297 citations · 1.2k across the 8 of their papers we have counts for
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Major mergers are not significant drivers of star formation or morphological transformation around the epoch of peak cosmic star formation
E. K. Lofthouse, S. Kaviraj, C. J. Conselice +2
We investigate the contribution of major mergers (mass ratios ) to stellar mass growth and morphological transformations around the epoch of peak cosmic star formation ($z\si…
Evolution of cosmic star formation in the SCUBA-2 Cosmology Legacy Survey
N. Bourne, J. S. Dunlop, E. Merlin +19
We present a new exploration of the cosmic star-formation history and dust obscuration in massive galaxies at redshifts . We utilize the deepest 450 and 850m imaging f…
Stellar masses from the CANDELS survey: the GOODS-South and UDS fields
P. Santini, H. C. Ferguson, A. Fontana +35
We present the public release of the stellar mass catalogs for the GOODS-S and UDS fields obtained using some of the deepest near-IR images available, achieved as part of the Cosmi…
The SCUBA-2 Cosmology Legacy Survey: ALMA resolves the rest-frame far-infrared emission of sub-millimeter galaxies
J. M. Simpson, Ian Smail, A. M. Swinbank +26
We present high-resolution (0.3'') ALMA 870um imaging of 52 sub-millimeter galaxies (SMGs) in the Ultra Deep Survey (UDS) field and investigate the size and morphology of the sub-m…
The host galaxies of X-ray selected Active Galactic Nuclei to z=2.5: Structure, star-formation and their relationships from CANDELS and Herschel/PACS
D. J. Rosario, D. H. McIntosh, A. van der Wel +60
We study the relationship between the structure and star-formation rate (SFR) of X-ray selected low and moderate luminosity active galactic nuclei (AGNs) in the two Chandra Deep Fi…
Why z > 1 radio-loud galaxies are commonly located in proto-clusters
N. A. Hatch, D. Wylezalek, J. D. Kurk +9
Distant powerful radio-loud active galactic nuclei (RLAGN) tend to reside in dense environments and are commonly found in proto-clusters at z > 1.3. We examine whether this occurs…