期刊
ASTRONOMISCHE NACHRICHTEN
卷 329, 期 2, 页码 147-150出版社
WILEY-V C H VERLAG GMBH
DOI: 10.1002/asna.200710900
关键词
cosmological parameters; galaxies : clusters : general; X-rays : galaxies : clusters
The Planck Satellite will survey the entire sky in 9 millimeter/submillimeter bands and detect thousands of galaxy clusters via their thermal Sunyaev-Zel'dovich (SZ) effect. The unprecedented volume of the survey will permit the construction of a unique catalog of massive clusters out to redshifts of order unity. We describe the expected contents of this catalog and use an empirical model of the intra-cluster gas to predict the X-ray proper-ties of Planck SZ clusters. Using this information we show how a similar to 10 Ms follow-up program on XMM-Newton could increase by similar to 100-fold the number of clusters with measured temperatures in the redshift range z = 0.5-1. Such a large sample of well-studied massive clusters at these redshifts would be a powerful cosmological tool and a significant legacy for XMM-Newton. (C) 2008 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim.
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