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SUMMARY:Gamma-Ray Burst Follow-up Observations with STACEE During 2003-200
 7
DTSTART;VALUE=DATE-TIME:20070709T175300Z
DTEND;VALUE=DATE-TIME:20070709T180500Z
DTSTAMP;VALUE=DATE-TIME:20261008T122416Z
UID:indico-contribution-409@cern.ch
DESCRIPTION:Speakers: JARVIS\, Alexander (University of California\, Los A
 ngeles\, Los Angeles\, CA 90095)\nThe Solar Tower Atmospheric Cherenkov Ef
 fect Experiment (STACEE) is an atmospheric\nCherenkov telescope that uses 
 a large mirror array to achieve a relatively low energy\nthreshold.  For s
 ources with Crab-like spectra\, at high elevations\, the detector\nrespons
 e peaks near 100 GeV.  Gamma-ray burst (GRB) observations have been a high
 \npriority for the STACEE collaboration since the inception of the experim
 ent.  We\npresent the results of 20 GRB follow-up observations ranging fro
 m 3 minutes to 15\nhours after the burst triggers.  Where redshift measure
 ments are available\, we place\nconstraints on the intrinsic high-energy s
 pectra of the bursts.\n\nhttps://indico.nucleares.unam.mx/event/4/session/
 98/contribution/409
LOCATION:Merida\, Mexico Uxmal + Tulum (Holiday Inn)
URL:https://indico.nucleares.unam.mx/event/4/session/98/contribution/409
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