The C-Band All-Sky Survey (C-BASS): Simulated parametric fitting in single pixels in total intensity and polarization

The cosmic microwave background (CMB) B-mode signal is potentially weaker than the diffuse Galactic foregrounds over most of the sky at any frequency. A common method of separating the CMB from these foregrounds is via pixel-based parametric-model fitting. There are not currently enough all-sky maps...

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Bibliographic Details
Main Authors:	Jew, L, Taylor, AC, Jones, ME, Barr, A, Chiang, HC, Dickinson, C, Grumitt, RDP, Harper, SE, Heilgendorff, HM, Hill-Valler, J, Jonas, JL, Leahy, JP, Leech, J, Pearson, TJ, Peel, MW, Readhead, ACS, Sievers, J
Format:	Journal article
Published:	Oxford University Press 2019

The C-Band All-Sky Survey (C-BASS): Simulated parametric fitting in single pixels in total intensity and polarization

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