activity
19992002
most citedThe Signature of Supernova Ejecta Measured in the X-ray Afterglow of Gamma-Ray Burst 011211

205 citations · 364 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph2002★ 53 cited

The X-ray afterglows of gamma-ray bursts GRB 001025A and GRB 010220 observed with XMM-Newton

D. Watson, J. N. Reeves, J. Osborne +5

The X-ray afterglows of GRB 001025A and GRB 010220 were detected by XMM-Newton with an average 0.2--10.0 keV flux of 4.4 and 3.3x10^{-14} erg cm^{-2} s^{-1} respectively; the after…

astro-ph2002★ 50 cited

Soft X-ray emission lines in the afterglow spectrum of GRB 011211:- a detailed XMM-Newton analysis

J. N. Reeves, D. Watson, J. P. Osborne +2

We report on an XMM-Newton observation of the X-ray afterglow of the Gamma Ray Burst GRB 011211, originally detected by Beppo-SAX on 11th December 2001. The early afterglow spectru…

astro-ph2002★ 7 cited

Temporal properties of short and long gamma-ray bursts

S. McBreen, F. Quilligan, B. McBreen +2

A temporal analysis was performed on a sample of 100 bright short GRBs with T90 < 2s from the BATSE Current Catalog along with a similar analysis on 319 long bright GRBs with T90 >…

astro-ph2002★ 205 cited

The Signature of Supernova Ejecta Measured in the X-ray Afterglow of Gamma-Ray Burst 011211

J. N. Reeves, D. Watson, J. P. Osborne +8

Since their identification with cosmological distances, Gamma-ray bursts (GRBs) have been recognised as the most energetic phenomena in the Universe, with an isotropic burst energy…

astro-ph2001★ 48 cited

Temporal properties of the short gamma-ray bursts

S. McBreen, F. Quilligan, B. McBreen +2

A temporal analysis has been performed on a sample of 100 bright gamma-ray bursts (GRBs) with T90<2s from the BATSE current catalog. The GRBs were denoised using a median filter an…

astro-ph2000★ 1 cited

ISO observations of a sample of 60 micron peaker galaxies

R. J. Laureijs, D. Watson, L. Metcalfe +9

The sample of IRAS galaxies with spectral energy distributions that peak near 60 microns are called Sixty Micron Peakers (SMPs or 60PKs). Their generally peculiar and amorphous mor…