| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 10700350 | Astroparticle Physics | 2005 | 14 Pages |
Abstract
The Short GAmma Ray Front Air Cherenkov Experiment (SGARFACE) is operated at the Whipple Observatory utilizing the Whipple 10 m γ-ray telescope. SGARFACE is sensitive to γ-ray bursts of more than 100 MeV with durations from 100 ns to 35 μs and provides a fluence sensitivity as low as 0.8 γ-rays/m2 above 200 MeV (0.05 γ-rays/m2 above 2 GeV) and allows to record the burst time structure.
Related Topics
Physical Sciences and Engineering
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Astronomy and Astrophysics
Authors
S. LeBohec, F. Krennrich, G. Sleege,