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- {{DISPLAYTITLE:2015 CMB and astrophysical component 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 other90 KB (13,248 words) - 13:06, 21 April 2020
- * 2013-03-27, Moneti/Cardoso, [[CMB and astrophysical component maps]]: update to correct product description, add figures, remove commented tex * 2013-04-03, Mendes. [[Sky temperature maps]]: fixed incorrect links (Ticket ID DTX-918825). <span style="color:Green">12 KB (1,788 words) - 08:42, 25 September 2014
- ...ven in [[HFIpreprocessingstatics | this table]]. As a secondary product, maps with estimates of the Zodiacal light and Far-Side-Lobes contribution remove ...used extensively to investigate the (high frequency) noise properties the maps themselves and of other products described elsewhere (see e.g., the [[HFI-V35 KB (5,146 words) - 17:59, 3 July 2014
- ...eaning]: absolute calibration refers to the 0th order calibration for each channel, 1 single number, while the relative calibration refers to the component of ...f a sphere], {{BibCite|gorski2005}}) pixelation used to produce Planck sky maps (and HFI HPR).10 KB (1,539 words) - 15:11, 21 July 2014
- We are displaying the microwave frequency maps over the frequency span of 22-353 GHz. Our principal target --- the ...data where the dynamic range of signal varies considerably from channel to channel, precisely as in the case at hand.2 KB (388 words) - 09:06, 21 June 2016
- ...above functionalities are available both for map cutouts and for full sky maps. ...nous format (read next section) due to the size and the multiple number of maps selected.30 KB (5,022 words) - 16:55, 16 March 2018
