Cosmic microwave background radiation anisotropies and data analysis

Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/4895

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DC Field	Value	Language
dc.contributor.author	Sethi, S.K.	-
dc.date.accessioned	2012-07-14T09:02:20Z	-
dc.date.available	2012-07-14T09:02:20Z	-
dc.date.issued	1999-12	-
dc.identifier.citation	Pramana, 1999, Vol.53, p951	en
dc.identifier.issn	0304-4289	-
dc.identifier.issn	0973-7111(online)	-
dc.identifier.uri	http://hdl.handle.net/2289/4895	-
dc.description	Open Access	en
dc.description.abstract	The theory of generation of CMBR temperature and polarization fluctuations is briefly reviewed. Also discussed is the present status of observations and the nature of future surveys.	en
dc.language.iso	en	en
dc.publisher	Indian Academy of Sciences, Bangalore, India	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1999Prama..53..951S	en
dc.relation.uri	http://dx.doi.org/10.1007/s12043-999-0050-7	en
dc.rights	1999 Indian Academy of Sciences	en
dc.subject	CMBR	en
dc.subject	large scale structure	en
dc.subject	cosmology	en
dc.title	Cosmic microwave background radiation anisotropies and data analysis	en
dc.type	Article	en
Appears in Collections:	Research Papers (A&A)

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