Fabrice Jouvenot University of Liverpool The 3 rd of February 2006 Calculus principle Detection probability Getting probability NlNl Number of events b Probability (N obs > N l ) < 1% If theres only background b+s Detection probability estimatedobserved Detection probability Introduction The Galaxy Galactic Neutrinos ANTARESSensitivityKm3Conclusion years Detection probability Cut on log of the reconstructed energy log[GeV]
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