XMM-Newton Bright Serendipitous Survey (Della Ceca+, 2004)

Details XMM-Newton Bright Serendipitous Survey (Della Ceca+, 2004) XMM-Newton Bright Serendipitous Survey (Della Ceca+, 2004)

Sep 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005ycat..34280383d&link_type=abstract

VizieR On-line Data Catalog: J/A+A/428/383. Originally published in: 2004A&A...428..383D

Computer Science

X-Ray Sources, Surveys

Scientific paper

We present here "The XMM-Newton Bright Serendipitous Survey", composed of two flux-limited samples: the XMM-Newton Bright Source Sample (BSS, hereafter) and the XMM-Newton "Hard" Bright Source Sample (HBSS, hereafter) having a flux limit of fX~7x10-14erg/cm2/s in the 0.5-4.5keV and 4.5-7.5keV energy band, respectively. After discussing the main goals of this project and the survey strategy, we present the basic data on a complete sample of 400 X-ray sources (389 of them belong to the BSS, 67 to the HBSS with 56 X-ray sources in common) derived from the analysis of 237 suitable XMM-Newton fields (211 for the HBSS). At the flux limit of the survey we cover a survey area of 28.10 (25.17 for the HBSS) sq. deg. The extragalactic number-flux relationships (in the 0.5-4.5keV and in the 4.5-7.5keV energy bands) are in good agreement with previous and new results making us confident about the correctness of data selection and analysis.
(5 data files).

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