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- {{DISPLAYTITLE:2015 CMB maps}} ...These products are derived from some or all of the nine frequency channel maps described above using different techniques and, in some cases, using other73 KB (10,660 words) - 08:15, 21 August 2016
- Instrument (LFI), and a SAMBA-like High Frequency Instrument (HFI), ...uency Instrument (LFI), which was able to work at higher temperatures than HFI, continued to survey the sky for a large part of 2013, providing even more15 KB (2,330 words) - 12:43, 17 July 2018
- ...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
- {{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 descr133 KB (19,918 words) - 11:57, 14 December 2022
- ...These products are derived from some or all of the nine frequency channel maps described above using different techniques and, in some cases, using other == Commander-derived astrophysical foreground maps ==107 KB (15,543 words) - 17:33, 22 October 2021
- ...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
- ...eaned in the Planck HFI Legacy release as an empirical time-varying linear detector chain response which is the first-order effect. The SRoll2 method fits the ...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/fu10 KB (1,475 words) - 11:48, 13 June 2023