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INCREASING EVIDENCE FOR HEMISPHERICAL POWER ASYMMETRY IN THE FIVE-YEARWMAPDATA

Authors :
Krzysztof M. Gorski
A. J. Banday
H. K. Eriksen
F. K. Hansen
J. Hoftuft
P. B. Lilje
Source :
The Astrophysical Journal. 699:985-989
Publication Year :
2009
Publisher :
American Astronomical Society, 2009.

Abstract

(Abridged)Motivated by the recent results of Hansen et al. (2008) concerning a noticeable hemispherical power asymmetry in the WMAP data on small angular scales, we revisit the dipole modulated signal model introduced by Gordon et al. (2005). This model assumes that the true CMB signal consists of a Gaussian isotropic random field modulated by a dipole, and is characterized by an overall modulation amplitude, A, and a preferred direction, p. Previous analyses of this model has been restricted to very low resolution due to computational cost. In this paper, we double the angular resolution, and compute the full corresponding posterior distribution for the 5-year WMAP data. The results from our analysis are the following: The best-fit modulation amplitude for l<br />Comment: 6 pages, 2 figures; added references and minor comments. Accepted for publication in ApJ

Details

ISSN :
15384357 and 0004637X
Volume :
699
Database :
OpenAIRE
Journal :
The Astrophysical Journal
Accession number :
edsair.doi.dedup.....f6797899cb874ecb369f78e22fbaa91c
Full Text :
https://doi.org/10.1088/0004-637x/699/2/985