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The XMM-LSS Survey: Mapping hot, luminous, obscured and dark material out to z~1-2

Marguerite Pierre
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Abstract

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.

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Marguerite Pierre. 2001-11-13. The XMM-LSS Survey: Mapping hot, luminous, obscured and dark material out to z~1-2. https://arxiv.org/abs/astro-ph/0111242

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