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19 April 2024
 
  » arxiv » astro-ph/0407027

 Article overview


Bayesian Power Spectrum Analysis of the First-Year WMAP data
I.J. O’Dwyer ; H.K. Eriksen ; B.D. Wandelt ; J.B. Jewell ; D.L. Larson ; K. M. Gorski ; A.J. Banday ; S. Levin ; P.B. Lilje ;
Date 1 Jul 2004
Journal Astrophys.J. 617 (2004) L99-102
Subject astro-ph
AbstractWe present the first results from a Bayesian analysis of the WMAP first year data using a Gibbs sampling technique. Using two independent, parallel supercomputer codes we analyze the WMAP Q, V and W bands. The analysis results in a full probabilistic description of the information the WMAP data set contains about the power spectrum and the all-sky map of the cosmic microwave background anisotropies. We present the complete probability distributions for each C_l including any non-Gaussianities of the power spectrum likelihood. While we find good overall agreement with the previously published WMAP spectrum, our analysis uncovers discrepancies in the power spectrum estimates at low l multipoles. For example we claim the best-fit Lambda-CDM model is consistent with the C_2 inferred from our combined Q+V+W analysis with a 10% probability of an even larger theoretical C_2. Based on our exact analysis we can therefore attribute the "low quadrupole issue" to a statistical fluctuation.
Source arXiv, astro-ph/0407027
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