The planck cluster survey

被引：12

作者：

Bartlett, J. G. ^{[1
]}

Chamballu, A. ^{[1
]}

Melin, J. -B. ^{[2
]}

Arnaud, M. ^{[3
]}

机构：

[1] Univ Paris 07, Lab Astroparticule & Cosmol APC, F-75205 Paris 13, France

[2] CEA, SPP, Saclay, France

[3] CEA, SAp, Saclay, France

来源：

ASTRONOMISCHE NACHRICHTEN | 2008年 / 329卷 / 02期

关键词：

cosmological parameters; galaxies : clusters : general; X-rays : galaxies : clusters;

D O I：

10.1002/asna.200710900

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

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.

引用

页码：147 / 150

页数：4

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