activity
20142026
most citedObscuration-dependent evolution of Active Galactic Nuclei

306 citations · 1.3k across the 23 of their papers we have counts for

collaborators
Showing 2016Show all

6 papers · 1 filter

astro-ph.HE201666 cited

The NuSTAR Serendipitous Survey: The 40 month Catalog and the Properties of the Distant High Energy X-ray Source Population

G. B. Lansbury, D. Stern, J. Aird +35

We present the first full catalog and science results for the NuSTAR serendipitous survey. The catalog incorporates data taken during the first 40 months of NuSTAR operation, which…

astro-ph.GA201628 cited

IC 3639 - A new bona fide Compton thick AGN unveiled by NuSTAR

Peter G. Boorman, P. Gandhi, D. Alexander +19

We analyse high-quality NuSTAR observations of the local (z = 0.011) Seyfert 2 active galactic nucleus (AGN) IC 3639, in conjunction with archival Suzaku and Chandra data. This pro…

astro-ph.HE201681 cited

Spectral Changes in the Hyperluminous Pulsar in NGC 5907 as a Function of Super-Orbital Phase

F. Fuerst, D. J. Walton, D. Stern +5

We present broad-band, multi-epoch X-ray spectroscopy of the pulsating ultra-luminous X-ray source (ULX) in NGC 5907. Simultaneous XMM-Newton and NuSTAR data from 2014 are best des…

astro-ph.HE201672 cited

NuSTAR observations of WISE J1036+0449, a Galaxy at z obscured by hot dust

C. Ricci, R. J. Assef, D. Stern +34

Hot, Dust-Obscured Galaxies (Hot DOGs), selected from the WISE all sky infrared survey, host some of the most powerful Active Galactic Nuclei (AGN) known, and might represent an im…

astro-ph.HE201675 cited

A 78 Day X-ray Period Detected from NGC 5907 ULX1 by Swift

D. J. Walton, F. Fuerst, M. Bachetti +12

We report the detection of a day period in the X-ray lightcurve of the extreme ultraluminous X-ray source NGC 5907 ULX1 ( erg s$^{-1…

astro-ph.HE201637 cited

A growth-rate indicator for Compton-thick active galactic nuclei

M. Brightman, A. Masini, D. R. Ballantyne +10

Due to their heavily obscured central engines, the growth rate of Compton-thick (CT) active galactic nuclei (AGN) is difficult to measure. A statistically significant correlation b…