112 citations · 184 across the 7 of their papers we have counts for
7 papers
The Signature of Refreshed Shocks in the of Afterglow of GRB030329
Michael J. Moss, Robert Mochkovitch, Frédéric Daigne +2
GRB030329 displays one clear and, possibly, multiple less intense fast-rising () jumps in its optical afterglow light curve. The decay rate of the optical light cu…
A structured jet explains the extreme GRB 221009A
B. O'Connor, E. Troja, G. Ryan +29
Long duration gamma-ray bursts (GRBs) are powerful cosmic explosions, signaling the death of massive stars. Among them, GRB 221009A is by far the brightest burst ever observed. Due…
GRB 221009A: Discovery of an Exceptionally Rare Nearby and Energetic Gamma-Ray Burst
Maia A. Williams, Jamie A. Kennea, S. Dichiara +53
We report the discovery of the unusually bright long-duration gamma-ray burst (GRB), GRB 221009A, as observed by the Neil Gehrels Swift Observatory (Swift), Monitor of All-sky X-ra…
Instrumental Tip-of-the-iceberg Effects on the Prompt Emission of Swift/BAT Gamma-ray Bursts
M. Moss, A. Lien, S. Guiriec +2
The observed durations of prompt gamma-ray emission from gamma-ray bursts (GRBs) are often used to infer the progenitors and energetics of the sources. Inaccurate duration measurem…
Evidence of extended emission in GRB 181123B and other high-redshift short GRBs
S. Dichiara, E. Troja, P. Beniamini +7
We study the high-energy properties of GRB 181123B, a short gamma-ray burst (sGRB) at redshift 1.75. We show that, despite its nominal short duration with 2 s, t…
Observations of GX 339-4 in 1996
I. A. Smith, E. P. Liang, D. Lin +9
GX 339-4 is an unusual black hole candidate in that it is a persistent source, being detected by X-ray telescopes most of the time, but it also has nova-like flaring states. In 199…
Multiwavelength Observations of GX 339-4 in 1996. I. Daily Light Curves and X-ray and Gamma-Ray Spectroscopy
I. A. Smith, E. P. Liang, D. Lin +6
As part of our multiwavelength campaign of GX 339-4 observations in 1996 we present our radio, X-ray, and gamma-ray observations made in July, when the source was in a hard state (…