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X-ray Cluster Large Scale Structure and Cosmology
Published online by Cambridge University Press: 23 September 2016
Abstract
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