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• Simulation data
  ...pipeline, and 1000 other realizations are convolved with FEBeCoP{{BibCite|mitra2010}} effective beams to be combined with the 300 noise and systematic residual The CMB MC set is generated using ''FEBeCoP''{{BibCite|mitra2010}}, which generates an effective beam for each pixel in a map at each freque
  114 KB (17,146 words) - 09:49, 21 February 2022
• HFI sims
  ...pipeline, and 1000 other realizations are convolved with FEBeCoP{{BibCite|mitra2010}} effective beams to be combined with the 300 noise and systematic residual
  29 KB (4,250 words) - 13:56, 2 July 2018
• Beams LFI
  ...ffective beams for temperature and polarisation was presented in {{BibCite|mitra2010}}. Here we summarise the main results. The observed temperature on the sky ...e polarization weight vectors, as defined in Mitra et al. (2010).{{BibCite|mitra2010}}
  23 KB (3,593 words) - 15:15, 9 November 2018
• References
  #mitra2010 bibtex=@ARTICLE{mitra2010,
  173 KB (25,381 words) - 15:29, 4 June 2014
• Effective Beams
  ...ffective beams for temperature and polarization was presented in {{BibCite|mitra2010}}, and a discussion of its application to Planck data is given in the appro FEBeCoP, the Fast Effective Beam Convolution in Pixel space{{BibCite|mitra2010}}, is an approach for representing and computing effective beams (including
  67 KB (9,735 words) - 02:01, 22 March 2018
• Beams
  ...thod for the calculation of effective beams was presented in Ref.{{BibCite|mitra2010}}. Here we summarize the main results. The observed temperature sky <math>\ ...math> are the the polarization weight vectors, as defined in Ref.{{BibCite|mitra2010}}.
  53 KB (8,689 words) - 15:07, 2 July 2018