Some sources of systematic errors on CMB polarized measurements with bolometers
arXiv:astro-ph/0112488 · doi:10.1063/1.1471849
Abstract
Some sources of systematic errors, specific to polarized CMB measurements using bolometers, are examined. Although the evaluations we show have been made in the context of the Planck mission (and more specifically the Planck HFI), many of our conclusions are valid for other experiments as well.
Contribution to the International workshop "Background Polarized Emission from Radio to Microwave Wavelengths" October 9-12, 2001, Bologna, Italy