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Signals of statistical anisotropy in WMAP foreground-cleaned maps
dc.contributor.author | Kumar Samal, Pramoda | |
dc.contributor.author | Saha, Rajib | |
dc.contributor.author | Jain, Pankaj | |
dc.contributor.author | Ralston, John P. | |
dc.date.accessioned | 2023-07-31T16:53:28Z | |
dc.date.available | 2023-07-31T16:53:28Z | |
dc.date.issued | 2009-06-03 | |
dc.identifier.citation | Pramoda Kumar Samal, Rajib Saha, Pankaj Jain, John P. Ralston, Signals of statistical anisotropy in WMAP foreground-cleaned maps, Monthly Notices of the Royal Astronomical Society, Volume 396, Issue 1, June 2009, Pages 511–522, https://doi.org/10.1111/j.1365-2966.2009.14728.x. | en_US |
dc.identifier.uri | https://hdl.handle.net/1808/34674 | |
dc.description | This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society © 2008 The Authors. Journal compilation © 2009 RAS. Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved. | en_US |
dc.description.abstract | Recently, a symmetry-based method to test for statistical isotropy of the cosmic microwave background was developed. We apply the method to template-cleaned 3- and 5-years Wilkinson Microwave Anisotropy Probe-Differencing Assembly maps. We examine a wide range of angular multipoles from 2 < l < 300. The analysis detects statistically significant signals of anisotropy inconsistent with an isotropic cosmic microwave background in some of the foreground-cleaned maps. We are unable to resolve whether the anomalies have a cosmological, local astrophysical or instrumental origin. Assuming the anisotropy arises due to residual foreground contamination, we estimate the residual foreground power in the maps. For the W-band maps, we also find a highly improbable degree of isotropy we cannot explain. We speculate that excess isotropy may be caused by faulty modelling of detector noise. | en_US |
dc.publisher | Oxford University Press | en_US |
dc.rights | © 2008 The Authors. Journal compilation © 2009 RAS. | en_US |
dc.subject | Methods: data analysis | en_US |
dc.subject | Cosmic microwave background | en_US |
dc.subject | Cosmology: miscellaneous | en_US |
dc.title | Signals of statistical anisotropy in WMAP foreground-cleaned maps | en_US |
dc.type | Article | en_US |
kusw.kuauthor | Ralston, John P. | |
kusw.kudepartment | Physics & Astronomy | en_US |
dc.identifier.doi | 10.1111/j.1365-2966.2009.14728.x | en_US |
kusw.oaversion | Scholarly/refereed, publisher version | en_US |
kusw.oapolicy | This item meets KU Open Access policy criteria. | en_US |
dc.rights.accessrights | openAccess | en_US |