2.2k citations · 7.4k across the 25 of their papers we have counts for
25 papers
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…
Non-parametric analysis of the rest-frame UV sizes and morphological disturbance amongst L* galaxies at 4<z<8
E. Curtis-Lake, R. J. McLure, J. S. Dunlop +12
We present the results of a study investigating the sizes and morphologies of redshift 4 < z < 8 galaxies in the CANDELS GOODS-S, HUDF and HUDF parallel fields. Based on non-parame…
Evidence for a correlation between the sizes of quiescent galaxies and local environment to z ~ 2
Caterina Lani, Omar Almaini, William G. Hartley +14
We present evidence for a strong relationship between galaxy size and environment for the quiescent population in the redshift range 1 < z < 2. Environments were measured using pro…
The Redshift and Mass Dependence on the Formation of The Hubble Sequence at z>1 from CANDELS/UDS
Alice Mortlock, Christopher J. Conselice, William G. Hartley +16
In this paper we present a detailed study of the structures and morphologies of a sample of 1188 massive galaxies with Mstar>10^10Msun between redshifts z=1-3 within the Ultra Deep…
CANDELS Multiwavelength catalogs: Source Identification and Photometry in the CANDELS UKIDSS Ultra-Deep Survey Field
Audrey Galametz, Andrea Grazian, Adriano Fontana +42
We present the multiwavelength - ultraviolet to mid-infrared - catalog of the UKIDSS Ultra-Deep Survey (UDS) field observed as part of the Cosmic Assembly Near-infrared Deep Extrag…
The Morphologies of Massive Galaxies at 1 < z < 3 in the CANDELS-UDS Field
V. A. Bruce, J. S. Dunlop, M. Cirasuolo +16
We have used high-resolution, HST WFC3/IR, near-infrared imaging to conduct a detailed bulge-disk decomposition of the morphologies of ~200 of the most massive (M_star > 10^11 M_so…