Bianchi type VIIh models and the WMAP 3-year data
Abstract
Context. A specific example of Bianchi type VIIh models, i.e. those including universal rotation (vorticity) and differential expansion (shear), has been shown in Jaffe et al. (2005, ApJ, 629, L1) to correlate unexpectedly with the WMAP first-year data. 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, ApJ, 643, 616). We use the WMAP 3-year data release, including maps for individual years, and perform additional comparisons to assess the influence of both noise and residual foregrounds and eliminate potential non-cosmological sources for the correlation. Results. We confirm that the signal is detected in both the combined 3-year data and the individual yearly sky maps at a level consistent with our original analysis. The significance of the correlation is not affected by either noise or foreground residuals. Conclusions. The results of our previous study are unchanged.
Additional Information
© ESO 2006. (Received 2 June 2006 / Accepted 13 September 2006) We acknowledge use of the HEALPix software (Górski et al. 2005) and of the Legacy Archive for Microwave Background Data Analysis (LAMBDA). Support for LAMBDA is provided by the NASA Office of Space Science.Attached Files
Published - JAFaanda06.pdf
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Additional details
- Eprint ID
- 12818
- Resolver ID
- CaltechAUTHORS:JAFaanda06
- NASA
- Created
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2008-12-24Created from EPrint's datestamp field
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2021-11-08Created from EPrint's last_modified field