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• Simulation data
  ...rst time the realistic simulation of instrumental effects for both HFI and LFI. Moreover these simulated systematic effects are processed in the timelines * separated input sky components per HFI bolometer and LFI radiometer
  114 KB (17,146 words) - 09:49, 21 February 2022
• Product Table for PLAv2
  ...color in the products category name, e.g. <span style="color:Blue">1 year maps</span>). Please check this in the tables and let me know whether there are |rowspan="3" align="center" | LFI
  83 KB (8,209 words) - 12:21, 5 February 2015
• CMB maps
  {{DISPLAYTITLE:2018 CMB maps}} ...These products are derived from some or all of the nine frequency channel maps using different techniques and, in some cases, using other constraints from
  124 KB (18,807 words) - 18:58, 20 March 2023
• Sky temperature maps
  {{DISPLAYTITLE:2015 Sky temperature and polarization maps}} ...r the study of source variability, but they are especially interesting for characterisation purposes (see also the [[HFI-Validation | data validation]] section). The
  45 KB (6,563 words) - 06:51, 27 May 2016
• 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
• 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