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Uspekhi Fizicheskikh Nauk, 2012, Volume 182, Number 11, Pages 1177–1193
DOI: https://doi.org/10.3367/UFNr.0182.201211d.1177 (Mi ufn4106) 		 
This article is cited in 11 scientific papers (total in 11 papers)

PHYSICS OF OUR DAYS

Searching for non-Gaussianity in observational cosmic microwave background data

O. V. Verkhodanov

Special Astrophysical Observatory, Russian Academy of Sciences
Full-text PDF (4458 kB) Citations (11)
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DOI: https://doi.org/10.3367/UFNr.0182.201211d.1177
Abstract: Methods for searching for non-Gaussianity in the WMAP data are reviewed and the associated problems related to the cosmic microwave background (CMB) data analysis are discussed. Evidence for non-Gaussianity has been obtained by various methods and from a number of multipole ranges. Different approaches to searching for non-Gaussian CMB data are sensitive to different manifestations of non-Gaussianity, which sometimes are due to the primordial non-Gaussianity and sometimes to galactic foregrounds and/or systematic residuals remaining after the data analysis that are difficult to take into account.
Received: July 13, 2011
Revised: December 1, 2011
Accepted: December 6, 2011
English version:
Physics–Uspekhi, 2012, Volume 55, Issue 11, Pages 1098–1114
DOI: https://doi.org/10.3367/UFNe.0182.201211d.1177
Bibliographic databases:
Document Type: Article
PACS: 95.75.-z, 98.70.Vc, 98.80.-k
Language: Russian
Citation: O. V. Verkhodanov, “Searching for non-Gaussianity in observational cosmic microwave background data”, UFN, 182:11 (2012), 1177–1193; Phys. Usp., 55:11 (2012), 1098–1114
Citation in format AMSBIB
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    • This publication is cited in the following 11 articles:
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