Predicting the Polarization of The Microwave Background from the WMAP Temperature Maps

Details Predicting the Polarization of The Microwave Background from the WMAP Temperature Maps Predicting the Polarization of The Microwave Background from the WMAP Temperature Maps

2003-07-07

arxiv.org/abs/astro-ph/0307118v1

Astronomy and Astrophysics

Astrophysics

To be published in the proceedings of "The Cosmic Microwave Background and its Polarization", New Astronomy Reviews, (eds. S.

Scientific paper

In this paper, we study how to predict the polarization of the Cosmic
Microwave Background using knowledge of only the temperature (intensity) and
the cross-correlation between temperature and polarization. We derive a
``Wiener prediction'' method and apply it to the WMAP all-sky CMB temperature
maps and to the MAXIMA field.

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