activity
19932005
most citedPossible Gravitational Microlensing of a Star in the Large Magellanic Cloud

769 citations · 1.4k across the 12 of their papers we have counts for

collaborators

12 papers

astro-ph2005★ 119 cited

Discovery and identification of the very high redshift afterglow of GRB 050904

J. Haislip, M. Nysewander, D. Reichart +39

In 2000, Lamb and Reichart predicted that gamma-ray bursts (GRBs) and their afterglows occur in sufficient numbers and at sufficient brightnesses at very high redshifts (z > 5) to…

astro-ph2004★ 43 cited

The Swift Gamma-Ray Burst Mission

N. Gehrels, G Chincarini, P. Giommi +12

The Swift mission, scheduled for launch in early 2004, is a multiwavelength observatory for gamma-ray burst (GRB) astronomy. It is the first-of-its-kind autonomous rapid-slewing sa…

hep-ex2002★ 11 cited

Tracking Performance of the Scintillating Fiber Detector in the K2K Experiment

B. J. Kim, T. Iwashita, T. Ishida +39

The K2K long-baseline neutrino oscillation experiment uses a Scintillating Fiber Detector (SciFi) to reconstruct charged particles produced in neutrino interactions in the near det…

astro-ph2001★ 54 cited

Afterglow upper limits for four short duration, hard spectrum gamma-ray bursts

K. Hurley, E. Berger, A. Castro-Tirado +21

We present interplanetary network localization, spectral, and time history information for four short-duration, hard spectrum gamma-ray bursts, GRB000607, 001025B, 001204, and 0101…

astro-ph1999★ 1 cited

LOTIS Upper Limits and the Prompt OT from GRB 990123

G. G. Williams, D. H. Hartmann, H. S. Park +14

GRB 990123 established the existence of prompt optical emission from gamma-ray bursts (GRBs). The Livermore Optical Transient Imaging System (LOTIS) has been conducting a fully aut…

astro-ph1999★ 21 cited

Discovery of the Optical Transient of the Gamma Ray Burst 990308

Bradley E. Schaefer, J. A. Snyder, J. Hernandez +53

The optical transient of the faint Gamma Ray Burst 990308 was detected by the QUEST camera on the Venezuelan 1-m Schmidt telescope starting 3.28 hours after the burst. Our photomet…