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• Compact Source catalogues
  ==Planck Catalogue of Compact Sources== ...ency lists of sources, both Galactic and extragalactic, extracted from the Planck maps.
  25 KB (3,934 words) - 15:07, 26 September 2016
• HFI detection chain
  ...of the HFI - the detectors - are bolometers, solid-state devices in which the incoming radiation dissipates its energy as heat that increases the temperature of a
  14 KB (2,155 words) - 23:49, 12 November 2014
• Effective Beams
  ...etry of the beam and the uneven distribution of scanning angles across the sky. ..., the objects whose convolution with the true CMB sky produce the observed sky map.
  22 KB (3,180 words) - 10:37, 5 February 2015
• Main Page3
  #[[The Planck mission|The Planck mission]] <span style="color:red">(Dupac)</span> #[[The satellite|The satellite]]
  6 KB (770 words) - 17:33, 29 January 2013
• List of acronyms
  * '''DMC''' : Data Management Component, the databases used at the HFI and LFI DPCs * '''FLS ''' : (Planck) First Light Survey
  6 KB (650 words) - 23:43, 1 February 2015
• LFI systematic effect uncertainties
  ...are dependent on the sky and that cannot be considered independently from the observation strategy. ...und in {{PlanckPapers|planck2013-p02a}} and {{PlanckPapers|planck2014-a04||Planck-2015-A04}}.
  20 KB (2,907 words) - 13:28, 19 September 2016
• References2
  author = {Planck Collaboration XXXI,}, title = {Planck 2013 results: All-sky model of thermal dust emission},
  39 KB (5,438 words) - 09:40, 20 May 2014
• LFIAppendix
  ...h component of the LFI instrument, which were already briefly described in the main [[LFI design, qualification, and performance|LFI instrument]] page. ...mposed of a sine-squared profiled section, and an exponential profile near the aperture plane.
  60 KB (9,314 words) - 08:48, 2 January 2015
• Frequency maps angular power spectra
  {{DISPLAYTITLE:Sky temperature power spectra}} Angular power spectra of cut sky CMB dominated maps are provided to allow independent cosmological analysis
  25 KB (3,718 words) - 15:37, 18 July 2014
• Astrophysical component separation
  See the Component Separation paper {{PlanckPapers|planck2013-p06}} {{PlanckPapers|p ...' which are spherical wavelets. A special procedure is used for processing the coarsest needlet scale
  14 KB (2,212 words) - 15:15, 26 September 2016
• Astrophysical component maps test
  We describe diffuse foreground products for the Planck 2013 release. See Planck paper P06-Component Separation <cite>#planck2013-p06</cite> for a detailed ...e result of the fitting for one foreground component at low frequencies in Planck bands,
  22 KB (2,713 words) - 18:48, 1 March 2013
• Beams
  = The 2015 Data Release = ...tions of Uranus and Neptune are used to obtain an absolute calibration for the 545 and 857 GHz channels.
  52 KB (8,515 words) - 12:52, 7 July 2015
• CMB and astrophysical component maps
  ...how it is obtained, followed by a description of the FITS file containing the data and associated information. All the details can be found in {{PlanckPapers|planck2014-a11}} and {{PlanckPapers|
  90 KB (13,248 words) - 13:06, 21 April 2020
• Changelog
  * 2013-04-03, Mendes. [[Sky temperature maps]]: fixed incorrect links (Ticket ID DTX-918825). <span sty ...Mendes, [[CMB and astrophysical component maps]]: Fixed incorrect links to the new nilc and smica CMB maps. <span style="color:Green">Moved to public ES.<
  12 KB (1,788 words) - 08:42, 25 September 2014
• TOC WorkInProgress
  ##[[The Planck mission_WiP|The Planck mission]] ##[[The satellite_WiP|The satellite]]
  5 KB (581 words) - 09:33, 31 March 2014
• TOCV1 BackUp
  #[[The Planck mission|The Planck mission]] (<span style="color:red">Dupac</span>,<span style="color:blue">Le #[[The satellite|The satellite]](<span style="color:red">Dupac</span>,<span style="color:blue">M
  6 KB (744 words) - 09:45, 31 March 2014
• TestMassEditing
  ...ngstatics | this table]]. As a secondary product, maps with estimates of the Zodiacal light and Far-Side-Lobes contribution removed are also provided. ...s the maps themselves and of other products described elsewhere (see e.g., the [[HFI-Validation | data validation]] section).
  35 KB (5,146 words) - 17:59, 3 July 2014
• TestReplace2
  ...of the HFI - the detectors - are bolometers, solid-state devices in which the incoming radiation dissipates its energy as heat that increases the temperature of a
  13 KB (2,128 words) - 15:29, 4 June 2014
• Terminology
  ;4K lines: EMI/EMC influence of the 4K cooler mechanical motion on the bolometer readout electronics. ...led spectral energy distributions or well known spectra, and requires that the detector's spectral bandpass also be well known.
  10 KB (1,539 words) - 15:11, 21 July 2014
• NoiseCovarMatrices
  ...matrix is required for maximum likelihood analysis of CMB anisotropies in the maps but also for low resolution component separation. ...detector noise. We do this for each detector at roughly one day intervals. The process is
  6 KB (1,020 words) - 18:38, 19 December 2014

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