activity
19962025
most cited3D-HST+CANDELS: The Evolution of the Galaxy Size-Mass Distribution since

1.4k citations · 3.4k across the 21 of their papers we have counts for

collaborators
Showing 2014Show all

5 papers · 1 filter

astro-ph.GA2014★ 74 cited

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…

astro-ph.GA2014★ 91 cited

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…

astro-ph.GA2014★ 89 cited

Keck-I MOSFIRE spectroscopy of compact star-forming galaxies at z2: High velocity dispersions in progenitors of compact quiescent galaxies

G. Barro, J. R. Trump, D. C. Koo +28

We present Keck-I MOSFIRE near-infrared spectroscopy for a sample of 13 compact star-forming galaxies (SFGs) at redshift with star formation rates of SFR100…

astro-ph.GA2014★ 1.4k cited

3D-HST+CANDELS: The Evolution of the Galaxy Size-Mass Distribution since

A. van der Wel, M. Franx, P. G. van Dokkum +27

Spectroscopic + photometric redshifts, stellar mass estimates, and rest-frame colors from the 3D-HST survey are combined with structural parameter measurements from CANDELS imaging…

astro-ph.GA2014★ 172 cited

Morphologies of z~0.7 AGN Host Galaxies in CANDELS: No trend of merger incidence with AGN luminosity

C. Villforth, F. Hamann, D. J. Rosario +24

The processes that trigger Active Galactic Nuclei (AGN) remain poorly understood. While lower luminosity AGN may be triggered by minor disturbances to the host galaxy, stronger dis…