Sunyaev-Zel'dovich cluster surveys using a large beam
| dc.creator | Battye, Richard A. | |
| dc.creator | Weller, Jochen | |
| dc.date | 2003-05-23 | |
| dc.date.accessioned | 2026-07-07T02:08:35Z | |
| dc.date.available | 2026-07-07T02:08:35Z | |
| dc.description | Sunyaev Zel'dovich cluster surveys can be used to constrain cosmological parameters. Extracting clusters from the primary anisotropies and the unresolved background from very faint clusters is simple when the telescope beam size is small (1 arcmin), but could be difficult if the beam is larger (8 arcmin). By reference to examples, we show that this is possible by carefully designing the depth of the survey. | |
| dc.description | 4 pages, 1 figure XVIIIth IAP Colloquium, "On the nature of dark energy", 1-5 July 2002, Paris, France | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0305465 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0305465 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/6107 | |
| dc.subject | Astrophysics | |
| dc.title | Sunyaev-Zel'dovich cluster surveys using a large beam | |
| dc.type | text |