Published July 5, 1993 | Version v1
Journal article

A method for searching the Whipple Observatory gamma ray data base for evidence of GRB's

  • 1. Whipple Observatory, Harvard-Smithsonian CfA, Box 97, Amado, Arizona 85645 (United States)
  • 2. Physics Dept., University of Michigan, Ann Arbor, Michigan 48109 (United States)
  • 3. Physics Dept., St. Patrick's College, Maynooth, County Kildare (Ireland)
  • 4. Physics Dept., University College, Dublin, Belfield, Dublin 4 (Ireland)
  • 5. Physics Dept., Purdue University, West Lafayette, Indiana 47907 (United States)
  • 6. Physics Dept., University of Leeds, Leeds, LS2 9JT (United Kingdom)
  • 7. Physics and Astronomy Dept., Iowa State University, Ames, Iowa 50011 (United States)

Description

In light of recent Gamma Ray Burst (GRB) data from GRO, it is desirable to have a method for searching data from the Fred Lawrence Whipple Observatory 10 meter Cherenkov telescope for evidence of GRB's at TeV energies. In particular, this instrument's narrow field of view and high angular resolution make it well suited for observations of M31 as a test of the galactic halo model of GRB origin. We present here such a method, and give the results of its application to data taken on M31. Also reported here is an upper limit for the detection of a DC signal from M31

Additional details

Publishing Information

Journal Title
AIP Conference Proceedings
Journal Volume
280
Journal Issue
1
Journal Page Range
p. 833-837.
ISSN
0094-243X
CODEN
APCPCS

Conference

Title
Gamma Ray Observatory (GRO) symposium.
Dates
15-17 Oct 1992.
Place
St. Louis, MO (United States).

INIS

Optional Information

Secondary number(s)
CONF-9210245--.