Publications of Christopher Walter    :chronological  alphabetical  combined listing:

%% Books   
@inbook{SK-Chapter,
   Author = {Walter, CW},
   Title = {The super-kamiokande experiment},
   Pages = {19-43},
   Booktitle = {Neutrino Oscillations: Present Status and Future
             Plans},
   Publisher = {World Scientific Publishing Company},
   Editor = {J. Thomas and P. Vahle},
   Chapter = {The Super-Kamiokande Experiment},
   Year = {2008},
   Month = {January},
   ISBN = {9789812771971},
   url = {http://arxiv.org/abs/0802.1041},
   Abstract = {© 2008 by World Scientific Publishing Co. Pte. Ltd. All
             rights reserved. Super-Kamiokande is a 50 kiloton water
             Cherenkov detector located at the Kamioka Observatory of the
             Institute for Cosmic Ray Research, University of Tokyo. It
             was designed to study neutrino oscillations and carry out
             searches for the decay of the nucleon. The Super-Kamiokande
             experiment began in 1996 and in the ensuing 10 years of
             running has produced extremely important results in the
             fields of atmospheric and solar neutrino oscillations.
             Furthermore, it has set stringent limits on the decay of the
             nucleon and the existence of dark matter and astrophysical
             sources of neutrinos. Perhaps most crucially,
             Super-Kamiokande was the first to definitively show that
             neutrinos have mass and undergo flavor oscillations. This
             chapter will summarize the published scientific output of
             the experiment with a particular emphasis on the atmospheric
             neutrino results.},
   Doi = {10.1142/9789812771971_0002},
   Key = {SK-Chapter}
}


%% Papers Published   
@article{fds329105,
   Author = {Abe, K and Amey, J and Andreopoulos, C and Antonova, M and Aoki, S and Ariga, A and Ashida, Y and Ban, S and Barbi, M and Barker, GJ and Barr, G and Barry, C and Batkiewicz, M and Berardi, V and Berkman, S and Bhadra, S and Bienstock, S and Blondel, A and Bolognesi, S and Bordoni, S and Boyd,
             SB and Brailsford, D and Bravar, A and Bronner, C and Buizza Avanzini,
             M and Calland, RG and Campbell, T and Cao, S and Cartwright, SL and Catanesi, MG and Cervera, A and Chappell, A and Checchia, C and Cherdack, D and Chikuma, N and Christodoulou, G and Coleman, J and Collazuol, G and Coplowe, D and Cudd, A et al.},
   Title = {Measurement of and charged current inclusive cross sections
             and their ratio with the T2K off-axis near
             detector},
   Journal = {Physical Review D},
   Volume = {96},
   Number = {5},
   Year = {2017},
   Month = {September},
   url = {http://dx.doi.org/10.1103/PhysRevD.96.052001},
   Doi = {10.1103/PhysRevD.96.052001},
   Key = {fds329105}
}

@article{fds328442,
   Author = {Abe, K and Bronner, C and Pronost, G and Hayato, Y and Ikeda, M and Iyogi,
             K and Kameda, J and Kato, Y and Kishimoto, Y and Marti, L and Miura, M and Moriyama, S and Nakahata, M and Nakano, Y and Nakayama, S and Okajima,
             Y and Orii, A and Sekiya, H and Shiozawa, M and Sonoda, Y and Takeda, A and Takenaka, A and Tanaka, H and Tasaka, S and Tomura, T and Akutsu, R and Kajita, T and Kaneyuki, K and Nishimura, Y and Okumura, K and Tsui, KM and Labarga, L and Fernandez, P and Blaszczyk, FDM and Gustafson, J and Kachulis, C and Kearns, E and Raaf, JL and Stone, JL and Sulak, LR and Berkman, S and Tobayama, S et al.},
   Title = {Search for nucleon decay into charged antilepton plus meson
             in exposure of the Super-Kamiokande water Cherenkov
             detector},
   Journal = {Physical Review D},
   Volume = {96},
   Number = {1},
   Year = {2017},
   Month = {July},
   url = {http://dx.doi.org/10.1103/PhysRevD.96.012003},
   Doi = {10.1103/PhysRevD.96.012003},
   Key = {fds328442}
}

