102 citations · 584 across the 14 of their papers we have counts for
14 papers
Strength in Numbers: Red Galaxies Bolster the Cosmic Star Formation Rate Density at z > 3
L. Barrufet, J. S. Dunlop, R. Begley +20
A comprehensive account of the cosmic star-formation history demands an accurate census of dust-enshrouded star formation over cosmic time. We provide strong new constraints from a…
Deep ATCA and VLA radio observations of short-GRB host galaxies. Constraints on star-formation rates, afterglow flux, and kilonova radio flares
S. Klose, A. M. Nicuesa Guelbenzu, M. Michalowski +6
We report the results of an extensive radio-continuum observing campaign of host galaxies of short gamma-ray bursts (GRBs). The goal of this survey was to search for optically obsc…
The Causes of the Red Sequence, the Blue Cloud, the Green Valley and the Green Mountain
Stephen Eales, Maarten Baes, Nathan Bourne +23
The galaxies found in optical surveys fall in two distinct regions of a diagram of optical colour versus absolute magnitude: the red sequence and the blue cloud with the green vall…
Modelling high resolution ALMA observations of strongly lensed highly star forming galaxies detected by Herschel
S. Dye, C. Furlanetto, L. Dunne +12
We have modelled high resolution ALMA imaging of six strong gravitationally lensed galaxies detected by the Herschel Space Observatory. Our modelling recovers mass properties of th…
An imperfectly passive nature: Bright sub-millimeter emission from dust-obscured star formation in the z=3.717 "passive" system, ZF20115
J. M. Simpson, Ian Smail, Wei-Hao Wang +28
The identification of high-redshift massive galaxies with old stellar populations may pose challenges to some models of galaxy formation. However, to securely classify a galaxy as…
VALES: II. The physical conditions of interstellar gas in normal star-forming galaxies up to z=0.2 revealed by ALMA
T. M. Hughes, E. Ibar, V. Villanueva +18
We use new Band-3 CO(1-0) observations taken with the Atacama Large Millimeter/submillimeter Array (ALMA) to study the physical conditions in the interstellar gas of a sample of 27…