activity
19962005
most citedRelativistic spectral features from X-ray illuminated spots and the measure of the black hole mass in AGN

80 citations · 165 across the 5 of their papers we have counts for

collaborators

28 papers

astro-ph200519 cited

The relativistic shift of narrow spectral features from black-hole accretion discs

T. Pechacek, M. Dovciak, V. Karas +1

Transient spectral features have been discovered in the X-ray spectra of Active Galactic Nuclei, mostly in the 5--7 keV energy range. Several interpretations were proposed for the…

astro-ph20051 cited

Polarization signatures of strong gravity in black-hole accretion discs

V. Karas, M. Dovciak, G. Matt

We discuss the effects of strong gravity on the polarization properties of a black hole accretion disc. The intrinsic polarization is computed taking into account light scattered o…

astro-ph200464 cited

Polarization signatures of strong gravity in AGN accretion discs

M. Dovciak, V. Karas, G. Matt

The effects of strong gravity on the polarization of the Compton reflection from an X-ray illuminated accretion disc are studied. The gravitational field of a rotating black hole i…

astro-ph200480 cited

Relativistic spectral features from X-ray illuminated spots and the measure of the black hole mass in AGN

M. Dovciak, S. Bianchi, M. Guainazzi +2

Narrow spectral features in the 5--6 keV range were recently discovered in the X-ray spectra of a few active galactic nuclei. We discuss the possibility that these features are due…

astro-ph20031 cited

The HELLAS2XMM 1dF survey: on the nature of high X-ray to optical flux ratio sources

F. Fiore, M. Brusa, F. Cocchia +12

We present results from the photometric and spectroscopic identification of 122 X-ray sources discovered by XMM-Newton in the 2-10 keV band (the HELLAS2XMM 1dF sample). One of the…

astro-ph2002

On the nature of X-ray Bright Optically Normal galaxies

A. Comastri, M. Brusa, P. Ciliegi +10

Multiwavelength observations of the hard X-ray selected sources by Chandra and XMM-Newton surveys have significantly improved our knowledge of the objects responsible of the hard X…