Very High Energy Observations of Gamma Ray Bursts with the Whipple/VERITAS Telescopes

Journal Article · Mon Feb 21 04:00:00 EST 2005 · AIP Conference Proceedings

DOI:https://doi.org/10.1063/1.1878468· OSTI ID:20630536

Horan, D ^[1]; Badran, H M; Blaylock, G; Bond, I H; Boyle, P J; Bradbury, S M; Buckley, J H; Byrum, K; Carter-Lewis, D A; Celik, O; Cogan, P; Cui, W; Daniel, M K; Duke, C; Falcone, A; Fegan, D J; Fegan, S J; Finley, J P; Fortson, L F ^[2]

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1. Harvard-Smithsonian Center for Astrophysics, P.O. Box 97, Amado, AZ 85645 (United States)
2. and others

Gamma-ray Burst (GRB) observations at Very High Energies (VHE, E > 100 GeV) can impose tight constraints on some GRB emission models. Many GRB after-glow models predict a VHE component similar to that seen in blazars and supernova remnants, in which the GRB spectral energy distribution has a double-peaked shape extending into the VHE regime. Consistent with this afterglow scenario, EGRET detected delayed high energy emission from all five bright BATSE GRBs that occurred within its field of view. GRB observations have had high priority in the observing program at the Whipple 10m Telescope and will continue to be high priority targets when the next generation observatory VERITAS comes online. Upper limits on the VHE emission from ten GRBs observed with the Whipple Telescope are reported here.

• OSTI ID: 20630536
• Journal Information: AIP Conference Proceedings, Journal Name: AIP Conference Proceedings Journal Issue: 1 Vol. 745; ISSN APCPCS; ISSN 0094-243X
• Country of Publication: United States
• Language: English

Related Subjects

72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS
AFTERGLOW
COSMIC GAMMA BURSTS
COSMIC GAMMA SOURCES
COSMIC PHOTONS
COSMIC RAY DETECTION
ENERGY SPECTRA
GAMMA ASTRONOMY
GEV RANGE
PHOTON EMISSION
SUPERNOVA REMNANTS
TELESCOPE COUNTERS