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• Beam Window Functions
  ...ow functions have been computed with the <code>Febecop</code> Pipeline (as described [[Effective_Beams#Statistics_of_the_effective_beams_computed_using_FEBeCoP| ...Temperature beam window functions for polarized and unpolarized detectors (HFI PSB and SWBs) ====
  11 KB (1,796 words) - 11:47, 22 June 2021
• The satellite WiP
  ...diation from the sky onto a focal plane shared by detectors of the LFI and HFI, operating at 20K and 0.1K, respectively; a telescope baffle that simultane ...optical system was optimized for a set of representative detectors (eight HFI and eight LFI).
  30 KB (4,647 words) - 09:23, 10 July 2018
• TOCV1 BackUp
  ##[[HFI design, qualification, and performance|HFI design, qualification, and performance]] ##[[The HFI DPC| HFI Data Processing]]
  6 KB (744 words) - 09:45, 31 March 2014
• Terminology
  ;calibration [HFI meaning]: For a single detector, the absolute calibration is gain factor be ;detector set [HFI meaning]: a detector set (aka detset aka quad) is a combinaison of two pair
  10 KB (1,542 words) - 09:41, 2 February 2018
• NoiseCovarMatrices
  ...rix is required for maximum likelihood analysis of CMB anisotropies in the maps but also for low resolution component separation. ...e-ordered information (TOI) is cleaned of signal by interpolating the full frequency, full mission map to the sample positions on the sky.
  6 KB (1,020 words) - 18:38, 19 December 2014
• Frequency maps
  {{DISPLAYTITLE:Frequency maps in Temperature and Polarization}} ...the zodiacal light). The Planck Collaboration has made three releases of maps, in 2013, 2015 and 2018. This section describes the 2018 release. For descr
  133 KB (19,918 words) - 11:57, 14 December 2022
• Astrophysical component maps
  ...e products are derived from some or all of the nine frequency channel maps described above using different techniques and, in some cases, using other constraint ...vey by Haslam et al. (1982). This allows a direct decomposition of the low-frequency foregrounds into separate synchrotron, free-free and spinning dust componen
  23 KB (3,241 words) - 08:49, 31 May 2016
• Foreground maps
  ...e products are derived from some or all of the nine frequency channel maps described above using different techniques and, in some cases, using other constraint == Commander-derived astrophysical foreground maps ==
  107 KB (15,543 words) - 17:33, 22 October 2021
• Planck high dynamic range colour palette
  We are displaying the microwave frequency maps over the frequency span of 22-353 GHz. Our principal target --- the ...of order <math>\lesssim 10~ \mu {\rm K}</math>, in bolometric channels of HFI. Further, the foreground emission in the bright parts of the Galaxy reaches
  2 KB (388 words) - 09:01, 21 June 2016
• Planck Added Value Tools
  ...above functionalities are available both for map cutouts and for full sky maps. ...nous format (see next section), due to the size and the multiple number of maps selected.
  61 KB (9,846 words) - 08:09, 27 August 2019
• Planck Legacy Archive: mission products
  * [[Maps|Maps]] The products of the Planck mission described in this document consist of:
  3 KB (425 words) - 12:19, 12 July 2018
• HFI-systematics
  {{DISPLAYTITLE:HFI systematic effects}} Like all experiments, ''Planck'' HFI had a number of specific issues that needed to be tracked to verify that th
  10 KB (1,498 words) - 07:38, 18 January 2019
• Subpixel HFI
  ...frequency map of the bias for the frequency. Those frequency averaged bias maps are displayed in the table ''(a)''. For convenience, we also provide ''(b)'' the maps of the logarithm of the ratio of the bias variance, in each N<sub>side</sub
  6 KB (904 words) - 13:03, 30 May 2018
• BeyondPLANCK
  ...as successfully concluded in 2022. The final results from this project are described in a [https://beyondplanck.science/products/publications/ series of 17 pape * M denotes the component-frequency mixing matrix, which depends on both astrophysical foreground spectral para
  25 KB (3,590 words) - 09:35, 15 February 2023
• Sroll2
  ...of the onboard analog-to-digital convertors that was cleaned in the Planck HFI Legacy release as an empirical time-varying linear detector chain response ...ge-scale systematic effects in the Planck High Frequency Instrument legacy maps (Delouis et al., A&A 609, A38, 2019), [https://www.aanda.org/articles/aa/fu
  10 KB (1,475 words) - 11:48, 13 June 2023

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