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X-ray Cluster Large Scale Structure and Cosmology

Published online by Cambridge University Press:  23 September 2016

Marguerite Pierre
Marguerite Pierre*
Affiliation:
Service d'Astrophysique, CEA Saclay, F-91191 Gif Sur Yvette

Abstract

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We outline the main arguments in favor of cosmological X-ray surveys of galaxy clusters. We summarize recent advances in our understanding of cluster physics. After a short review of past surveys, we present the scientific motivations of the XMM Large Scale Structure survey. We further illustrate how such a survey can help constrain the nature of the dark energy as well as cluster scaling law evolution, i.e. non-gravitational physics.

Type
Session VII: Ongoing and Future Studies
Information
Symposium - International Astronomical Union , Volume 216: Maps of the Cosmos , 2005 , pp. 373 - 380
Copyright
Copyright © Astronomical Society of the Pacific 2005 

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