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19932026
most citedBeaming in Gamma-Ray Bursts: Evidence for a Standard Energy Reservoir

1.2k citations · 24.4k across the 223 of their papers we have counts for

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astro-ph2000★ 250 cited

Observation of X-ray lines from a Gamma-Ray Burst (GRB991216): Evidence of Moving Ejecta from the Progenitor

L. Piro, G. Garmire, M. Garcia +18

We report on the discovery of two emission features observed in the X-ray spectrum of the afterglow of the gamma-ray burst (GRB) of 16 Dec. 1999 by the Chandra X-Ray Observatory. T…

astro-ph2000★ 43 cited

The Bright Gamma-Ray Burst 991208 - Tight Constraints on Afterglow Models from Observations of the Early-Time Radio Evolution

T. J. Galama, M. Bremer, F. Bertoldi +13

The millimeter wavelength emission from GRB 991208 is the second brightest ever detected, yielding a unique data set. We present here well-sampled spectra and light curves over mor…

astro-ph2000★ 103 cited

A Jet Model for the Afterglow Emission from GRB000301C

E. Berger, R. Sari, D. A. Frail +11

We present broad-band radio observations of the afterglow of GRB000301C, spanning from 1.4 to 350 GHz for the period of 3 to 83 days after the burst. This radio data, in addition t…

astro-ph2000★ 23 cited

The Rapidly Fading Afterglow from the Gamma-Ray Burst of 1999 May 6

G. B. Taylor, J. S. Bloom, D. A. Frail +3

We report on the discovery of the radio afterglow from the gamma-ray burst (GRB) of 1999 May 6 (GRB 990506) using the Very Large Array (VLA). The radio afterglow was detected at ea…

astro-ph2000★ 73 cited

Limits on radio emission from pulsar wind nebulae

B. M. Gaensler, B. W. Stappers, D. A. Frail +3

We report on a sensitive survey for radio pulsar wind nebulae (PWN) towards 27 energetic and/or high velocity pulsars. Observations were carried out at 1.4 GHz using the Very Large…

astro-ph2000★ 30 cited

Interplanetary Network Localization of GRB991208 and the Discovery of its Afterglow

K. Hurley, T. Cline, E. Mazets +9

The extremely energetic (~10^-4 erg/cm^2) gamma-ray burst (GRB) of 1999 December 8 was triangulated to a ~14 sq. arcmin. error box ~1.8 d after its arrival at Earth with the 3rd in…