activity
20072016
most citedA deep ALMA image of the Hubble Ultra Deep Field

385 citations · 2.1k across the 17 of their papers we have counts for

collaborators

17 papers

astro-ph.GA2016★ 385 cited

A deep ALMA image of the Hubble Ultra Deep Field

J. S. Dunlop, R. J. McLure, A. D. Biggs +33

We present the results of the first, deep ALMA imaging covering the full 4.5 sq arcmin of the Hubble Ultra Deep Field (HUDF) as previously imaged with WFC3/IR on HST. Using a mosai…

astro-ph.GA2016★ 112 cited

The ASTRODEEP Frontier Fields Catalogues: I - Multiwavelength photometry of Abell-2744 and MACS-J0416

E. Merlin, R. Amorìn, M. Castellano +28

We present multiwavelength photometric catalogues (HST, Spitzer and Hawk-I K band) for the first two of the Frontier Fields, Abell2744 and MACSJ0416 (plus their parallel fields). T…

astro-ph.HE2015★ 46 cited

Chandra counterparts of CANDELS GOODS-S sources

N. Cappelluti, A. Comastri, A. Fontana +18

Improving the capabilities of detecting faint X-ray sources is fundamental to increase the statistics on faint high-z AGN and star-forming galaxies. We performed a simultaneous Max…

astro-ph.GA2015★ 17 cited

Identification of z~>2 Herschel 500 micron sources using color-deconfusion

X. W. Shu, D. Elbaz, N. Bourne +19

We present a new method to search for candidate z~>2 Herschel 500μm sources in the GOODS-North field, using a S500μm/S24μm "color deconfusion" technique. Potential high-z sources a…

astro-ph.GA2015★ 23 cited

The bulge-disk decomposition of AGN host galaxies

V. A. Bruce, J. S. Dunlop, A. Mortlock +3

We present the results from a study of the morphologies of moderate luminosity X-ray selected AGN host galaxies in comparison to a carefully mass-matched control sample at 0.5 < z…

astro-ph.GA2014★ 60 cited

The Decomposed Bulge and Disk Size-Mass Relations of Massive Galaxies at 1<z<3 in CANDELS

V. A. Bruce, J. S. Dunlop, R. J. McLure +15

We have constructed a mass-selected sample of Mstar>10^11Msolar galaxies at 1<z<3 in the CANDELS UDS and COSMOS fields and have decomposed these systems into their separate bulge a…