Astrophys. J., 596, 944-956 (2003/October-3)
The Serendipitous Extragalactic X-ray Source Identification program. I. Characteristics of the hard X-ray sample.
HARRISON F.A., ECKART M.E., MAO P.H., HELFAND D.J. and STERN D.
Abstract (from CDS):
The Serendipitous Extragalactic X-Ray Source Identification (SEXSI) program is designed to extend greatly the sample of identified extragalactic hard X-ray (2-10 keV) sources at intermediate fluxes (∼10–13 to 10–15 ergs/cm2/s). SEXSI, which studies sources selected from more than 2 deg2, provides an essential complement to the Chandra Deep Fields, which reach depths of 5x10–16 ergs/cm2/s (2-10 keV) but over a total area of less than 0.2 deg2. In this paper we describe the characteristics of the survey and our X-ray data analysis methodology. We present the cumulative flux distribution for the X-ray sample of 1034 hard sources and discuss the distribution of spectral hardness ratios. Our logN-logS in this intermediate flux range connects to those found in the Deep Fields, and by combining the data sets, we constrain the hard X-ray population over the flux range in which the differential number counts change slope and from which the bulk of the 2-10 keV X-ray background arises. We further investigate the logN-logS distribution separately for soft and hard sources in our sample, finding that while a clear change in slope is seen for the softer sample, the hardest sources are well described by a single power law down to the faintest fluxes, consistent with the notion that they lie at lower average redshift.
Catalogs - Surveys - X-Rays: Galaxies - X-Rays: General
VizieR on-line data:
<Available at CDS (J/ApJ/596/944): table2.dat table4.dat table6.dat>
Tables 4, 6: CXOSEXSI JHHMMSS.s+DDMMSS N=1034+879.
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