XMMU J100111.1+015330 , the SIMBAD biblio

The COSMOS survey is a multiwavelength survey aimed to study the evolution of galaxies, AGN and large scale structures. Within this survey XMM-COSMOS a powerful tool to detect AGN and galaxy clusters. The XMM-COSMOS is a deep X-ray survey over the full 2deg² of the COSMOS area. It consists of 55 XMM-Newton pointings for a total exposure of ∼1.5Ms with an average vignetting-corrected depth of 40 ks across the field of view and a sky coverage of 2.13deg². We present the catalogue of point-like X-ray sources detected with the EPIC CCD cameras, the logN - logS relations and the X-ray colour-colour diagrams. The analysis was performed using the XMM-SAS data analysis package in the 0.5-2keV, 2-10keV and 5-10keV energy bands. Source detection has been performed using a maximum likelihood technique especially designed for raster scan surveys. The completeness of the catalogue as well as logN -logS and source density maps have been calibrated using Monte Carlo simulations. The catalogs contains a total of 1887 unique sources detected in at least one band with likelihood parameter det_ml>10. The survey, which shows unprecedented homogeneity, has a flux limit of ∼1.7x10^–15erg/cm2/s, ∼9.3x10^–15erg/cm2/s and ∼1.3x10^–14erg/cm2/s over 90% of the area (1.92deg²) in the 0.5-2keV, 2-10keV and 5-10keV energy band, respectively. Thanks to the rather homogeneous exposure over a large area, the derived logN - logS relations are very well determined over the flux range sampled by XMM-COSMOS. These relations have been compared with XRB synthesis models, which reproduce the observations with an agreement of ∼10% in the 5-10keV and 2-10keV band, while in the 0.5-2keV band the agreement is of the order of ∼20%. The hard X-ray colors confirmed that the majority of the extragalactic sources in a bright subsample are actually type I or type II AGN. About 20% of the sources have a X-ray luminosity typical of AGN (L_X>10⁴²erg/s) although they do not show any clear signature of nuclear activity in the optical spectrum.