Publisher： Edp Sciences
E-ISSN： 1638-1963|23|issue|189-203
ISSN： 1633-4760
Source： EAS Publications Series, Vol.23, Iss.issue, 2010-03, pp. : 189-203
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Abstract
Future cosmology space missions will concentrate on measuring thepolarization of the Cosmic Microwave Background (CMB), which potentiallycarries invaluable information about the earliest phases of the evolutionof our universe. Such ambitious projects will ultimately be limited bythe sensitivity of the instrument and by the accuracy at whichpolarized foreground emission from our own Galaxy can be subtractedout. We present the
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