@article{fds328443,
   Author = {Abe, K and Amey, J and Andreopoulos, C and Antonova, M and Aoki, S and Ariga, A and Ashida, Y and Autiero, D and Ban, S and Barbi, M and Barker,
             GJ and Barr, G and Barry, C and Bartet-Friburg, P and Batkiewicz, M and Berardi, V and Berkman, S and Bhadra, S and Bienstock, S and Blondel, A and Bolognesi, S and Bordoni, S and Boyd, SB and Brailsford, D and Bravar,
             A and Bronner, C and Buizza Avanzini and M and Calland, RG and Campbell, T and Cao, S and Cartwright, SL and Catanesi, MG and Cervera, A and Chappell,
             A and Checchia, C and Cherdack, D and Chikuma, N and Christodoulou, G and Clifton, A and Coleman, J et al.},
   Title = {Updated T2K measurements of muon neutrino and antineutrino
             disappearance using protons on target},
   Journal = {Physical Review D},
   Volume = {96},
   Number = {1},
   Year = {2017},
   Month = {July},
   url = {http://dx.doi.org/10.1103/PhysRevD.96.011102},
   Doi = {10.1103/PhysRevD.96.011102},
   Key = {fds328443}
}

@article{fds327380,
   Author = {Abe, K and Amey, J and Andreopoulos, C and Antonova, M and Aoki, S and Ariga, A and Assylbekov, S and Autiero, D and Ban, S and Barbato, FCT and Barbi, M and Barker, GJ and Barr, G and Barry, C and Bartet-Friburg, P and Batkiewicz, M and Berardi, V and Berkman, S and Bhadra, S and Bienstock,
             S and Blondel, A and Bolognesi, S and Bordoni, S and Boyd, SB and Brailsford, D and Bravar, A and Bronner, C and Buizza Avanzini and M and Calland, RG and Campbell, T and Cao, S and Cartwright, SL and Castillo,
             R and Catanesi, MG and Cervera, A and Chappell, A and Checchia, C and Cherdack, D and Chikuma, N et al.},
   Title = {Search for Lorentz and violation using sidereal time
             dependence of neutrino flavor transitions over a short
             baseline},
   Journal = {Physical Review D},
   Volume = {95},
   Number = {11},
   Year = {2017},
   Month = {June},
   url = {http://dx.doi.org/10.1103/PhysRevD.95.111101},
   Doi = {10.1103/PhysRevD.95.111101},
   Key = {fds327380}
}

@article{fds326461,
   Author = {Abe, K and Amey, J and Andreopoulos, C and Antonova, M and Aoki, S and Ariga, A and Autiero, D and Ban, S and Barbi, M and Barker, GJ and Barr, G and Barry, C and Bartet-Friburg, P and Batkiewicz, M and Berardi, V and Berkman, S and Bhadra, S and Bienstock, S and Blondel, A and Bolognesi,
             S and Bordoni, S and Boyd, SB and Brailsford, D and Bravar, A and Bronner,
             C and Buizza Avanzini and M and Calland, RG and Campbell, T and Cao, S and Cartwright, SL and Catanesi, MG and Cervera, A and Checchia, C and Cherdack, D and Chikuma, N and Christodoulou, G and Clifton, A and Coleman, J and Collazuol, G and Coplowe, D et al.},
   Title = {Combined Analysis of Neutrino and Antineutrino Oscillations
             at T2K.},
   Journal = {Physical Review Letters},
   Volume = {118},
   Number = {15},
   Pages = {151801},
   Year = {2017},
   Month = {April},
   url = {http://dx.doi.org/10.1103/physrevlett.118.151801},
   Abstract = {T2K reports its first results in the search for CP violation
             in neutrino oscillations using appearance and disappearance
             channels for neutrino- and antineutrino-mode beams. The data
             include all runs from January 2010 to May 2016 and comprise
             7.482×10^{20} protons on target in neutrino mode, which
             yielded in the far detector 32 e-like and 135  μ-like
             events, and 7.471×10^{20} protons on target in antineutrino
             mode, which yielded 4 e-like and 66  μ-like events.
             Reactor measurements of sin^{2}2θ_{13} have been used as an
             additional constraint. The one-dimensional confidence
             interval at 90% for the phase δ_{CP} spans the range
             (-3.13, -0.39) for normal mass ordering. The CP conservation
             hypothesis (δ_{CP}=0, π) is excluded at
             90% C.L.},
   Doi = {10.1103/physrevlett.118.151801},
   Key = {fds326461}
}

