EDP Sciences
Free Access
Volume 432, Number 2, March III 2005
Page(s) 395 - 400
Section Cosmology (including clusters of galaxies)
DOI https://doi.org/10.1051/0004-6361:20041977

A&A 432, 395-400 (2005)
DOI: 10.1051/0004-6361:20041977

XMM-Newton observations of the Lockman Hole

III. A relativistic Fe line in the mean X-ray spectra of type-1 and type-2 AGN
A. Streblyanska1, G. Hasinger1, A. Finoguenov1, X. Barcons2, S. Mateos2 and A. C. Fabian3

1  Max-Planck-Institut für Extraterrestrische Physik, Giessenbachstraße, 85740 Garching, Germany
    e-mail: alina@mpe.mpg.de
2  Instituto de Física de Cantabria (CSIC-UC), 39005 Santander, Spain
3  Institute of Astronomy, Madingley Road, Cambridge CB3 0HA, USA

(Received 9 September 2004 / Accepted 17 November 2004)

Using the 770 ks XMM-Newton survey of the Lockman Hole field in combination with extensive optical identifications of the AGN population, we derive an average rest-frame spectrum of AGN types-1 and 2. The most prominent feature in the averaged spectrum is a strong fluorescent Fe line. In both type-1 and type-2 AGN, a clear relativistic line profile is revealed. A laor line profile with an inner disk radius smaller than the last stable orbit of a Schwarzschild black hole is most consistent with the data, indicating that the average supermassive black hole has significant spin. Equivalent widths of the broad relativistic lines range between 400-600 eV. We used the disk reflection model to compare the observed strength of the line with the amplitude of the reflection component, concluding that to consistently describe the observations the average iron abundance should be about three times the solar value.

Key words: galaxies: active -- galaxies: quasars: general -- X-rays: general -- X-rays: diffuse background

SIMBAD Objects

© ESO 2005

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