activity
20072023
most citedGOODS-Herschel: an infrared main sequence for star-forming galaxies

1.1k citations · 9.5k across the 105 of their papers we have counts for

collaborators
Showing 2015 · astro-ph.GAShow all

5 papers · 2 filters

astro-ph.GA2015★ 161 cited

The KMOS AGN Survey at High redshift (KASHz): the prevalence and drivers of ionised outflows in the host galaxies of X-ray AGN

C. M. Harrison, D. M. Alexander, J. R. Mullaney +7

We present the first results from the KMOS AGN Survey at High redshift (KASHz), a VLT/KMOS integral-field spectroscopic survey of z>0.6 AGN. We present galaxy-integrated spectra of…

astro-ph.GA2015★ 24 cited

ALMA resolves extended star formation in high-z AGN host galaxies

C. M. Harrison, J. M. Simpson, F. Stanley +6

We present high resolution (0.3") Atacama Large Millimeter Array (ALMA) 870um imaging of five z~1.5-4.5 X-ray detected AGN with luminosities of L(2-8keV)>10^42 erg/s. These data pr…

astro-ph.GA2015★ 125 cited

ALMA and Herschel reveal that X-ray selected AGN and main-sequence galaxies have different star formation rate distributions

J. R. Mullaney, D. M. Alexander, J. Aird +15

Using deep Herschel and ALMA observations, we investigate the star formation rate (SFR) distributions of X-ray selected AGN host galaxies at 0.5<z<1.5 and 1.5<z<4, comparing them t…

astro-ph.GA2015★ 82 cited

Mid-infrared luminous quasars in the GOODS-Herschel fields: a large population of heavily-obscured, Compton-thick quasars at z~2

A. Del Moro, D. M. Alexander, F. E. Bauer +10

We present the infrared (IR) and X-ray properties of a sample of 33 mid-IR luminous quasars (L(6 micron)>6x10 erg/s) at redshift z~1-3, identified through detailed spectr…

astro-ph.GA2015★ 184 cited

A remarkably flat relationship between the average star formation rate and AGN luminosity for distant X-ray AGN

F. Stanley, C. M. Harrison, D. M. Alexander +5

In this study we investigate the relationship between the star formation rate, SFR, and AGN luminosity, L(AGN), for ~2000 X-ray detected AGN. The AGN span over three orders of magn…