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Instrumented Water Tanks can Improve Air Shower Detector Sensitivity
R. Atkins, W. Benbow, D. Berley +40
Previous works have shown that water Cherenkov detectors have superior sensitivity to those of scintillation counters as applied to detecting extensive air showers (EAS). This is i…
Calibration of the Milagro Cosmic Ray Telescope
R. Atkins, W. Benbow, D. Berley +40
The Milagro detector is an air shower array which uses the water Cherenkov technique and is capable of continuously monitoring the sky at energies near 1 TeV. The detector consists…
Study of the Shadows of the Moon and the Sun with VHE Cosmic Rays
R. Atkins, W. Benbow, D. Berley +40
Milagrito, a prototype for the Milagro detector, operated for 15 months in 1997-8 and collected 8.9 billion events. It was the first extensive air shower (EAS) array sensitive to s…
Search for Short Duration Bursts of TeV Gamma Rays with the Milagrito Telescope
R. Atkins, W. Benbow, D. Berley +40
The Milagrito water Cherenkov telescope operated for over a year. The most probable gamma-ray energy was ~1 TeV and the trigger rate was as high as 400 Hz. We have developed an eff…
Search for a TeV Component of GRBs using the Milagrito Detector
R. Atkins, W. Benbow, D. Berley +40
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 Milag…
Milagrito Detection of TeV Emission from Mrk 501
R. Atkins, W. Benbow, D. Berley +40
The Milagro water Cherenkov detector near Los Alamos, New Mexico, has been operated as a sky monitor at energies of a few TeV between February 1997 and April 1998. Serving as a tes…