground products for the Planck 2013 release. See Planck paper P06-Component Separation <cit The products below contain the result of the fitting for one foreground component at low
  22 KB (2,713 words) - 18:48, 1 March 2013
• Unit conversion and Color correction
  ...is delivered as a tarfile and contains a detailed instruction manual. The data and software file requirements are provided below along with basic use inst ...ro</tt>: 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
  ...d time response function, and the software low-pass filter, applied to the data. The "effective beam" represents the averaging of the signal due to the sca = The 2015 and 2018 Data Releases =
  53 KB (8,689 words) - 15:07, 2 July 2018
• CMB and astrophysical component maps
  ...it is obtained, followed by a description of the FITS file containing the data and associated information. ...his data release, to fully characterize the large-scale residuals from the data or from simulations. Therefore all results published by the Planck Collabor
  73 KB (10,660 words) - 08:15, 21 August 2016
• Summary from PR1
  ...r details, users are advised to consult the Planck papers accompanying the data release. ...or added, every time more information becomes available and at every major data release.
  1 KB (217 words) - 16:06, 25 March 2013
• Changelog
  ...processing]], [[Spectral response]], [[HFI-Validation]], [[Summary of HFI data characteristics]], [[Compact Source catalogues]], [[The RIMO]], [[Effective ...12, Zacchei, [[CMB and astrophysical component maps]]: add COMMANDER-Ruler products. <span style="color:Green">Moved to public ES.</span>
  12 KB (1,788 words) - 08:42, 25 September 2014
• TOC WorkInProgress
  #[[Data processing]] ##[[The HFI DPC| HFI Data Processing]]
  5 KB (581 words) - 09:33, 31 March 2014
• The Planck mission WiP
  instruments, as well as the ensuing data analysis ...continued to survey the sky for a large part of 2013, providing even more data to improve the final Planck results.
  15 KB (2,330 words) - 12:43, 17 July 2018
• Beam Window Functions
  === QuickPol effective beam window products === The effective beam products are defined for each multipole 0 &le; &#8467; &le; &#8467;_max =
  11 KB (1,796 words) - 11:47, 22 June 2021
• The satellite WiP
  |'''On-board data storage capacity''' |'''Data transmission rate to ground (max)'''
  30 KB (4,647 words) - 09:23, 10 July 2018
• TOCV1 BackUp
  ##[[Data flow overview|Data flow overview]] (<span style="color:red">Leonardi</span>,<span style="color ##[[MOC data transfer and storage|MOC data transfer and storage]]
  6 KB (744 words) - 09:45, 31 March 2014
• Terminology
  ...ombined effect of the instrumental response, the scanning strategy and the data processing. ...he first half of each pointing period (typically 20 minutes of contiguous data) and the one built with the second half. This difference effectively remove
  10 KB (1,542 words) - 09:41, 2 February 2018
• ADC correction
  ...averaged and transmitted to the ground. The TOI data delivered in the HFI products are made up of these averaged values, with the raw signal of a bolometer fo ...orrection cannot be done using only the TOI values, but requires ancillary data from ground-based tests and additional tests done during the LFI extension
  1 KB (169 words) - 14:55, 23 May 2015
• Frequency maps
  ...interesting for characterization purposes (see also the [[HFI-Validation | data validation]] section), though some are also useful for the study of source Sky maps are produced by appropriately combining the data from all working detectors in a frequency channel over some period of the m
  133 KB (19,918 words) - 11:57, 14 December 2022
• Astrophysical component maps
  ...it is obtained, followed by a description of the FITS file containing the data and associated information. ...paper {{PlanckPapers|planck2014-a12}} for a detailed description of these products. Further scientific discussion and interpretation may be found in {{PlanckP
  23 KB (3,241 words) - 08:49, 31 May 2016
• Foreground maps
  ...it is obtained, followed by a description of the FITS file containing the data and associated information. ...we do not release parametric temperature foreground products from the 2018 data set, but rather recommend continued usage of the 2015 temperature model. Fo
  107 KB (15,543 words) - 17:33, 22 October 2021
• Planck Added Value Tools
  ...arts is intended to allow users to use the existing products to create new data. ...g the user with several tools to create a map cutout from the time-ordered data.
  61 KB (9,846 words) - 08:09, 27 August 2019

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