activity
20042009
most citedThe formation and assembly of a typical star-forming galaxy at z~3

170 citations · 530 across the 6 of their papers we have counts for

collaborators

10 papers

astro-ph.GA2009124 cited

A submillimetre galaxy at z=4.76 in the LABOCA survey of the Extended Chandra Deep Field South

Kristen Coppin, Ian Smail, David M. Alexander +30

We report on the identification of the highest redshift submm-selected source currently known: LESSJ033229.4-275619. This source was detected in the Large Apex BOlometer CAmera (LA…

astro-ph.GA20094 cited

Kinematics and Formation Mechanisms of High-Redshift Galaxies

David R. Law, Shelley A. Wright, Richard S. Ellis +4

Recent years have witnessed a substantial increase in our ability to trace the spatially resolved properties of rapidly star-forming galaxies in the high-redshift universe and nume…

astro-ph.CO200928 cited

Evidence of a link between the evolution of clusters and their AGN fraction

Caroline van Breukelen, Chris Simpson, Steve Rawlings +9

We discuss the optical properties, X-ray detections, and Active Galactic Nucleus (AGN) populations of four clusters at z ~ 1 in the Subaru-XMM Deep Field (SXDF). The velocity distr…

astro-ph2008170 cited

The formation and assembly of a typical star-forming galaxy at z~3

Daniel P. Stark, Mark Swinbank, Richard S. Ellis +3

Recent studies of galaxies ~2-3 Gyr after the Big Bang have revealed large, turbulent rotating systems. The existence of well-ordered rotation in galaxies during this peak epoch of…

astro-ph2008158 cited

Testing the Evolutionary Link Between Submillimetre Galaxies and Quasars: CO Observations of QSOs at z~2

Kristen Coppin, Mark Swinbank, Roberto Neri +10

We have used the IRAM Plateau de Bure mm interferometer and the UKIRT 1-5 um Imager Spectrometer to test the connection between the major phases of spheroid growth and nuclear accr…

astro-ph200646 cited

Galaxies Under the Cosmic Microscope: Resolved Spectroscopy and New Constraints on the z=1 Tully-Fisher relation

M. Swinbank, R. Bower, G. P. Smith +5

We exploit the gravitational potential of massive cluster lenses to probe the emission line properties of six z=1 galaxies which appear as highly magnified luminous arcs. Using the…