activity
20042019
most citedMultiwavelength study of massive galaxies at z~2. II. Widespread Compton thick AGN and the concurrent growth of black holes and bulges

346 citations · 4.4k across the 48 of their papers we have counts for

collaborators

48 papers

astro-ph.GA2019★ 40 cited

Hot Dust-Obscured Galaxies with Excess Blue Light

R. J. Assef, M. Brightman, D. J. Walton +10

Hot Dust-Obscured Galaxies (Hot DOGs) are among the most luminous galaxies in the Universe. Powered by highly obscured, possibly Compton-thick, active galactic nuclei (AGNs), Hot D…

astro-ph.GA2018★ 18 cited

SMBH accretion properties of radio-selected AGN out to z~4

I. Delvecchio, V. Smolcic, G. Zamorani +8

Exploring how radio-emitting active galactic nuclei (AGN) behave and evolve with time is critical for understanding how AGN feedback impacts galaxy evolution. In this work, we inve…

astro-ph.HE2018★ 20 cited

A long hard-X-ray look at the dual active galactic nuclei of M51 with NuSTAR

M. Brightman, M. Baloković, M. Koss +14

We present a broadband X-ray spectral analysis of the M51 system, including the dual active galactic nuclei (AGN) and several off-nuclear point sources. Using a deep observation by…

astro-ph.GA2017★ 62 cited

Identifying the subtle signatures of feedback from distant AGN using ALMA observations and the EAGLE hydrodynamical simulations

J. Scholtz, D. M. Alexander, C. M. Harrison +10

We present sensitive 870m continuum measurements from our ALMA programmes of 114 X-ray selected AGN in the CDF-S and COSMOS fields. We use these observations in combination with…

astro-ph.HE2017★ 54 cited

The NuSTAR Serendipitous Survey: Hunting for The Most Extreme Obscured AGN at >10 keV

G. B. Lansbury, D. M. Alexander, J. Aird +27

We identify sources with extremely hard X-ray spectra (i.e., with photon indices of Gamma<0.6 in the 13 sq. deg. NuSTAR serendipitous survey, to search for the most highly obscured…

astro-ph.GA2017★ 40 cited

Galaxy-scale Bars in Late-type Sloan Digital Sky Survey Galaxies Do Not Influence the Average Accretion Rates of Supermassive Black Holes

Andy D. Goulding, Eve Matthaey, Jenny E. Greene +8

Galaxy-scale bars are expected to provide an effective means for driving material towards the central region in spiral galaxies, and possibly feeding supermassive black holes (BHs)…