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19982004
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astro-ph2004

Measurements of Gamma-Ray Bursts (GRBs) with Glast

G. G. Lichti, M. Briggs, R. Diehl +9

One of the scientific goals of the main instrument of GLAST is the study of Gamma-Ray Bursts (GRBs) in the energy range from ~20 MeV to ~300 GeV. In order to extend the energy meas…

astro-ph2001

The GLAST Burst Monitor (GBM)

G. G. Lichti, M. S. Briggs, R. Diehl +9

The selection of the GLAST burst monitor (GBM) by NASA will allow the investigation of the relation between the keV and the MeV-GeV emission from gamma-ray bursts. The GBM consists…

astro-ph1999

Gamma-Ray Burst Lines

Michael S. Briggs

The evidence for spectral features in gamma-ray bursts is summarized. As a guide for evaluating the evidence, the properties of gamma-ray detectors and the methods of analyzing gam…

astro-ph1999

Localizations of Thirteen Gamma-ray Bursts by the All-Sky Monitor on RXTE

D. A. Smith, A. M. Levine, H. V. Bradt +9

The All-Sky Monitor (ASM) on the Rossi X-ray Timing Explorer (RXTE) has been used to localize thirteen confirmed X-ray counterparts to Gamma-Ray Bursts (GRBs) detected over three y…

astro-ph1999

The Role of the BATSE Instrument Response in Creating the Gamma-Ray Burst E-Peak Distribution

J. J. Brainerd, G. Pendleton, R. Mallozzi +2

All gamma-ray bursts are observed to have approximately the same characteristic gamma-ray energy. We show in this article that for bursts in the BATSE data set, this property as me…

astro-ph1999

Spectral Energy Distributions and Light Curves of GRB 990123 and its Afterglow

T. J. Galama, M. S. Briggs, R. A. M. J. Wijers +38

Gamma-ray bursts (GRBs) are thought to result from the interaction of an extremely relativistic outflow interacting with a small amount of material surrounding the site of the expl…