XMM-Newton serendipitous survey. IV (Barcons+, 2007)

Details XMM-Newton serendipitous survey. IV (Barcons+, 2007) XMM-Newton serendipitous survey. IV (Barcons+, 2007)

Nov 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007ycat..34761191b&link_type=abstract

VizieR On-line Data Catalog: J/A+A/476/1191. Originally published in: 2007A&A...476.1191B

Computer Science

Scientific paper

X-ray sources at intermediate fluxes (a few x10-14erg/cm a sky density of ~100deg-2 are responsible for a significant fraction of the cosmic X-ray background at various energies below 10keV. The aim of this paper is to provide an unbiased and quantitative description of the X-ray source population at these fluxes and in various X-ray energy bands.
We present the XMM-Newton Medium sensitivity Survey (XMS), including a total of 318 X-ray sources found among the serendipitous content of 25 XMM-Newton target fields. The XMS comprises four largely overlapping source samples selected at soft (0.5-2keV), intermediate (0.5-4.5keV), hard (2-10keV) and ultra-hard (4.5-7.5keV) bands, the first three of them being flux-limited.
(2 data files).

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