We present the largest sample to date of spectroscopically confirmed x-ray luminous high-redshift galaxy clusters comprising 22 systems in the range 0.9 as part of the XMM-Newton Distant Cluster Project (XDCP). All systems were initially selected as extended x-ray sources over 76.1 deg2 of non-contiguous deep archival XMM-Newton coverage, of which 49.4 deg2 are part of the core survey with a quantifiable selection function and 17.7 deg2 are classified as ‘gold’ coverage as the starting point for upcoming cosmological applications.

The x-ray luminous galaxy cluster population at 0.9
ROSATI, Piero;
2011

Abstract

We present the largest sample to date of spectroscopically confirmed x-ray luminous high-redshift galaxy clusters comprising 22 systems in the range 0.9 as part of the XMM-Newton Distant Cluster Project (XDCP). All systems were initially selected as extended x-ray sources over 76.1 deg2 of non-contiguous deep archival XMM-Newton coverage, of which 49.4 deg2 are part of the core survey with a quantifiable selection function and 17.7 deg2 are classified as ‘gold’ coverage as the starting point for upcoming cosmological applications.

2011
R., Fassbender; H., Böhringer; A., Nastasi; R., Šuhada; M., Mühlegger; A., de Hoon; J., Kohnert; G., Lamer; J. J., Mohr; D., Pierini; G. W., Pratt; H., Quintana; Rosati, Piero; J. S., Santos; A. D., Schwope
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11392/1892947
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