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Results from the AMANDA neutrino telescope
Nuclear Physics B (Proc. Suppl.) 136 (85-92): 2004
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Friday, October 14, 2005 03:08:08 PM CDT
Tuesday, April 3, 2007 05:49:41 PM CDT
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  • 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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Preferred Version: Results from the AMANDA neutrino telescope