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INCREASING EVIDENCE FOR HEMISPHERICAL POWER ASYMMETRY IN THE FIVE-YEARWMAPDATA
- 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
- Subjects :
- Physics
Cosmology and Nongalactic Astrophysics (astro-ph.CO)
Random field
Degree (graph theory)
Cosmic microwave background
Isotropy
FOS: Physical sciences
Astronomy and Astrophysics
Astrophysics::Cosmology and Extragalactic Astrophysics
Astrophysics
CMB cold spot
Dipole
Amplitude
Distribution (mathematics)
Space and Planetary Science
Astrophysics - Cosmology and Nongalactic Astrophysics
Subjects
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