The XMM-Newton/2dF survey - II. The nature of X-ray - faint optically bright X-ray sources
journal contributionposted on 08.12.2009, 16:24 by A. Georgakakis, I. Georgantopoulos, M. Vallbe, V. Kolokotronis, S. Basilakos, S. M. Plionis, G. C. Stewart, T. Shanks, B. J. Boyle
In this paper we investigate the properties of low X-ray-to-optical flux ratio sources detected in a wide-area (2.5 deg2) shallow [fX(0.5–8 keV) ≈ 10−14 erg s−1 cm−2]XMM–Newton survey. We find a total of 26 sources (5 per cent of the total X-ray-selected population) with log fX/fopt < −0.9 to the above flux limit. Optical spectroscopy is available for 20 of these low X-ray-to-optical flux ratio objects. Most of them are found to be associated with Galactic stars (a total of eight) and broad-line active galactic nuclei (AGNs; a total of eight). We also find two sources with optical spectra showing absorption and/or narrow emission lines and X-ray/optical properties suggesting AGN activity. Another two sources are found to be associated with low-redshift galaxies with narrow emission-line optical spectra, X-ray luminosities LX(0.5–8 keV) ≈ 1041 erg s−1 and log fX/fopt≈−2 suggesting ‘normal’ star-forming galaxies. Despite the small-number statistics the sky density of ‘normal’ X-ray-selected star-forming galaxies at the flux limit of the present sample is low, consistent with previous ROSAT High-Resolution Imager (HRI) deep surveys. Also, the number density estimated here is in good agreement with both the log N–log S of ‘normal’ galaxies in the Chandra Deep Field North (extrapolated to bright fluxes) and model predictions based on the X-ray luminosity function of local star-forming galaxies.