activity
20062009
most citedThe First Swift Ultra-Violet/Optical Telescope GRB Afterglow Catalog

144 citations · 508 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph200944 cited

Swift-UVOT captures the earliest ultraviolet spectrum of a Gamma Ray Burst

N. P. M. Kuin, W. B. Landsman, M. J. Page +22

We present the earliest ever ultraviolet spectrum of a gamma-ray burst (GRB) as observed with the Swift-UVOT. The GRB 081203A spectrum was observed for 50 seconds with the UV grism…

astro-ph.HE2009144 cited

A statistical study of gamma-ray burst afterglows measured by the Swift Ultra-violet Optical Telescope

S. R. Oates, M. J. Page, P. Schady +14

We present the first statistical analysis of 27 UVOT optical/ultra-violet lightcurves of GRB afterglows. We have found, through analysis of the lightcurves in the observer's frame,…

astro-ph200842 cited

Jet breaks at the end of the slow decline phase of Swift GRB lightcurves

M. De Pasquale, P. Evans, S. Oates +9

The Swift mission has discovered an intriguing feature of Gamma-Ray Burst (GRBs) afterglows, a phase of shallow decline of the flux in the X-ray and optical lightcurves. This behav…

astro-ph2008144 cited

The First Swift Ultra-Violet/Optical Telescope GRB Afterglow Catalog

P. W. A. Roming, T. S. Koch, S. R. Oates +21

We present the first Swift Ultra-Violet/Optical Telescope (UVOT) gamma-ray burst (GRB) afterglow catalog. The catalog contains data from over 64,000 independent UVOT image observat…

astro-ph200845 cited

GRB 060605: multi-wavelength analysis of the first GRB observed using integral field spectroscopy

Patrizia Ferrero, Sylvio Klose, David Alexander Kann +16

The long and relatively faint gamma-ray burst GRB 060605 detected by \emph{Swift}/BAT lasted about 20 sec. Its afterglow could be observed with \emph{Swift}/XRT for nearly 1 day, w…

astro-ph200729 cited

GRB 060607A: A GRB with Bright Asynchronous Early -ray and Optical Emissions

Houri Ziaeepour, Stephen T. Holland, Patricia T. Boyd +8

The early optical emission of the moderately high redshift () GRB 060607A shows a remarkable broad and strong peak with a rapid rise and a relatively slow power-law decay.…