activity
19952005
most citedThe X-ray spectra of accreting Kerr black holes

26 citations · 27 across the 2 of their papers we have counts for

collaborators

15 papers

astro-ph200526 cited

The X-ray spectra of accreting Kerr black holes

Andrew C. Fabian, Giovanni Miniutti

The relativistic broad iron lines seen in the X-ray spectra of several active galaxies and Galactic black hole systems are reviewed. Most such objects require emission from within…

astro-ph20031 cited

Obscured Active Galactic Nuclei and Obscured Accretion

A. C. Fabian

Most of the local active galactic nucleus (AGN) population is obscured and much of the X-ray background originates in obscured AGNs. The contribution of obscured accretion to the g…

astro-ph2002

Study of X-ray reflection features in a sample of Sy 1s observed by BeppoSAX

A. De Rosa, A. C. Fabian, L. Piro +1

The ionized disc reflection model of Ross & Fabian is applied to a sample of five Seyfert 1 galaxies observed by BeppoSAX. Good fits were obtained for all the objects in the sample…

astro-ph2002

Powerful obscured AGN in Chandra cluster fields

P. Gandhi, A. C. Fabian, C. S. Crawford

Models for the origin of the hard X-ray background have suggested that sources with the most accretion activity lie hidden in highly obscured AGN. We report on our study of hard, s…

astro-ph2001

The Chandra High Energy Transmission Grating Spectrometer probes the dusty warm absorber in the Seyfert 1 galaxy MCG--6-30-15

J. C. Lee, C. R. Canizares, H. L. Marshall +4

The Chandra HETGS spectra of the Seyfert 1 galaxy MCG--6-30-15 show numerous narrow, unresolved (FWHM < 200 km/s) absorption lines from a wide range of ionization states of N, O, M…

astro-ph2001

Multi-wavelength observations of serendipitous Chandra sources

P. Gandhi, C. S. Crawford, A. C. Fabian +4

We describe progress in a programme to study a sample of sources typical of those which contribute a large fraction of the hard X-ray background. The sources are selected from the…