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Title:	Results from the AMANDA neutrino telescope
Abstract:	Nuclear Physics B (Proc. Suppl.) 136 (85-92): 2004
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Handle:	Document-17266
Owner:	Site Administrator (User-2, admin:DocuShare)^DS
Create Date:	Friday, October 14, 2005 03:08:08 PM CDT
Modified Date:	Tuesday, April 3, 2007 05:49:41 PM CDT
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Abstract:	For this same reason, the energy resolution (correlated to the total light detected) is better for cascades, ?(log E)? 15% than for muon tracks, ?(log E)? 40%. For most of the analyses presented in this summary, the systematic uncertainties amount to ?25%. Including the systematic uncertainties this leads to a 90% CL flux limit on an E?2 ?spectrum in the region 3 TeV to 6 PeV of E2 ? This leads to a 90% CL limit on the diffuse flux of neutrinos from all flavors in the region 50 TeV to 5 PeV of E2 ? liminary 90% CL limit of E2 ? The estimated systematic uncertainties for this analysis are at the level of 30%.
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Appears In:	2005
Preferred Version:	Results from the AMANDA neutrino telescope