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19972025
most citedMethods and results of an automatic analysis of a complete sample of Swift-XRT observations of GRBs

1.8k citations · 14.4k across the 145 of their papers we have counts for

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10 papers · 1 filter

astro-ph.HE2011★ 13 cited

Swift follow-up observations of unclassified ASCA sources

N. Degenaar, R. L. C. Starling, P. A. Evans +11

We present Swift follow-up observations of a sample of 35 unclassified faint X-ray sources drawn from the ASCA Galactic centre and plane surveys. Our short pointed XRT observations…

astro-ph.HE2011★ 49 cited

Panchromatic observations of the textbook GRB 110205A: constraining physical mechanisms of prompt emission and afterglow

W. Zheng, R. F. Shen, T. Sakamoto +56

We present a comprehensive analysis of a bright, long duration (T90 ~ 257 s) GRB 110205A at redshift z= 2.22. The optical prompt emission was detected by Swift/UVOT, ROTSE-IIIb and…

astro-ph.SR2011★ 161 cited

Swift X-Ray Observations of Classical Novae. II. The Super Soft Source sample

Greg J. Schwarz, Jan-Uwe Ness, J. P. Osborne +9

The Swift GRB satellite is an excellent facility for studying novae. Its rapid response time and sensitive X-ray detector provides an unparalleled opportunity to investigate the pr…

astro-ph.IM2011★ 12 cited

Recovering Swift-XRT energy resolution through CCD charge trap mapping

C. Pagani, A. P. Beardmore, A. F. Abbey +13

The X-ray telescope on board the Swift satellite for gamma-ray burst astronomy has been exposed to the radiation of the space environment since launch in November 2004. Radiation c…

astro-ph.HE2011★ 2 cited

Swift observations of the March 2011 outburst of the cataclysmic variable NSV 1436: a probable dwarf nova (Research Note)

J. P. Osborne, K. L. Page, A. A. Henden +7

The March 2011 outburst of the poorly-studied cataclysmic variable NSV 1436 offered an opportunity to decide between dwarf nova and recurrent nova classifications. We use seven dai…

astro-ph.HE2011★ 28 cited

Swift observations of the 2006 outburst of the recurrent nova RS Ophiuchi: III. X-ray spectral modelling

N. M. H. Vaytet, T. J. O'Brien, K. L. Page +3

Following the Swift X-ray observations of the 2006 outburst of the recurrent nova RS Ophiuchi, we developed hydrodynamical models of mass ejection from which the forward shock velo…