The XMM-LSS Survey: Mapping hot, luminous, obscured and dark material out to z~1-2
| dc.creator | Pierre, Marguerite | |
| dc.date | 2001-11-13 | |
| dc.date.accessioned | 2026-07-07T02:01:20Z | |
| dc.date.available | 2026-07-07T02:01:20Z | |
| dc.description | We review the unique cosmological implications of the XMM-LSS survey in association with its multi-WL follow-up: (1) Large Scale Structures traced by X-ray clusters and AGNs, optical galaxies, weak lensing as well as Sunyaev-Zel'dovich effect; (2) location of IR star forming galaxies and IR (obscured) AGNs within the cosmic web. The XMM/MegaCam/VIRMOS/SIRTF data base will provide the first comprehensive study of structure formation - from hundreds of Mpc to galaxy scale - in close connection with environmental processes. | |
| dc.description | 5 pages, 1 figure, Proceedings of the Conference "Where is the matter?" Marseille, June 2001 | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0111242 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0111242 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/3710 | |
| dc.subject | Astrophysics | |
| dc.title | The XMM-LSS Survey: Mapping hot, luminous, obscured and dark material out to z~1-2 | |
| dc.type | text |