Data

Overview

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>6×10^-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.

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Catalogue Bibcode

2017yCat..74491422M

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References

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

Mateos, S. ; Carrera, F. J. ; Alonso-Herrero, A. ; Rovilos, E. ; Hernan-Caballero, A. ; Barcons, X. ; Blain, A. ; Caccianiga, A. ; Della Ceca, R. ; Severgnini, P.

2015MNRAS.449.1422M

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Parameters

Source name (IAU identification)

IAU identification

Class

Optical spectroscopic classification

logLX

Log of the rest-frame 2-10 keV intrinsic X-ray luminosity (in erg/s)

e_ogLX

The 1σ uncertainty in the luminosity in log units

logLIR

Log of the rest-frame 6 μm AGN luminosity associated with the emission of the nuclear obscurer (the dusty torus) (in erg/s)

e_logLIR

The 1σ uncertainty in the 6 μm luminosity in log units