Observing gamma ray bursts (GRBs) in the TeV energy range can be extremely valuable in providing insight to GRB radiation mechanisms and in constraining source distances. The Milagrito detector was an air shower array which used the water Cherenkov technique to search for TeV sources. Data from this detector was analyzed to look for a TeV component of GRBs coincident with low energy -rays detected by the BATSE instrument on the Compton Gamma Ray Observatory. A sample of 54 BATSE GRBs which were in the field of view of the Milagrito detector during its lifetime (February 1997 to May 1998) was used
Milagrito, a large, covered water-Cherenkov detector, was the world\u27s rst air-shower-particle de...
A wide field of view, high duty factor TeV gamma-ray observa-tory is essential for studying TeV astr...
Abstract: Gamma-ray bursts (GRBs) have been detected up to GeV energies and are predicted by many mo...
Milagrito, a detector sensitive to gamma-rays at TeV energies, monitored the northern sky during the...
Milagrito, a detector sensitive to very high energy gamma rays, monitored the northern sky from 1997...
Abstract. The Milagro detector surveyed the sky almost continuously in the very high energy regime f...
The Milagro gamma-ray observatory employs a water Cherenkov detector to observe extensive air shower...
Milagro is a wide field (2 sr) high duty cycle (>90%) ground-based water Cherenkov detector designed...
Milagro is a water-Cherenkov detector that observes the extended air showers produced by cosmic gamm...
The Milagro telescope monitors the northern sky for 100 GeV - 100 TeV transient emission through con...
The Milagro gamma-ray observatory employs a water Cherenkov detector to observe extensive air shower...
The Milagrito water Cherenkov telescope operated for over a year. The most probable gamma-ray energy...
The Milagro Gamma-Ray Observatory employs a water Cerenkov detector to observe extensive air showers...
The Milagro Gamma-Ray Observatory, located at an altitude of 2630m in the mountains of northern New ...
discovered one of the brightest gamma-ray bursts ever recorded. With a peak visual magnitude of 5.3,...
Milagrito, a large, covered water-Cherenkov detector, was the world\u27s rst air-shower-particle de...
A wide field of view, high duty factor TeV gamma-ray observa-tory is essential for studying TeV astr...
Abstract: Gamma-ray bursts (GRBs) have been detected up to GeV energies and are predicted by many mo...
Milagrito, a detector sensitive to gamma-rays at TeV energies, monitored the northern sky during the...
Milagrito, a detector sensitive to very high energy gamma rays, monitored the northern sky from 1997...
Abstract. The Milagro detector surveyed the sky almost continuously in the very high energy regime f...
The Milagro gamma-ray observatory employs a water Cherenkov detector to observe extensive air shower...
Milagro is a wide field (2 sr) high duty cycle (>90%) ground-based water Cherenkov detector designed...
Milagro is a water-Cherenkov detector that observes the extended air showers produced by cosmic gamm...
The Milagro telescope monitors the northern sky for 100 GeV - 100 TeV transient emission through con...
The Milagro gamma-ray observatory employs a water Cherenkov detector to observe extensive air shower...
The Milagrito water Cherenkov telescope operated for over a year. The most probable gamma-ray energy...
The Milagro Gamma-Ray Observatory employs a water Cerenkov detector to observe extensive air showers...
The Milagro Gamma-Ray Observatory, located at an altitude of 2630m in the mountains of northern New ...
discovered one of the brightest gamma-ray bursts ever recorded. With a peak visual magnitude of 5.3,...
Milagrito, a large, covered water-Cherenkov detector, was the world\u27s rst air-shower-particle de...
A wide field of view, high duty factor TeV gamma-ray observa-tory is essential for studying TeV astr...
Abstract: Gamma-ray bursts (GRBs) have been detected up to GeV energies and are predicted by many mo...