activity
19982019
most citedA semi-empirical simulation of the extragalactic radio continuum sky for next generation radio telescopes

340 citations · 2.8k across the 54 of their papers we have counts for

collaborators

53 papers

astro-ph.GA2019★ 35 cited

The first spectroscopic dust reverberation programme on active galactic nuclei: the torus in NGC 5548

H. Landt, M. J. Ward, D. Kynoch +16

We have recently initiated the first spectroscopic dust reverberation programme on active galactic nuclei (AGN) in the near-infrared. Spectroscopy enables measurement of dust prope…

astro-ph.GA2016★ 99 cited

Optical Emission Line Nebulae in Galaxy Cluster Cores 1: The Morphological, Kinematic and Spectral Properties of the Sample

S. L. Hamer, A. C. Edge, A. M. Swinbank +9

We present an Integral Field Unit survey of 73 galaxy clusters and groups with the VIsible Multi Object Spectrograph (VIMOS) on VLT. We exploit the data to determine the H gas d…

astro-ph.GA2015★ 96 cited

A Comprehensive Study of the Radio Properties of Brightest Cluster Galaxies

M. T. Hogan, A. C. Edge, J. Hlavacek-Larrondo +7

We examine the radio properties of the Brightest Cluster Galaxies (BCGs) in a large sample of X-ray selected galaxy clusters comprising the Brightest Cluster Sample (BCS), the exte…

astro-ph.CO2013★ 75 cited

Massive molecular gas flows in the Abell 1664 brightest cluster galaxy

H. R. Russell, B. R. McNamara, A. C. Edge +14

We report ALMA Early Science CO(1-0) and CO(3-2) observations of the brightest cluster galaxy (BCG) in Abell 1664. The BCG contains 1.1x10^{10} solar masses of molecular gas divide…

astro-ph.CO2013★ 57 cited

Resolving the optical emission lines of Lya blob 'B1' at z=2.38: another hidden quasar

R. A. Overzier, N. P. H. Nesvadba, M. Dijkstra +5

We have used the SINFONI near-infrared integral field unit on the VLT to resolve the optical emission line structure of one of the brightest (L~1e44 erg/s) and nearest (z=2.38) of…

astro-ph.CO2012★ 23 cited

Multiphase Signatures of AGN Feedback in Abell 2597

G. R. Tremblay, C. P. O'Dea, S. A. Baum +18

We present new Chandra X-ray observations of the brightest cluster galaxy (BCG) in the cool core cluster Abell 2597. The data reveal an extensive kpc-scale X-ray cavity network as…