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SUMMARY:Observations of the Draco Dwarf Spheroidal Galaxy with STACEE
DTSTART;VALUE=DATE-TIME:20070706T194500Z
DTEND;VALUE=DATE-TIME:20070706T194500Z
DTSTAMP;VALUE=DATE-TIME:20260721T072651Z
UID:indico-contribution-1076@cern.ch
DESCRIPTION:Speakers: COVAULT\, C. E. (Department of Physics\, Case Wester
 n Reserve University\, Cleveland\, OH 44106 USA)\nThe Draco dwarf spheroid
 al galaxy has garnered interest as a possible source for the\nindirect det
 ection of dark matter.  Draco has a large mass-to-light ratio\, and its\nr
 elative proximity to the Earth provides favorable conditions for the produ
 ction of\ndetectable gamma-rays from dark matter self-annihilation in the 
 galaxy's core.  The\nSolar Tower Atmospheric Cherenkov Effect Experiment (
 STACEE) is an air-shower\nCherenkov telescope located in Albuquerque\, NM 
 capable of detecting gamma-rays with\nan energy threshold of about 250 GeV
  for this source. We present the results of the\nSTACEE observations of Dr
 aco during the 2005-2006 observing season totaling\napproximately 10 hours
  of livetime after cuts.\n\nhttps://indico.nucleares.unam.mx/event/4/sessi
 on/39/contribution/1076
LOCATION:Merida\, Mexico Regency (Hyatt)
URL:https://indico.nucleares.unam.mx/event/4/session/39/contribution/1076
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