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Phys. Rev. D 76, 087301 (2007) [4 pages]

Correlation between galactic HI and the cosmic microwave background

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Kate Land1 and Anže Slosar1,2
1Astrophysics, Denys Wilkinson Building, University of Oxford, Keble Road, OX3RH1, Oxford, United Kingdom
2Faculty of Mathematics and Physics, University of Ljubljana, Slovenia

Received 13 June 2007; revised 9 August 2007; published 17 October 2007

We revisit the issue of a correlation between the atomic hydrogen gas in our local galaxy and the cosmic microwave background, a detection of which has been claimed in some literature. We cross correlate the 21-cm emission of galactic atomic hydrogen as traced by the Leiden/Argentine/Bonn Galactic Hi survey with the 3-year cosmic microwave background data from the Wilkinson microwave anisotropy probe. We consider a number of angular scales, masks, and Hi velocity slices and find no statistically significant correlation.

© 2007 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevD.76.087301
DOI:
10.1103/PhysRevD.76.087301
PACS:
98.70.Vc, 98.80.−k, 98.80.Es