VizieR Online Data Catalog: 2XMM AGN X-ray and mid-IR luminosities (Mateos+, 2015)

Our AGN sample was drawn from the wide-angle BUXS (Mateos et al. 2012MNRAS.426.3271M). BUXS is a large, complete, flux-limited sample of X-ray bright (f_4.5-10keV>6x10^-14erg/s/cm²) AGN detected with the XMM-Newton observatory at 4.5-10 keV energies. The survey is based on 381 high Galactic latitude (|b|>20°) XMM-Newton observations having good quality for serendipitous source detection that were used to derive extragalactic source count distributions at intermediate X-ray fluxes (Mateos et al. 2008A&A...492...51M). BUXS contains 255 AGN, after removal of Galactic stars and known BL Lacs (<3 per cent), detected over a total sky area of 44.43 deg².

(1 data file).