An SZ/X-ray galaxy cluster model and the X-ray follow-up of the Planck clusters

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dc.creatorChamballu, A.
dc.creatorBartlett, J. G.
dc.creatorMelin, J. -B.
dc.creatorArnaud, M.
dc.date2008-05-28
dc.date.accessioned2026-07-07T09:41:22Z
dc.date.available2026-07-07T09:41:22Z
dc.descriptionSunyaev-Zel'dovich (SZ) cluster surveys will become an important cosmological tool over next few years, and it will be essential to relate these new surveys to cluster surveys in other wavebands. We present an empirical model of cluster SZ and X-ray observables constructed to address this question and to motivate, dimension and guide X-ray follow-up of SZ surveys. As an example application of the model, we discuss potential XMM-Newton follow-up of Planck clusters.
dc.description4 pages, 5 figures. To appear in the proceedings of the XXXXIIIrd Rencontres de Moriond
dc.identifierhttps://arxiv.org/abs/0805.4361
dc.identifierhttp://arxiv.org/abs/0805.4361
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/161803
dc.subjectAstrophysics
dc.titleAn SZ/X-ray galaxy cluster model and the X-ray follow-up of the Planck clusters
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