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• The LFI DPC
  ...etry handling]] • [[Pre-processing LFI#Auxiliary data handling|Auxiliary data handling]]'' ...ulations]] • [[HFI-Validation#Simulations_versus_data|Simulations versus data]] • [[HFI-Validation#Systematics_Impact_Estimates|Systematics Impact Esti
  8 KB (1,072 words) - 20:27, 4 February 2015
• Additional angular power spectra
  ...the product. In particular any limitations and approximations used in the data processing should be listed. Avoiding detailed descriptions of methods and ...erate this product (down to file names), as well as any external ancillary data sets which were used.</span>
  2 KB (338 words) - 18:41, 26 February 2013
• CMB spectrum & Likelihood Code
  ...separation algorithm applied to the combination of Planck 2015 temperature data between 30 and 857 GHz, the 9-year WMAP sky maps, and the 408-MHz Haslam et ...shown in the figure below, cover the multipole range &#8467; = 2-1996. The data points relative to the multipole range &#8467; = 2-29 are quadratic maximum
  61 KB (9,011 words) - 08:06, 15 May 2017
• Frequency map angular power spectrum
  ...the product. In particular any limitations and approximations used in the data processing should be listed. Avoiding detailed descriptions of methods and ...erate this product (down to file names), as well as any external ancillary data sets which were used.</span>
  3 KB (478 words) - 18:38, 26 February 2013
• References
  title = {Planck 2013 results: The Low Frequency Instrument data processing (p02)}, title = {Planck 2013 results: High Frequency Instrument Data Processing (p03)},
  173 KB (25,381 words) - 15:29, 4 June 2014
• Frequency maps angular 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, ...e high-<math>\ell</math> likelihood of a given theoretical model given the data available. -->
  25 KB (3,718 words) - 15:37, 18 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
• Astrophysical component maps test
  applied to the data at full resolution in order to obtain the provided products at Nside=2048. ===Meta Data===
  22 KB (2,713 words) - 18:48, 1 March 2013