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The bright end of the galaxy luminosity function at z ~ 7: before the onset of mass quenching?
R. A . A. Bowler, J. S. Dunlop, R. J. McLure +9
We present the results of a new search for bright star-forming galaxies at z ~ 7 within the UltraVISTA DR2 and UKIDSS UDS DR10 data, which together provide 1.65 sq deg of near-infr…
Caught in the act: Cluster `k+a' galaxies as a link between spirals and S0s
Bruno Rodriguez Del Pino, Steven P. Bamford, Alfonso Aragon-Salamanca +3
We use integral field spectroscopy of 13 disk galaxies in the cluster AC114 at z ~ 0.31 in an attempt to disentangle the physical processes responsible for the transformation of sp…
The Redshift Distribution of the TOUGH Survey
P. Jakobsson, R. Chapman, J. Hjorth +5
We present the redshift results from a Very Large Telescope program aimed at optimizing the legacy value of the Swift mission: to characterize a homogeneous, X-ray selected, sample…
The metallicity and dust content of a redshift 5 gamma-ray burst host galaxy
M. Sparre, O. E. Hartoog, T. Krühler +26
Observations of the afterglows of long gamma-ray bursts (GRBs) allow the study of star-forming galaxies across most of cosmic history. Here we present observations of GRB 111008A f…
Spectroscopy of the short-hard GRB 130603B: The host galaxy and environment of a compact object merger
A. de Ugarte Postigo, C. C. Thoene, A. Rowlinson +40
Short duration gamma-ray bursts (SGRBs) are thought to be related to the violent merger of compact objects, such as neutron stars or black holes, which makes them promising sources…
Discovery of the broad-lined Type Ic SN 2013cq associated with the very energetic GRB 130427A
D. Xu, A. de Ugarte Postigo, G. Leloudas +25
Long-duration gamma-ray bursts (GRBs) at z < 1 are in most cases found to be accompanied by bright, broad-lined Type Ic supernovae (SNe Ic-BL). The highest-energy GRBs are mostly l…