Search for Very High Energy Emission from Gamma-Ray Bursts using Milagro

Journal Article · Thu Jul 12 00:00:00 EDT 2007 · AIP Conference Proceedings

DOI:https://doi.org/10.1063/1.2757406· OSTI ID:21067769

Saz Parkinson, P M ^[1]

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1. Santa Cruz Institute for Particle Physics, University of California, Santa Cruz, CA 95064 (United States)

Gamma-Ray Bursts (GRBs) have been detected at GeV energies by EGRET and models predict emission at > 100 GeV. Milagro is a wide field (2 sr) high duty cycle (> 90%) ground based water Cherenkov detector that records extensive air showers in the energy range 100 GeV to 100 TeV. We have searched for very high energy emission from a sample of 106 gamma-ray bursts (GRB) detected since the beginning of 2000 by BATSE, BeppoSax, HETE-2, INTEGRAL, Swift or the IPN. No evidence for emission from any of the bursts has been found and we present upper limits from these bursts.

• OSTI ID: 21067769
• Journal Information: AIP Conference Proceedings, Vol. 921, Issue 1; Conference: 1. GLAST symposium, Stanford, CA (United States), 5-8 Feb 2007; Other Information: DOI: 10.1063/1.2757406; (c) 2007 American Institute of Physics; Country of input: International Atomic Energy Agency (IAEA). Milagro Collaboration; ISSN 0094-243X
• Country of Publication: United States
• Language: English

Related Subjects

71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
CHERENKOV COUNTERS
COSMIC GAMMA BURSTS
COSMIC GAMMA SOURCES
COSMIC PHOTONS
EXTENSIVE AIR SHOWERS
GAMMA DETECTION
GEV RANGE
PHOTON EMISSION
TELESCOPE COUNTERS
TEV RANGE
WATER