activity
19982008
most citedThe short GRB070707 afterglow and its very faint host galaxy

43 citations · 45 across the 5 of their papers we have counts for

collaborators
Showing astro-phShow all

6 papers · 1 filter

astro-ph2008

Swift Observations of Shock Evolution in RS Ophiuchi

M. F. Bode, J. P. Osborne, K. L. Page +11

Our \textit{Swift} observations of RS Oph form an unprecedented X-ray dataset to undertake investigations of both the central source and the interaction of the outburst ejecta with…

astro-ph200843 cited

The short GRB070707 afterglow and its very faint host galaxy

S. Piranomonte, P. D'Avanzo, S. Covino +18

We present the results from an ESO/VLT campaign aimed at studying the afterglow properties of the short/hard gamma ray burst GRB 070707. Observations were carried out at ten differ…

astro-ph2008

V723 Cassiopeia still on in X-rays: A bright Super Soft Source 12 years after outburst

J. U-. Ness, G. Schwarz, S. Starrfield +5

We find that the classical nova V723 Cas (1995) is still an active X-ray source more than 12 years after outburst and analyze seven X-ray observations carried out with Swift betwee…

astro-ph2007

Automatic analysis of Swift-XRT data

P. A. Evans, L. G. Tyler, A. P. Beardmore +1

The Swift spacecraft detects and autonomously observes ~100 Gamma Ray Bursts (GRBs) per year, ~96% of which are detected by the X-ray telescope (XRT). GRBs are accompanied by optic…

astro-ph20052 cited

Prompt and afterglow early X-ray phases in the comoving frame. Evidence for Universal properties?

G. Chincarini, A. Moretti, P. Romano +38

We analyze the Swift XRT light curves and spectra of the gamma-ray bursts (GRBs) for which the redshift has been measured. The sample consists of seven GRBs. The soft X-ray light c…

astro-ph1998

YY Draconis and V709 Cassiopeiae: two intermediate polars with weak magnetic fields

A. J. Norton, A. P. Beardmore, Alasdair Allan +1

We present data from long ROSAT HRI observations of the intermediate polars YY Dra and V709 Cas which show that V709 Cas, like YY Dra, exhibits a double-peaked X-ray pulse profile.…