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DeMuth, D; Alner, G.J; Ayres, D; Barrett, W.L; Border, P; Cockerill, D.J.A; Cobb, J.H; Courant, H; Fields, T; Gallagher, H; Goodman, M.C; Gran, R; Joffe-Minor, T; Kafka, T; Kasahara, S; Litchfield, P.J; Mann, W.A; Marshak, M; Milburn, R; Miller, W; Mualem, L; Napier, A; Oliver, W; Pearce, G.F; Peterson, E; Petyt, D; Ruddick, K; Sanchez, M; Schneps, J; Sousa, A; Speakman, B; Thron, J; Trost, H.J; Uretsky, J; Villaume, G; West, N
Astroparticle physics, 02/2004, Letnik: 20, Številka: 5Journal Article
We measure the horizontal (|cos( θ z )|<0.14 corresponding to a slant depth cut 14 kmwe) neutrino-induced muon flux ( E μ>1.8 GeV) in Soudan 2 to be 4.01 ± 0.50 ± 0.30 × 10 −13 cm −2 sr −1 s −1. From the absence of horizontal muons with large energy loss, we set a limit on the flux of muon neutrinos from active galactic nuclei.
