SZ surveys with the Arcminute MicroKelvin Imager
| dc.creator | Jones, Michael E. | |
| dc.date | 2001-09-20 | |
| dc.date.accessioned | 2026-07-07T02:00:07Z | |
| dc.date.available | 2026-07-07T02:00:07Z | |
| dc.description | The Arcminute MicroKelvin Imager (AMI) is an instrument currently under construction in Cambridge designed to produce a survey of galaxy clusters via the Sunyaev-Zel'dovich effect. It consists of two interferometric arrays, both operating at 12-18 GHz; one of ten 3.7-m antennas to provide good temperature sensitivity to arcminute-scale structures, and one of eight 13-m antennas (the present Ryle Telescope) to provide flux sensitivity for removing contaminating radio sources. The telescope is due to be observing by 2003, and will produce a public survey of galaxy clusters, as well as being available to guest observers. | |
| dc.description | To appear in 8th Taipei Astrophysics Workshop `AMiBA 2001' | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0109351 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0109351 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/3359 | |
| dc.subject | Astrophysics | |
| dc.title | SZ surveys with the Arcminute MicroKelvin Imager | |
| dc.type | text |