Constraining cosmological parameters through Sunyaev-Zel'dovich  surveys

Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/1044

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DC Field	Value	Language
dc.contributor.author	Majumdar, Subhabrata	-
dc.contributor.author	Subrahmanyan, Ravi	-
dc.date.accessioned	2006-01-03T04:05:13Z	-
dc.date.available	2006-01-03T04:05:13Z	-
dc.date.issued	1999-12	-
dc.identifier.citation	Pramana, 1999, Vol. 53, p971-975.	en
dc.identifier.issn	0304-4289	-
dc.identifier.uri	http://hdl.handle.net/2289/1044	-
dc.description.abstract	For cold dark matter models, images of temperature fluctuations in the cosmic microwave background (CMB), due to Sunyaev Zel¢dovich (SZ) effect have been been simulated taking a cosmolgical distribution of clusters into account. All the models are normalised to the 4-year COBE data. The image statistics are compared with the ATCA limits on arcmin scale anisotropy. The comparison appears to favour low-W0 open universe models.	en
dc.format.extent	334453 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	en
dc.publisher	Indian Academy of Sciences, Bangalore, India.	en
dc.rights	Indian Academy of Sciences, Bangalore, India.	en
dc.subject	Cosmic microwave background	en
dc.subject	Clusters	en
dc.subject	Cosmology theory	en
dc.subject	Cosmology observations	en
dc.title	Constraining cosmological parameters through Sunyaev-Zel'dovich surveys	en
dc.type	Article	en
Appears in Collections:	Research Papers (A&A)

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