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• LFI-Validation
  All the details can be found in {{PlanckPapers|planck2013-p02}}.
  13 KB (1,992 words) - 16:09, 23 July 2014
• HFI cold optics
  The cold optics is described in {{PlanckPapers|ade2010}}}. ...description of the HFI optical design and beam performances is given in {{PlanckPapers|maffei2010}}.
  25 KB (3,767 words) - 15:43, 22 July 2014
• Spectral response
  ...Further details on the definition of these parameters are available in {{PlanckPapers|planck2013-p03d}}.
  18 KB (805 words) - 14:32, 23 July 2014
• Compact Source catalogues
  ...from each of Planck's nine frequency channels. It is fully described in {{PlanckPapers|planck2013-p05}}. ...are based on aperture photometry, PSF fitting and Gaussian fitting (see {{PlanckPapers|planck2013-p05}} for a detailed description of these additional photometrie
  12 KB (1,879 words) - 16:37, 23 July 2014
• HFI detection chain
  {{PlanckPapers|rosset2010}}. The thermometers are ...e the Q and U Stokes parameters with minimal correction for the pointing {{PlanckPapers|rosset2010}}. Residual systematics will come from the differences between t
  13 KB (2,126 words) - 15:54, 22 July 2014
• Effective Beams
  ...is given in the appropriate LFI {{PlanckPapers|planck2013-p02d}} and HFI {{PlanckPapers|planck2013-p03c}} papers. Relevant details of the processing steps are give
  23 KB (3,381 words) - 12:28, 28 August 2014
• Cosmological Parameters
  ...arameter tables. Definitions, conventions and reference are contained in {{PlanckPapers|planck2013-p11}}. ...n into account when comparing with BBN results reported in Sect. 6.4. of {{PlanckPapers|planck2013-p11}}, which use an updated version for the neutron lifetime (an
  10 KB (1,566 words) - 17:32, 23 July 2014
• Summary of HFI data characteristics
  ...contains the information from the summary section of the HFI DPC paper {{PlanckPapers|planck2013-p03}} which describes the most important characteristics of the
  449 bytes (64 words) - 15:03, 23 July 2014
• Survey scanning and performance
  ...ng strategy'', makes use of the characteristics of the Planck spacecraft {{PlanckPapers|planck2011-1-1}} and orbit in order to achieve the survey goals in terms of [[File:AHF_353_OD389.png|thumb|400px|The 353 GHz detectors {{PlanckPapers|lamarre2010}} integration time after 389 Operational Days (the unit is seco
  16 KB (2,501 words) - 14:28, 22 July 2014
• Summary LFI
  ...e 1 below. All the details can be found in the LFI data processing paper {{PlanckPapers|planck2013-p02}}. ...ective beam. Those are the values used in the source extraction pipeline {{PlanckPapers|planck2013-p05}}.
  2 KB (296 words) - 16:20, 23 July 2014
• LFI systematic effect uncertainties
  ...report a brief summary of these effects, all the details can be found in{{PlanckPapers|planck2013-p02a}}. ...aps. The CMB curve corresponds to the Planck best-fit model presented in {{PlanckPapers|planck2013-p08}}.'''
  16 KB (2,578 words) - 16:05, 23 July 2014
• L3 LFI
  ...sked Galactic plane and point sources using masks described in Sec. 3 of {{PlanckPapers|planck2013-p06}}. In particular, we have used the 70% Galactic mask for 44 ...ment between the observed spectra and the Planck Likelihood Code bestfit {{PlanckPapers|planck2013-p08}} when adding a simple foreground component to account for u
  2 KB (270 words) - 16:19, 23 July 2014
• LFIAppendix
  ...nels. Details about the definition of colour corrections are provided in {{PlanckPapers|planck2011-1-6}}. As detailed in {{PlanckPapers|planck2011-1-4}}, one effect detected during the first survey was the daily
  59 KB (9,067 words) - 10:10, 23 July 2014
• Frequency maps angular power spectra
  ...h-<math>\ell</math> likelihoods are described, discussed and compared in {{PlanckPapers|planck2013-p08}}. ...Y}(\ell)</math> of the relative error on <math>B^{XY}_{\ell}</math> (see {{PlanckPapers|planck2013-p03c|1|HFI time response and beams paper}}), defined for <math>p
  25 KB (3,721 words) - 17:10, 23 July 2014
• Astrophysical component separation
  See the Component Separation paper {{PlanckPapers|planck2013-p06}} for details.
  12 KB (1,894 words) - 16:38, 23 July 2014
• LFI overview
  ...ntre frequency. A detailed description of the LFI instrument is given in {{PlanckPapers|bersanelli2010}}, and references therein.
  3 KB (479 words) - 16:15, 22 July 2014
• Unit conversion and Color correction
  ...t (i.e. 2.2.1.2, 4.4.5, and 4.6), as well as the Spectral Response Paper {{PlanckPapers|planck2013-p03d}} for details of the derivation of the detector spectra and ...dpass routine. Details of the unit conversion equations are available in {{PlanckPapers|planck2013-p03d}}.
  28 KB (4,680 words) - 10:21, 2 October 2014
• Beams
  In {{PlanckPapers|planck2013-p03c}} we consider two models of the beam in order to better und ...cessing (see [[Frequency_Maps#HFI_processing | here]] or Section 3.11 of {{PlanckPapers|planck2013-p03}} for more info). We use JPL Horizons ephemerides to determi
  33 KB (5,387 words) - 14:27, 23 July 2014
• CMB and astrophysical component maps
  All the details can be found in {{PlanckPapers|planck2013-p06}}. ...isotropy map. These are the maps used in the component separation paper {{PlanckPapers|planck2013-p06}}.
  55 KB (8,302 words) - 09:26, 20 June 2016
• Detector pointing
  ...detector transfer function, which is complex in the Fourier domain (see {{PlanckPapers|planck2013-p03c}}). This phase shift was not measured during normal operati ...e radiometer electronics box assembly (REBA) as discussed more fully in {{PlanckPapers|planck2013-p03}}.
  17 KB (2,628 words) - 16:32, 23 July 2014

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