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most citedGRB 080503: Implications of a Naked Short Gamma-Ray Burst Dominated by Extended Emission

205 citations · 609 across the 9 of their papers we have counts for

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astro-ph2008★ 205 cited

GRB 080503: Implications of a Naked Short Gamma-Ray Burst Dominated by Extended Emission

D. A. Perley, B. D. Metzger, J. Granot +22

We report on observations of GRB 080503, a short gamma-ray burst with very bright extended emission (about 30 times the gamma-ray fluence of the initial spike) in conjunction with…

astro-ph2006★ 11 cited

Discovery of a New X-Ray Burst/Millisecond Accreting Pulsar HETE J1900.1-2455

M. Suzuki, N. Kawai, T. Tamagawa +16

A class of low-mass X-ray binary sources are known to be both X-ray burst sources and millisecond pulsars at the same time. A new source of this class was discovered by High Energy…

astro-ph2005

HETE-2 Localization and Observations of the Gamma-Ray Burst GRB 020813

R. Sato, the HETE Science Team

A bright, long gamma-ray burst (GRB) was detected and localized by the instruments on board the High Energy Transient Explorer 2 satellite (HETE-2) at 02:44:19.17 UTC (9859.17 s UT…

astro-ph2005★ 9 cited

High Resolution Gratings Spectroscopy of GRBs 030382 and 041006 with Chandra LETGS

N. R. Butler, G. R. Ricker, P. G. Ford +5

We present high resolution X-ray spectroscopy of two recent GRB afterglows observed with the Low Energy Transmission Gratings on Chandra. The afterglows to GRBs 030328 and 041006 a…

astro-ph2004★ 68 cited

HETE Observations of the Gamma-Ray Burst GRB030329: Evidence for an Underlying Soft X-ray Component

R. Vanderspek, T. Sakamoto, C. Barraud +30

An exceptionally intense gamma-ray burst, GRB030329, was detected and localized by the instruments on board the High Energy Transient Explorer satellite (HETE) at 11:37:14 UT on 29…

astro-ph2003★ 56 cited

The X-ray Afterglows of GRB 020813 and GRB 021004 with Chandra HETGS: Possible Evidence for a Supernova Prior to GRB 020813

Nathaniel R. Butler, Herman L. Marshall, George R. Ricker +5

We report on the detection of an emission line near 1.3 keV, which we associate with blue-shifted hydrogen-like sulfur (S XVI), in a 76.8 ksec Chandra HETGS spectrum of the aftergl…