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Studies of Air Showers above 10^18 eV with the CHICOS Array
T. W. Lynn, E. Brobeck, B. E. Carlson +10
CHICOS (California HIgh school Cosmic ray ObServatory) is presently an array of more than 140 detectors distributed over a large area (~400 km^2) of southern California, and will c…
Search for Correlated High Energy Cosmic Ray Events with CHICOS
R. D. McKeown, B. E. Carlson, E. Brobeck +8
We present the results of a search for time correlations in high energy cosmic ray data (primary E > 10^14 eV) collected by the California HIgh school Cosmic ray ObServatory (CHICO…
Evidence for TeV Emission from GRB 970417a
The Milagro Collaboration, R. Atkins, W. Benbow +37
Milagrito, a detector sensitive to very high energy gamma rays, monitored the northern sky from February 1997 through May 1998. With a large field of view and a high duty cycle, th…
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…