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Title:	Sensitivity of the IceCube detector to astrophysical sources of high energy muon nuetrinos
Abstract:	Astroparticle Physics 20(507-532): 2004
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Handle:	Document-17265
Owner:	Site Administrator (User-2, admin:DocuShare)^DS
Create Date:	Friday, October 14, 2005 03:06:46 PM CDT
Modified Date:	Tuesday, April 3, 2007 05:49:42 PM CDT
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Abstract:	1GeV at a 5r significance, or, in the absence of a signal, place a 90% c.l. limit at a level of E2 m? Integrating the fitted density functions over the full solid angle shows that the narrower Gaussian accounts for about 44% of the event statistics, the broader Gaussian accounts for 40%, and roughly 16% of the events lie in the tail of the distribution where the track density is not described by a double Gaussian. / Astroparticle Physics 20 (2004) 507 532 5r significance, but we can find the signal strength such that the probability of P5r is close to certainty, e.g., 70%, 90% or 99%. 1sr?1GeV, and the corresponding 90% c.l. average upper limit (dotted), as a function of a cut in channel ...
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File name:	scienceSensitivity.pdf
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Appears In:	2005
Preferred Version:	Sensitivity of the IceCube detector to astrophysical sources of high energy muon nuetrinos