activity
20112026
most citedImproved Reflection Models of Black-Hole Accretion Disks: Treating the Angular Distribution of X-rays

715 citations · 3.7k across the 78 of their papers we have counts for

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Showing 2015Show all

6 papers · 1 filter

astro-ph.HE2015

The Corona of the Broad-Line Radio Galaxy 3C 390.3

Anne Lohfink, Patrick Ogle, Francesco Tombesi +17

We present the results from a joint Suzaku/NuSTAR broad-band spectral analysis of 3C 390.3. The high quality data enables us to clearly separate the primary continuum from the repr…

astro-ph.HE2015

The NuSTAR X-ray spectrum of the low-luminosity AGN in NGC 7213

F. Ursini, A. Marinucci, G. Matt +11

We present an analysis of the 3-79 keV NuSTAR spectrum of the low-luminosity active galactic nucleus NGC 7213. In agreement with past observations, we find a lower limit to the hig…

astro-ph.HE2015★ 31 cited

NuSTAR observations of the powerful radio-galaxy Cygnus A

Christopher S. Reynolds, Anne M. Lohfink, Patrick M. Ogle +17

We present NuSTAR observations of the powerful radio galaxy Cygnus A, focusing on the central absorbed active galactic nucleus (AGN). Cygnus A is embedded in a cool-core galaxy clu…

astro-ph.HE2015★ 141 cited

NuSTAR and Suzaku observations of the hard state in Cygnus X-1: locating the inner accretion disk

M. L. Parker, J. A. Tomsick, J. M. Miller +20

We present simultaneous Nuclear Spectroscopic Telescope Array (NuSTAR ) and Suzaku observations of the X-ray binary Cygnus X-1 in the hard state. This is the first time this state…

astro-ph.HE2015★ 8 cited

Properties of AGN coronae in the NuSTAR era

A. C. Fabian, A. Lohfink, E. Kara +3

The focussing optics of NuSTAR have enabled high signal-to-noise spectra to be obtained from many X-ray bright Active Galactic Nuclei (AGN) and Galactic Black Hole Binaries (BHB).…

astro-ph.HE2015★ 37 cited

The Compton hump and variable blue wing in the extreme low-flux NuSTAR observations of 1H0707-495

E. Kara, A. C. Fabian, A. M. Lohfink +10

The Narrow-line Seyfert I galaxy, 1H0707-495, has been well observed in the 0.3-10 keV band, revealing a dramatic drop in flux in the iron K alpha band, a strong soft excess, and s…