A Hard Medium Survey with the ASCA GIS: the (2-10 keV) Number Counts Relationship

Abstract

In this paper we report the first results on a medium survey program conducted in the 2-10 keV energy band using data from the GIS2 instrument onboard the ASCA satellite. We have selected from the ASCA public archive (as of February 14, 1996) 87 images which are suitable for this project. 60 serendipitous X-ray sources, with a snr greater than 3.5, were found. The 2-10 keV flux of the detected sources ranges from 1.1e-13 erg/cm2/s to 4.1e-12 erg/cm2/s. Using this sample we have extended the description of the 2-10 keV LogN(>S)-LogS to a flux limit of ~6.3e-14 erg/cm2/s (the faintest detectable flux), i.e. about 2.7 orders of magnitude fainter than the Piccinotti et al. (1982) determination. The derived number-flux relationship is well described by a power law model, N(>S) = K S^{-a}, with best fit values a = 1.67 +- 0.18 and K = 2.85e-21 1/deg2. At the flux limit of the survey about 27% of the Cosmic X-ray Background in the 2-10 keV energy band is resolved in discrete sources. A flattening of the number-flux relationship, within a factor of 10 from the flux limit of the present survey, is expected in order to avoid saturation. The implications of these results on the models for the origin of the hard X-ray background are briefly discussed.