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XXXXIIIrd Rencontres de Moriond, La Thuile : Italie (2008)
An SZ/X-ray galaxy cluster model and the X-ray follow-up of the Planck clusters
A. Chamballu1, J.G. Bartlett1, J.-B. Melin2, M. Arnaud3
(05/2008)

Sunyaev-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.
1 :  APC - UMR 7164 - AstroParticule et Cosmologie
2 :  CEA, DSM, SPP
3 :  DEA, DSM, SAp
APC - Cosmologie et Gravitation
Physique/Astrophysique/Cosmologie et astrophysique extra-galactique

Planète et Univers/Astrophysique/Cosmologie et astrophysique extra-galactique
Astrophysics
Lien vers le texte intégral : 
http://fr.arXiv.org/abs/0805.4361