356 citations · 4.9k across the 111 of their papers we have counts for
6 papers · 1 filter
Host galaxies of luminous z0.6 quasars: Major mergers are not prevalent at the highest AGN luminosities
C. Villforth, T. Hamilton, M. M. Pawlik +10
Galaxy interactions are thought to be one of the main triggers of Active Galactic Nuclei (AGN), especially at high luminosities, where the accreted gas mass during the AGN lifetime…
Herschel-ATLAS: Revealing dust build-up and decline across gas, dust and stellar mass selected samples: I. Scaling relations
P. De Vis, L. Dunne, S. Maddox +19
We present a study of the dust, stars and atomic gas (HI) in an HI-selected sample of local galaxies (z<0.035) in the Herschel Astrophysical Terahertz Large Area Survey (H-ATLAS) f…
The evolution of post-starburst galaxies from z=2 to z= 0.5
Vivienne Wild, Omar Almaini, Jim Dunlop +5
We present the evolution in the number density and stellar mass functions of photometrically selected post-starburst galaxies in the UKIDSS Deep Survey (UDS), with redshifts of 0.5…
The Herschel-ATLAS Data Release 1 Paper II: Multi-wavelength counterparts to submillimetre sources
N. Bourne, L. Dunne, S. J. Maddox +27
This paper is the second in a pair of articles presenting data release 1 (DR1) of the Herschel Astrophysical Terahertz Large Area Survey (H-ATLAS), the largest single open-time key…
The identification of post-starburst galaxies at z~1 using multiwavelength photometry: a spectroscopic verification
David T. Maltby, Omar Almaini, Vivienne Wild +7
Despite decades of study, we still do not fully understand why some massive galaxies abruptly switch off their star formation in the early Universe, and what causes their rapid tra…
Shape asymmetry: a morphological indicator for automatic detection of galaxies in the post-coalescence merger stages
M. M. Pawlik, V. Wild, C. J. Walcher +5
We present a new morphological indicator designed for automated recognition of galaxies with faint asymmetric tidal features suggestive of an ongoing or past merger. We use this ne…