| 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 |