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• PSO processing
  ...L was required by MOC to prepare the lists of pointings that were uploaded to the satellite. ...e name indicates it covers long periods of time. In general it was updated to cover
  3 KB (444 words) - 16:04, 21 May 2014
• Specially processed maps
  ...contents are described below. The convergence map "dat_klm.fits" that can be found in the tarball, has been categorized as COM_Lensing-Convergence-dat-k ...aps of the noise in the full mission Planck y-maps that are also provided. To complement this we also provide the power spectra of the noise estimate map
  14 KB (2,235 words) - 07:29, 7 August 2017
• CMB spectrum & Likelihood Code
  ...s spectrum are the 68% confidence limits and include the uncertainties due to foreground subtraction. ...Planck TT+lowP in table 3 of Planck-2015-A15[3]). Residuals with respect to this model are shown in the lower panel. The error bars show ±1&sigm
  61 KB (9,011 words) - 08:06, 15 May 2017
• Timelines
  ...mission. For LFI, refer to {{PlanckPapers|planck2014-a03}}, and for HFI, to {{PlanckPapers|planck2014-a08}}. ...leaned and calibrated signal and 3 timelines of coordinates, corresponding to the two angular coordinates and one position angle.
  28 KB (4,415 words) - 18:43, 21 August 2015
• HFI Detector Spectral Response
  ...near-band spectral regions surrounding CO rotational transitions in order to support the CO extraction component separation effort <span style="color:#0 ...eter (FTS). The required accuracy to which the spectral transmission is to be recovered is 1<math>\%</math> (see §[[#Conformity with requirements|Req.]]
  58 KB (7,853 words) - 15:51, 5 October 2012
• TOI processing
  ...tails. It also adds a flag TOI that masks the TOI samples that are not to be projected onto maps for various reasons. ...s of 545 and 857 GHz TOIs, which were lost in the on-board compression due to saturation on the Galactic centre crossings.
  18 KB (2,794 words) - 14:55, 26 September 2016
• The satellite
  |$\pm 0.6$ arcmin/sec (changes due to manoeuvers); stability during inertial pointing <math>\sim 6.5\times 10^{-5 |'''Max angle of spin axis to Sun'''
  14 KB (2,170 words) - 09:29, 21 May 2014
• Beams LFI
  ...- RCA) is named as LFIXXM or LFIXXS. XX is the RCA number ranging from 18 to 28; M and S are the two polarizations, namely the main-arm and side-arm of ...{{PlanckPapers|planck2014-a05}}. Please note that many figures below refer to the previous Planck release {{PlanckPapers|planck2013-p02d}} since they hav
  24 KB (3,748 words) - 10:02, 26 September 2016
• HL-sims
  ...O) and create sky maps and catalogues at the specified frequencies. It can be supplemented by ad-hoc simulation software for particular (theoretical) CMB ...of the actual instruments. Alternatively, the output can be used as input to a detailed simulation of the instrumental behaviour.
  5 KB (779 words) - 16:03, 21 May 2014
• HFI detection chain
  Two extra bolometers, not optically coupled to the telescope, are added to the focal plane to monitor thermal noise (dark bolometers).
  14 KB (2,155 words) - 23:49, 12 November 2014
• HFI spectral response data processing
  ...t ZPD and that each spectrum has identical frequency sampling and can thus be averaged together. An example of a combined interferogram data set is illus ...Beer 1.5 apodization function{{BibCite|NaylorApod07}} has been selected to be used for the final spectral transmission profile data set, since it represe
  8 KB (717 words) - 08:00, 10 December 2014
• Astrophysical component separation
  ...eighting coefficients varying over the sky and over the multipole range up to <math>\ell=3200</math> and it does so using 'needlets' which are spherical : In this work, the NILC algorithm is applied to all Planck channels from 44 to 857 GHz omitting only the 30 GHz channel.
  14 KB (2,212 words) - 15:15, 26 September 2016
• TestMassEditing
  ...ble pointing part in each pointing period. These maps are used extensively to investigate the (high frequency) noise properties the maps themselves and o To help in further processing, there are also masks of the Galactic Plane and
  35 KB (5,146 words) - 17:59, 3 July 2014
• TestReplace2
  Two extra bolometers not optically coupled to the telescope are added to the focal plane to monitor thermal noise (dark bolometers).
  13 KB (2,128 words) - 15:29, 4 June 2014