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Context. A specific example of Bianchi Type VIIh models, i.e. those includinguniversal rotation (vorticity) and differential expansion (shear), has beenshown in Jaffe et al. (2005) to correlate unexpectedly with the WMAP first-yeardata. Aims. We re-assess the signature of this model in the WMAP 3-year data.Methods. The cross-correlation methods are described in Jaffe et al. (2006a).We use the WMAP 3-year data release, including maps for individual years, andperform additional comparisons to assess the influence of both noise andresidual foregrounds and eliminate potential non-cosmological sources for thecorrelation. Results. We confirm that the signal is detected in both thecombined 3-year data and the individual yearly sky maps at a level consistentwith our original analysis. The significance of the correlation is not affectedby either noise or foreground residuals. Conclusions. The results of ourprevious study are unchanged.Comment: 5 pages, 4 figures, submitted as A&A Research Not

Bianchi type VIIh models and the WMAP 3-year data

Bianchi type VII_h models and the WMAP 3-year data