Gamma-ray Burst Follow-up Observations With Stacee

Details Gamma-ray Burst Follow-up Observations With Stacee Gamma-ray Burst Follow-up Observations With Stacee

Sep 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006head....9.1320j&link_type=abstract

American Astronomical Society, HEAD meeting #9, #13.20; Bulletin of the American Astronomical Society, Vol. 38, p.369

Astronomy and Astrophysics

Astronomy

Scientific paper

STACEE is an atmospheric Cherenkov telescope that is sensitive to gamma rays above approximately 100 GeV. The relatively low energy threshold of STACEE is particularly advantageous for observations of gamma-ray bursts (GRBs), which typically have large redshifts. As of July 2006, follow-up observations with STACEE have been carried out for 18 bursts. Observations of GRB 050607 began 191 seconds after the Swift trigger and response times under 100 seconds are now possible. We will present the latest results on the search for very high-energy emission from GRBs with STACEE.

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