posted on 2012-10-24, 09:06authored byE. Memola, A. Caccianiga, F. Cocchia, Della Ceca R, T. Maccacaro, P. Severgnini, D. J. Fyfe, S. Mateos, M. G. Watson, G. Lamer
Aims.We aim to test a method of efficiently selecting X-ray obscured AGN in the 2XMM-Newton EPIC Serendipitous Source Catalogue.
Methods.By means of a strong correlation established using the XMM-Newton Hard Bright Sample between the intrinsic absorption and the hardness ratio to the 0.5-2.0 keV and 2.0-4.5 keV bands, an efficient way of selecting absorbed sources has been worked out. A hardness ratio selection based on the 2XMM-Newton pre-release Source Catalogue led us to the definition of candidates likely to be obscured in X-rays.
Results.X-ray and optical spectral analysis were performed for three objects. Strong absorption ($N_{\rm H} > 10^{22}$ cm-2) was detected from the X-ray analysis, confirming the efficiency of the method used to select obscured sources. The presence of absorption is also revealed in the optical band, although at a significantly lower level than inferred from the X-ray band.
History
Citation
Astronomy & Astrophysics, 2007, 465 (3), pp. 759-764
Version
VoR (Version of Record)
Published in
Astronomy & Astrophysics
Publisher
EDP Sciences for European Southern Observatory (ESO)