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| HAL : in2p3-00285093, version 1 |
| arXiv : 0805.4361 |
| Code Bibliographique ADS : 2008arXiv0805.4361C |
| Fiche détaillée |  Récupérer au format |
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| XXXXIIIrd Rencontres de Moriond, La Thuile : Italie (2008) |
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| An SZ/X-ray galaxy cluster model and the X-ray follow-up of the Planck clusters |
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| A. Chamballu1J.G. Bartlett1J.-B. Melin2M. Arnaud3 |
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| (05/2008) |
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| 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. |
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| 1 : | APC - AstroParticule et Cosmologie |
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| 2 : | CEA, DSM, SPP |
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| 3 : | DEA, DSM, SAp |
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| APC - Cosmologie et Gravitation |
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| Thème(s) | : | Physique/Astrophysique/Cosmologie et astrophysique extra-galactique Planète et Univers/Astrophysique/Cosmologie et astrophysique extra-galactique |
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| Astrophysics |
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| Lien vers le texte intégral : |
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| http://fr.arXiv.org/abs/0805.4361 |
| in2p3-00285093, version 1 | |
| http://hal.in2p3.fr/in2p3-00285093 | |
| oai:hal.in2p3.fr:in2p3-00285093 | |
| Contributeur : Simone Lantz | |
| Soumis le : Mercredi 4 Juin 2008, 16:08:03 | |
| Dernière modification le : Dimanche 24 Juin 2012, 12:39:51 | |
