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Search for point sources of high-energy neutrinos with AMANDA
The Astrophysical Journal 583:1040-1057; February 1, 2003
Handle: Document-17256
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Friday, October 14, 2005 02:39:31 PM CDT
Tuesday, April 3, 2007 05:49:17 PM CDT
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  • The curves do not include the normalization uncertainty, possibly 30% in magnitude (Gaisser 2002; T.
  • K.
  • Gaisser 2002, private communication).
  • ein the point-source analysis is only 0.3% of ? Approximately 85% of OMs remained after deselection.
  • The specific value for each cut after stage 2 was chosen to retain e80% of the signal.
  • 7, atmospheric neutrinos contribute about 25% of the events to the simulated background). For a zenith (declination) offset of 1=5, 6% of the signal events are shifted to the neighboring bin.
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