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- ;calibration: [LFI meaning]: absolute calibration refers to the 0th order calibration for each ...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
- ...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
- We are displaying the microwave frequency maps over the frequency span of 22-353 GHz. Our principal target --- the ...anisotropy, or even larger, in the noisy channels (radiometers in WMAP and LFI), and considerably smaller, of order <math>\lesssim 10~ \mu {\rm K}</math>,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
