Toward Ultra Short Gamma Ray Burst Ground Based Detection, SGARFACE status

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dc.creatorLeBohec, Stephan
dc.creatorKrennrich, Frank
dc.creatorSleege, Gary
dc.date2002-12-11
dc.date.accessioned2026-07-07T02:06:50Z
dc.date.available2026-07-07T02:06:50Z
dc.descriptionWe present the status and motivation of the Short GAmma Ray Front Air Cherenkov Experiment (SGARFACE) which will be operated parallel to standard Very High Energy gamma-ray observations using the Whipple 10m telescope. SGARFACE is sensitive to 100MeV-10GeV gamma-ray bursts with durations ranging from 100ns to 100us providing a fluence sensitivity as low as few $\rm 1E-9 erg/cm^2. Preliminary data taking started in November 2002.
dc.descriptionThe Universe Viewed in Gamma-Rays Proceedings
dc.identifierhttps://arxiv.org/abs/astro-ph/0212267
dc.identifierhttp://arxiv.org/abs/astro-ph/0212267
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/5502
dc.subjectAstrophysics
dc.titleToward Ultra Short Gamma Ray Burst Ground Based Detection, SGARFACE status
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