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Constraining cosmological parameters through Sunyaev-Zel'dovich surveys

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dc.contributor.author Majumdar, S
dc.contributor.author Subrahmanyan, R
dc.date.accessioned 2008-08-22T10:22:38Z
dc.date.available 2008-08-22T10:22:38Z
dc.date.issued 1999-12
dc.identifier.citation Pramana, Vol. 53, No. 6, pp. 971 - 975 en
dc.identifier.issn 0304-4289
dc.identifier.uri http://hdl.handle.net/2248/3249
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 cosmological 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-Ω0 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 en
dc.relation.uri http://adsabs.harvard.edu/abs/1999Prama..53..971M en
dc.subject Cosmic microwave background en
dc.subject Temperature fluctuations en
dc.title Constraining cosmological parameters through Sunyaev-Zel'dovich surveys en
dc.type Article en


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