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 |
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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 |