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Title:	Search for point sources of high-energy neutrinos with AMANDA
Abstract:	The Astrophysical Journal 583:1040-1057; February 1, 2003
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Handle:	Document-17256
Owner:	Site Administrator (User-2, admin:DocuShare)^DS
Create Date:	Friday, October 14, 2005 02:39:31 PM CDT
Modified Date:	Tuesday, April 3, 2007 05:49:17 PM CDT
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Abstract:	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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File name:	PtSrc2003.56513.web.pdf
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Appears In:	2004
Preferred Version:	Search for point sources of high-energy neutrinos with AMANDA