Galaxy groups and low mass clusters at z<0.6: A perspective from the XMM Large Scale Structure survey

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dc.creatorWillis, J. P.
dc.creatorPacaud, F.
dc.creatorPierre, M.
dc.date2006-10-26
dc.date.accessioned2026-07-07T07:27:10Z
dc.date.available2026-07-07T07:27:10Z
dc.descriptionGalaxy groups and low-mass clusters provide important laboratories in which to study X-ray gas physics and the interplay between galaxy evolution and environmental effects. The X-ray Multi-Mirror (XMM) Large Scale Structure (LSS) survey has currently imaged 5 deg2 to a nominal extended source flux limit of order 10e-14 ergs/s/cm2 and is dominated numerically by low-mass groups and clusters at redshifts 0.2 < z < 0.6. We discuss the generation of the XMM-LSS cluster sample, initial results on the physics of groups and low-mass clusters and the prospects for detailed follow-up studies of these systems.
dc.descriptionTo appear in the Proceedings of the XLIst Rencontres de Moriond, XXVIth Astrophysics Moriond Meeting: "From dark halos to light", Eds. L.Tresse, S. Maurogordato and J. Tran Thanh Van (Editions Frontieres)
dc.identifierhttps://arxiv.org/abs/astro-ph/0610800
dc.identifierhttp://arxiv.org/abs/astro-ph/0610800
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/117283
dc.subjectAstrophysics
dc.titleGalaxy groups and low mass clusters at z<0.6: A perspective from the XMM Large Scale Structure survey
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