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dc.contributor.authorKumar Samal, Pramoda
dc.contributor.authorSaha, Rajib
dc.contributor.authorJain, Pankaj
dc.contributor.authorRalston, John P.
dc.date.accessioned2023-07-31T16:53:28Z
dc.date.available2023-07-31T16:53:28Z
dc.date.issued2009-06-03
dc.identifier.citationPramoda 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.urihttps://hdl.handle.net/1808/34674
dc.descriptionThis 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.abstractRecently, 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.publisherOxford University Pressen_US
dc.rights© 2008 The Authors. Journal compilation © 2009 RAS.en_US
dc.subjectMethods: data analysisen_US
dc.subjectCosmic microwave backgrounden_US
dc.subjectCosmology: miscellaneousen_US
dc.titleSignals of statistical anisotropy in WMAP foreground-cleaned mapsen_US
dc.typeArticleen_US
kusw.kuauthorRalston, John P.
kusw.kudepartmentPhysics & Astronomyen_US
dc.identifier.doi10.1111/j.1365-2966.2009.14728.xen_US
kusw.oaversionScholarly/refereed, publisher versionen_US
kusw.oapolicyThis item meets KU Open Access policy criteria.en_US
dc.rights.accessrightsopenAccessen_US


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