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2XMM J083026+524133: the most X-ray luminous cluster at redshift 1

2XMM J083026+524133: the most X-ray luminous cluster at redshift 1

Publication date: 26 August 2008

Authors: Lamer, G. et al.

Journal: Astronomy & Astrophysics
Volume: 487
Issue: 2
Page: L33-L36
Year: 2008

Copyright: ESO

Aims. In the distant universe X-ray luminous clusters of galaxies are rare objects. Large area surveys are therefore needed to probe the high luminosity end of the cluster population at redshifts z>~1.
Methods. We correlated extended X-ray sources from the second XMM-Newton source catalogue (2XMM) with the SDSS in order to identify new clusters of galaxies. Distant cluster candidates in empty SDSS fields were imaged in the r- and z-bands with the Large Binocular Telescope. We extracted the X-ray spectra of the cluster candidates and fitted thermal plasma models to the data.
Results. We determined the redshift 0.99 ± 0.03 for 2XMM J083026.2+524133 from its X-ray spectrum. With a bolometric luminosity of 1.8 × 1045 erg s-1 this is the most X-ray luminous cluster at redshifts z>1. We measured a gas temperature of 8.2 ± 0.9 keV and estimate a cluster mass M500 = 5.6 × 1014 MSun. The optical imaging revealed a rich cluster of galaxies.

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