activity
19952023
most citedThe Nuclear Spectroscopic Telescope Array (NuSTAR) Mission

2.3k citations · 41.1k across the 542 of their papers we have counts for

collaborators
Showing 2007 · astro-phShow all

13 papers · 2 filters

astro-ph2007★ 167 cited

The effect of radiation pressure on dusty absorbing gas around AGN

A. C. Fabian, R. V. Vasudevan, P. Gandhi

Many Active Galactic Nuclei (AGN) are surrounded by gas which absorbs the radiation produced by accretion onto the central black hole and obscures the nucleus from direct view. The…

astro-ph2007★ 205 cited

Broad iron K-alpha emission lines as a diagnostic of black hole spin

Christopher S. Reynolds, Andrew C. Fabian

We address the ability of broad iron emission lines from black hole accretion disks to diagnose the spin of the black hole. Using a high-resolution 3-dimensional MHD simulation of…

astro-ph2007★ 11 cited

XMM-Newton and Broad Iron Lines

A. C. Fabian

Iron line emission is common in the X-ray spectra of accreting black holes. When the line emission is broad or variable then it is likely to originate from close to the black hole.…

astro-ph2007★ 84 cited

Cool X-ray emitting gas in the core of the Centaurus cluster of galaxies

J. S. Sanders, A. C. Fabian, S. W. Allen +3

We use a deep XMM-Newton Reflection Grating Spectrometer observation to examine the X-ray emission from the core of the Centaurus cluster of galaxies. We clearly detect Fe-XVII emi…

astro-ph2007★ 245 cited

Implications of very rapid TeV variability in blazars

Mitchell C. Begelman, Andrew C. Fabian, Martin J. Rees

We discuss the implications of rapid (few-minute) variability in the TeV flux of blazars, which has been observed recently with the HESS and MAGIC telescopes. The variability times…

astro-ph2007★ 7 cited

Radio Source Heating in the ICM: The Example of Cygnus A

Elena Belsole, Andrew C. Fabian

One of the most promising solutions for the cooling flow problem involves energy injection from the central AGN. However it is still not clear how collimated jets can heat the ICM…

astro-ph2007★ 15 cited

X-ray active galactic nuclei in the core of the Perseus cluster

S. Santra, J. S. Sanders, A. C. Fabian

We present a study of the X-ray emission from the nuclei of galaxies observed in the core of the Perseus cluster in a deep exposure with Chandra. Point sources are found coincident…

astro-ph2007★ 481 cited

Piecing Together the X-ray Background: Bolometric Corrections for Active Galactic Nuclei

R. V. Vasudevan, A. C. Fabian

(Abridged) The X-ray background can be used to constrain the accretion history of Supermassive Black Holes (SMBHs) in Active Galactic Nuclei (AGN). A knowledge of the hard X-ray bo…

astro-ph2007★ 35 cited

Fields and Filaments in the Core of the Centaurus Cluster

G. B. Taylor, A. C. Fabian, G. Gentile +3

We present high resolution images of the Faraday Rotation Measure (RM) structure of the radio galaxy PKS 1246-410, at the center of the Centaurus cluster. Comparison with Halpha-li…

astro-ph2007★ 24 cited

The high energy emission of GRO J1655-40 as revealed with INTEGRAL spectroscopy of the 2005 outburst

M. D. Caballero-Garcia, J. M. Miller, E. Kuulkers +10

We present broadband (3-500 keV) INTEGRAL X-ray spectra and X-ray/optical light curves of the luminous black hole X-ray transient and relativistic jet source GRO J1655-40. Our anal…

astro-ph2007★ 256 cited

A deeper X-ray study of the core of the Perseus galaxy cluster: the power of sound waves and the distribution of metals and cosmic rays

J. S. Sanders, A. C. Fabian

We make a further study of the very deep Chandra observation of the X-ray brightest galaxy cluster, A426 in Perseus. We examine the radial distribution of energy flux inferred by t…

astro-ph2007★ 16 cited

The luminous X-ray hotspot in 4C 74.26: synchrotron or inverse-Compton emission?

M. C. Erlund, A. C. Fabian, Katherine M. Blundell +2

We report the discovery of an X-ray counterpart to the southern radio hotspot of the largest-known radio quasar 4C 74.26 (whose redshift is z=0.104). Both XMM-Newton and Chandra im…

astro-ph2007★ 28 cited

A longer XMM-Newton look at I Zwicky 1: physical conditions and variability of the ionised absorbers

E. Costantini, L. C. Gallo, W. N. Brandt +2

We present a spectral analysis of the narrow-line Seyfert 1 galaxy I Zwicky 1, focusing on the characteristics of the ionised absorbers as observed with XMM-Newton in 2005. The sof…