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• Frequency maps angular power spectra
  == HFI maps power spectra == ...the data, and therefore determine the best cosmological models fitting the data. Several examples of such high-<math>\ell</math> likelihoods are described,
  25 KB (3,721 words) - 17:10, 23 July 2014
• Astrophysical component separation
  ...g 'needlets' which are spherical wavelets. A special procedure is used for processing the coarsest needlet scale ...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
  12 KB (1,894 words) - 16:38, 23 July 2014
• 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
• 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 ...>: a routine to get the desired detector level spectral transmission data (HFI) and output in a structure format used by the other routines.
  28 KB (4,680 words) - 10:21, 2 October 2014
• HFI instrument annexes
  This page lists all annexes about the HFI instrument section. ** [[HFI_optical_efficiency|HFI spectral response optical efficiency measurements]]
  804 bytes (95 words) - 20:09, 17 March 2013
• Beams
  ...on to reconstruct the beam. The data are processed with the bigPlanets TOI processing (see [[Frequency_Maps#HFI_processing | here]] or Section 3.11 of {{PlanckPa The time ordered data are used to fit a two dimensional B-Spline surface using a least square min
  33 KB (5,387 words) - 14:27, 23 July 2014
• 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 HFI (6 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; * 2013-04-18: Fixes in the LFI data processing [[Map-making LFI|Map-making]] page:
  6 KB (847 words) - 15:07, 24 July 2014
• Changelog (pdf)
  :* Fixed wrong links to simulated maps in [[Simulation data]]. :* Added download instructions to [[Simulation data | simulations page]].
  5 KB (657 words) - 16:33, 1 October 2014
• Detector pointing
  ...idual detectors are known exactly a priori, we must calibrate using flight data. ...dom as far as our ability to predict the effects thereof. In this delivery HFI used a model (described below) to follow the pointing drift continuously,
  17 KB (2,628 words) - 16:32, 23 July 2014
• The spacecraft
  ...diation 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 simultaneo |'''On-board data storage capacity'''
  14 KB (2,142 words) - 14:23, 22 July 2014
• Terminology
  ;calibration [HFI meaning]: For a single detector, the absolute calibration is gain factor be ;detector set [HFI meaning]: a detector set (aka detset aka quad) is a combinaison of two pair
  10 KB (1,539 words) - 09:19, 24 July 2014

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