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• Main Page
  ..."> This is the Explanatory Supplement development page for the Planck 2015 data release </span> ...y Supplement (2013 and 2015), including this one, are not fully up-to-date and will be discontinued during 2018. </span>
  6 KB (669 words) - 21:21, 6 August 2018
• LFI design, qualification, and performance
  ...ation stage, detector diodes, and all the electronics for data acquisition and bias supply. ...at the telescope focal area, the other on the 300 K portion of the Planck satellite. These design features allow the entire front-end LNA dissipation to be <0.
  50 KB (7,826 words) - 22:29, 4 February 2015
• Operational history
  The major operational phases and milestones are: ==Launch and transfer to orbit==
  11 KB (1,616 words) - 12:31, 26 March 2014
• Simulation data
  ...), together with separate sets of Monte Carlo realizations of the CMB and the instrument noise. ...ull mission CMB simulations: 1000 for each of the nine Planck frequencies, and for two different sets of cosmological parameters.
  46 KB (7,032 words) - 12:02, 29 March 2016
• Glossary
  ...es with well modelled spectral energy distributions or well known spectra, and requires that the detector's spectral bandpass is also well known. * '''DMC''': Data Management Component, the databases used at the HFI and LFI DPCs.
  7 KB (1,093 words) - 13:07, 7 July 2015
• Planck Collaboration
  ...humb | '''A pictorial overview of the major participating funding agencies and scientific institutes.''']] ...mission, and who participate in the scientific exploitation of the Planck data during the proprietary period, which nominally ends with the release of the
  9 KB (1,372 words) - 08:30, 21 September 2012
• Timelines
  ...me during the mission. For LFI, refer to {{PlanckPapers|planck2014-a03}}, and for HFI, to {{PlanckPapers|planck2014-a08}}. ...d 3 timelines of coordinates, corresponding to the two angular coordinates and one position angle.
  28 KB (4,415 words) - 18:43, 21 August 2015
• Sky temperature maps
  {{DISPLAYTITLE:2015 Sky temperature and polarization maps}} ...e [[HFI-Validation | data validation]] section). The details of the start and end of the time ranges are given in the table below.
  45 KB (6,681 words) - 11:55, 16 May 2017
• Map-making
  {{DISPLAYTITLE:Mapmaking and photometric calibration}} ...ures used by the HFI DPC to build detector and frequency maps for the 2015 data release. They are described in {{PlanckPapers|planck2014-a09}}.
  12 KB (1,956 words) - 12:56, 7 July 2015
• TOI processing
  ...ing involves modifying the TOI itself for the conversion to absorbed power and the correction of glitch tails. It also adds a flag TOI that masks the TOI ...lmost no missing data in the TOIs, except for a few hundred samples of 545 and 857 GHz TOIs, which were lost in the on-board compression due to saturation
  18 KB (2,794 words) - 14:55, 26 September 2016
• The Planck mission
  ...metry and content of the Universe, and which theories describing the birth and evolution of the Universe are correct. To achieve this ambitious objective, the Universe and is observed to have an average temperature of 2.7 K. Small deviations from
  13 KB (2,044 words) - 09:08, 21 August 2013
• Map-making LFI
  The main output consists of temperature and polarization maps. As auxiliary information, the code produces a hit-count map and a white noise covariance matrix.
  26 KB (3,949 words) - 15:33, 1 March 2017
• References
  title = {Planck 2013 results: Overview of Planck Products and Scientific Results (p01)}, title = {Planck 2013 results: The Low Frequency Instrument data processing (p02)},
  173 KB (25,381 words) - 15:29, 4 June 2014
• Main Page2
  #[[The satellite|The satellite]] ##[[HFI design, qualification, and performance|HFI design, qualification, and performance]] <span style="color:red">(Lamarre/Pajot)</span>
  2 KB (265 words) - 17:39, 25 January 2013
• Main Page3
  #[[The satellite|The satellite]] ##[[HFI design, qualification, and performance|HFI design, qualification, and performance]] <span style="color:red">(Lamarre/Pajot)</span>
  6 KB (770 words) - 17:33, 29 January 2013
• LFI systematic effect uncertainties
  ...ions to the measured timelines, and effects which are dependent on the sky and that cannot be considered independently from the observation strategy. ...effects, all the details can be found in {{PlanckPapers|planck2013-p02a}} and {{PlanckPapers|planck2014-a04||Planck-2015-A04}}.
  20 KB (2,907 words) - 13:28, 19 September 2016
• HFI operations timeline
  ...activities that are known to have affected or might have affected the HFI data. The time information is the start time of the event in On Board Time. The ...tions on the satellite SerVice Module that might have an impact on the HFI data;
  27 KB (2,766 words) - 19:41, 11 December 2014
• DatesObs
  ...riability, comparison with external observations, and understanding of the survey strategy. The files themselves are in FITS format, and gzipped, with data in the first extension
  2 KB (375 words) - 21:49, 29 January 2015
• References2
  keywords = {Astrophysics - Galaxy Astrophysics, Astrophysics - Cosmology and Extragalactic Astrophysics}, adsnote = {Provided by the SAO/NASA Astrophysics Data System}
  39 KB (5,438 words) - 09:40, 20 May 2014
• LFIAppendix
  ...ch were already briefly described in the main [[LFI design, qualification, and performance|LFI instrument]] page. .... Dual-profiled LFI horns are composed of a sine-squared profiled section, and an exponential profile near the aperture plane.
  60 KB (9,314 words) - 08:48, 2 January 2015

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