Hemispherical power asymmetry in the three-year Wilkinson Microwave Anisotropy Probe sky maps

Details Hemispherical power asymmetry in the three-year Wilkinson Microwave Anisotropy Probe sky maps Hemispherical power asymmetry in the three-year Wilkinson Microwave Anisotropy Probe sky maps

2007-01-04

arxiv.org/abs/astro-ph/0701089v2

Astrophys.J.660:L81-L84,2007

Astronomy and Astrophysics

Astrophysics

4 pages, 2 figures, accepted for publication in ApJL

Scientific paper

10.1086/518091

We consider the issue of hemispherical power asymmetry in the three-year WMAP data, adopting a previously introduced modulation framework. Computing both frequentist probabilities and Bayesian evidences, we find that the model consisiting of an isotropic CMB sky modulated by a dipole field, gives a substantially better fit to the observations than the purely isotropic model, even when accounting for the larger prior volume. For the ILC map, the Bayesian log-evidence difference is ~1.8 in favour of the modulated model, and the raw improvement in maximum log-likelihood is 6.1. The best-fit modulation dipole axis points toward (l,b) = (225 deg,-27 deg), and the modulation amplitude is 0.114, in excellent agreement with the results from the first-year analyses. The frequentist probability of obtaining such a high modulation amplitude in an isotropic universe is ~1%. These results are not sensitive to data set or sky cut. Thus, the statistical evidence for a power asymmetry anomaly is both substantial and robust, although not decisive, for the currently available data. Increased sky coverage through better foreground handling and full-sky and high-sensitivity polarization maps may shed further light on this issue.

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