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The flux used in our calculation was provided by T. Stanev.
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Three-neutrino fits to atmospheric data without explicit L/E dependence were made by S.M. Bilenky, C. Giunti, C.W. Kim, Astropart. Phys. 4 (1996) 241, A. Joshipura, P. Krastev, Phys. Rev. D50 (1994) 3484, G.L. Fogli, E. Lisi, D. Montanino, G. Scosia, Phys. Rev. D55 (1997) 4385, G.L. Fogli, E. Lisi, A. Marrone, D. Montanino, Phys. Lett. B 425 (1998) 341, H. Minakata, O. Yasuda, Nucl. Phys. B 523 (1998) 597, S.M. Bilenky, C. Giuinti, hep-ph/9802201, O. Yasuda, hep- ph/9804400, R. Barbieri, L.J. Hall, D. Smith, A. Strumia, N. Weiner, hep-ph/9807235.
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Three-neutrino fits to atmospheric data without explicit L/E dependence were made by S.M. Bilenky, C. Giunti, C.W. Kim, Astropart. Phys. 4 (1996) 241, A. Joshipura, P. Krastev, Phys. Rev. D50 (1994) 3484, G.L. Fogli, E. Lisi, D. Montanino, G. Scosia, Phys. Rev. D55 (1997) 4385, G.L. Fogli, E. Lisi, A. Marrone, D. Montanino, Phys. Lett. B 425 (1998) 341, H. Minakata, O. Yasuda, Nucl. Phys. B 523 (1998) 597, S.M. Bilenky, C. Giuinti, hep-ph/9802201, O. Yasuda, hep- ph/9804400, R. Barbieri, L.J. Hall, D. Smith, A. Strumia, N. Weiner, hep-ph/9807235.
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Three-neutrino fits to atmospheric data without explicit L/E dependence were made by S.M. Bilenky, C. Giunti, C.W. Kim, Astropart. Phys. 4 (1996) 241, A. Joshipura, P. Krastev, Phys. Rev. D50 (1994) 3484, G.L. Fogli, E. Lisi, D. Montanino, G. Scosia, Phys. Rev. D55 (1997) 4385, G.L. Fogli, E. Lisi, A. Marrone, D. Montanino, Phys. Lett. B 425 (1998) 341, H. Minakata, O. Yasuda, Nucl. Phys. B 523 (1998) 597, S.M. Bilenky, C. Giuinti, hep-ph/9802201, O. Yasuda, hep- ph/9804400, R. Barbieri, L.J. Hall, D. Smith, A. Strumia, N. Weiner, hep-ph/9807235.
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Three-neutrino fits to atmospheric data without explicit L/E dependence were made by S.M. Bilenky, C. Giunti, C.W. Kim, Astropart. Phys. 4 (1996) 241, A. Joshipura, P. Krastev, Phys. Rev. D50 (1994) 3484, G.L. Fogli, E. Lisi, D. Montanino, G. Scosia, Phys. Rev. D55 (1997) 4385, G.L. Fogli, E. Lisi, A. Marrone, D. Montanino, Phys. Lett. B 425 (1998) 341, H. Minakata, O. Yasuda, Nucl. Phys. B 523 (1998) 597, S.M. Bilenky, C. Giuinti, hep-ph/9802201, O. Yasuda, hep- ph/9804400, R. Barbieri, L.J. Hall, D. Smith, A. Strumia, N. Weiner, hep-ph/9807235.
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Three-neutrino fits to atmospheric data without explicit L/E dependence were made by S.M. Bilenky, C. Giunti, C.W. Kim, Astropart. Phys. 4 (1996) 241, A. Joshipura, P. Krastev, Phys. Rev. D50 (1994) 3484, G.L. Fogli, E. Lisi, D. Montanino, G. Scosia, Phys. Rev. D55 (1997) 4385, G.L. Fogli, E. Lisi, A. Marrone, D. Montanino, Phys. Lett. B 425 (1998) 341, H. Minakata, O. Yasuda, Nucl. Phys. B 523 (1998) 597, S.M. Bilenky, C. Giuinti, hep-ph/9802201, O. Yasuda, hep- ph/9804400, R. Barbieri, L.J. Hall, D. Smith, A. Strumia, N. Weiner, hep-ph/9807235.
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Three-neutrino fits to atmospheric data without explicit L/E dependence were made by S.M. Bilenky, C. Giunti, C.W. Kim, Astropart. Phys. 4 (1996) 241, A. Joshipura, P. Krastev, Phys. Rev. D50 (1994) 3484, G.L. Fogli, E. Lisi, D. Montanino, G. Scosia, Phys. Rev. D55 (1997) 4385, G.L. Fogli, E. Lisi, A. Marrone, D. Montanino, Phys. Lett. B 425 (1998) 341, H. Minakata, O. Yasuda, Nucl. Phys. B 523 (1998) 597, S.M. Bilenky, C. Giuinti, hep-ph/9802201, O. Yasuda, hep-ph/9804400, R. Barbieri, L.J. Hall, D. Smith, A. Strumia, N. Weiner, hep-ph/9807235.
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Three-neutrino fits to atmospheric data without explicit L/E dependence were made by S.M. Bilenky, C. Giunti, C.W. Kim, Astropart. Phys. 4 (1996) 241, A. Joshipura, P. Krastev, Phys. Rev. D50 (1994) 3484, G.L. Fogli, E. Lisi, D. Montanino, G. Scosia, Phys. Rev. D55 (1997) 4385, G.L. Fogli, E. Lisi, A. Marrone, D. Montanino, Phys. Lett. B 425 (1998) 341, H. Minakata, O. Yasuda, Nucl. Phys. B 523 (1998) 597, S.M. Bilenky, C. Giuinti, hep-ph/9802201, O. Yasuda, hep- ph/9804400, R. Barbieri, L.J. Hall, D. Smith, A. Strumia, N. Weiner, hep-ph/9807235.
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Osland, P.1
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