X-ray Cluster Large Scale Structure and Cosmology

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dc.creatorPierre, Marguerite
dc.date2003-11-19
dc.date.accessioned2026-07-07T02:11:16Z
dc.date.available2026-07-07T02:11:16Z
dc.descriptionWe outline 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.
dc.description8 pages, 3 figures
dc.identifierhttps://arxiv.org/abs/astro-ph/0311451
dc.identifierhttp://arxiv.org/abs/astro-ph/0311451
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/7022
dc.subjectAstrophysics
dc.titleX-ray Cluster Large Scale Structure and Cosmology
dc.typetext

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