Astronomy and Astrophysics – Astrophysics
Scientific paper
2007-02-14
Astronomy and Astrophysics
Astrophysics
submitted to ApJ
Scientific paper
10.1086/521591
We present the first systematic investigation of the morphological and timing properties of flares in GRBs observed by Swift/XRT. We consider a large sample drawn from all GRBs detected by Swift, INTEGRAL and HETE-2 prior to 2006 Jan 31, which had an XRT follow-up and which showed significant flaring. Our sample of 33 GRBs includes long and short, at low and high redshift, and a total of 69 flares. The strongest flares occur in the early phases, with a clear anti-correlation between the flare peak intensity and the flare time of occurrence. Fitting each X-ray flare with a Gaussian model, we find that the mean ratio of the width and peak time is
Burrows David N.
Campana Sergio
Capalbi Milvia
Chincarini Guido
Cusumano Giancarlo
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