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Searching for absorbed AGN in the 2XMM-Newton pre-release EPIC Serendipitous Source Catalogue

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journal contribution
posted on 2012-10-24, 09:06 authored by E. 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.

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Citation

Astronomy & Astrophysics, 2007, 465 (3), pp. 759-764

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  • VoR (Version of Record)

Published in

Astronomy & Astrophysics

Publisher

EDP Sciences for European Southern Observatory (ESO)

issn

0004-6361

eissn

1432-0746

Copyright date

2007

Available date

2012-10-24

Publisher version

http://www.aanda.org/articles/aa/abs/2007/15/aa6571-06/aa6571-06.html

Language

en

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