Faraday Rotation as a Diagnostic of Galactic Foreground Contamination of CMB Maps

Details Faraday Rotation as a Diagnostic of Galactic Foreground Contamination of CMB Maps Faraday Rotation as a Diagnostic of Galactic Foreground Contamination of CMB Maps

2003-06-25

arxiv.org/abs/astro-ph/0306529v2

Mon.Not.Roy.Astron.Soc.347:52,2004

Astronomy and Astrophysics

Astrophysics

8 pages, 1 figure, accepted for publication in MNRAS

Scientific paper

10.1111/j.1365-2966.2004.07241.x

We present a diagnostic test of possible Galactic contamination of cosmic microwave background sky maps designed to provide an independent check on the methods used to compile these maps. The method involves a non-parametric measurement of cross-correlation between the Faraday rotation measure (RM) of extragalactic sources and the measured microwave signal at the same angular position. We argue that statistical properties of the observed distribution of rotation measures are consistent with a Galactic origin, an argument reinforced by a direct measurement of cross-correlation between dust, free-free and synchrotron foreground maps and RM values with the strongest correlation being for dust and free-free. We do not find any statistically compelling evidence for correlations between the RM values and the COBE DMR maps at any frequency, so there is no evidence of residual contamination in these CMB maps. On the other hand, there is a statistically significant correlation of RM with the preliminary WMAP individual frequency maps which remains significant in the Tegmark et al. Wiener-filtered map but not in the Internal Linear Combination map produced by the WMAP team.

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