Abstract
The Short GAmma Ray Front Air Cherenkov Experiment (SGARFACE) is designed to search for bursts of γ rays above 200 MeV lasting from 1 ns to 16 μs. The custom-designed trigger and dataacquisition system is coupled to the camera on the Whipple 10m telescope, an air-Cherenkov telescope in southern Arizona. The experiment has operated for more than 3 years during which time about 1 million events were recorded. Rejection of the cosmic-ray background and of atmospheric phenomena is accomplished through time-resolved imaging of the recorded Cherenkov light. Potential sources of bursts of γ rays are the final explosion of primordial black holes within about 200 pc and γ-ray emission accompanying giant radio pulses. Results of the search for explosions of primordial black holes will be given in a future publication.
Original language | English (US) |
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Pages | 783-786 |
Number of pages | 4 |
State | Published - 2007 |
Event | 30th International Cosmic Ray Conference, ICRC 2007 - Merida, Yucatan, Mexico Duration: Jul 3 2007 → Jul 11 2007 |
Other
Other | 30th International Cosmic Ray Conference, ICRC 2007 |
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Country/Territory | Mexico |
City | Merida, Yucatan |
Period | 7/3/07 → 7/11/07 |
All Science Journal Classification (ASJC) codes
- Nuclear and High Energy Physics