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• CMB and astrophysical component maps
  ...it is obtained, followed by a description of the FITS file containing the data and associated information. # CMB-cleaned foreground maps from LFI (3 maps)
  55 KB (8,302 words) - 09:26, 20 June 2016
• Changelog
  **Updated product descriptions to take into account the inpainting data contained in the SMICA and NILC maps; * 2013-04-12: Added LFI 70 GHz 2048 product to [[Map-making_LFI | Map-making]];
  6 KB (847 words) - 15:07, 24 July 2014
• Changelog (pdf)
  :* Fixed reference to two Planck publications in [[LFI systematic effect uncertainties]] page. :* Fixed wrong links to simulated maps in [[Simulation data]].
  5 KB (657 words) - 16:33, 1 October 2014
• Detector pointing
  ...idual detectors are known exactly a priori, we must calibrate using flight data. ...model (described below) to follow the pointing drift continuously, while LFI uses two different focal plane description for the two time periods separat
  17 KB (2,628 words) - 16:32, 23 July 2014
• The spacecraft
  ...ssing radiation from the sky onto a focal plane shared by detectors of the LFI and HFI, operating at 20K and 0.1K respectively; a telescope baffle that si |Planck operated for 32 months with both instruments; the LFI continues surveying the sky
  14 KB (2,142 words) - 14:23, 22 July 2014
• Terminology
  ;calibration: [LFI meaning]: absolute calibration refers to the 0th order calibration for each ...ed effect of the instrumental response, the scanning strategy and the data processing.
  10 KB (1,539 words) - 09:19, 24 July 2014

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