@article{fds326487,
   Author = {Abe, K and Haga, Y and Hayato, Y and Ikeda, M and Iyogi, K and Kameda, J and Kishimoto, Y and Miura, M and Moriyama, S and Nakahata, M and Nakajima,
             T and Nakano, Y and Nakayama, S and Orii, A and Sekiya, H and Shiozawa, M and Takeda, A and Tanaka, H and Tomura, T and Wendell, RA and Akutsu, R and Irvine, T and Kajita, T and Kaneyuki, K and Nishimura, Y and Richard, E and Okumura, K and Labarga, L and Fernandez, P and Gustafson, J and Kachulis, C and Kearns, E and Raaf, JL and Stone, JL and Sulak, LR and Berkman, S and Nantais, CM and Tanaka, HA and Tobayama, S and Goldhaber,
             M and Kropp, WR and Mine, S et al.},
   Title = {Search for proton decay via and in exposure of the
             Super-Kamiokande water Cherenkov detector},
   Journal = {Physical Review D},
   Volume = {95},
   Number = {1},
   Year = {2017},
   Month = {January},
   url = {http://dx.doi.org/10.1103/PhysRevD.95.012004},
   Doi = {10.1103/PhysRevD.95.012004},
   Key = {fds326487}
}

@article{fds326462,
   Author = {Abe, K and Andreopoulos, C and Antonova, M and Aoki, S and Ariga, A and Assylbekov, S and Autiero, D and Ban, S and Barbi, M and Barker, GJ and Barr, G and Bartet-Friburg, P and Batkiewicz, M and Bay, F and Berardi,
             V and Berkman, S and Bhadra, S and Bienstock, S and Blondel, A and Bolognesi, S and Bordoni, S and Boyd, SB and Brailsford, D and Bravar,
             A and Bronner, C and Buizza Avanzini and M and Calland, RG and Campbell, T and Cao, S and Caravaca Rodríguez and J and Cartwright, SL and Castillo, R and Catanesi, MG and Cervera, A and Cherdack, D and Chikuma, N and Christodoulou, G and Clifton, A and Coleman, J et
             al.},
   Title = {First measurement of the muon neutrino charged current
             single pion production cross section on water with the T2K
             near detector},
   Journal = {Physical Review D},
   Volume = {95},
   Number = {1},
   Year = {2017},
   Month = {January},
   url = {http://dx.doi.org/10.1103/PhysRevD.95.012010},
   Doi = {10.1103/PhysRevD.95.012010},
   Key = {fds326462}
}

@article{fds326463,
   Author = {Abe, K and Andreopoulos, C and Antonova, M and Aoki, S and Ariga, A and Assylbekov, S and Autiero, D and Ban, S and Barbi, M and Barker, GJ and Barr, G and Bartet-Friburg, P and Batkiewicz, M and Bay, F and Berardi,
             V and Berkman, S and Bhadra, S and Blondel, A and Bolognesi, S and Bordoni,
             S and Boyd, SB and Brailsford, D and Bravar, A and Bronner, C and Buizza
             Avanzini, M and Calland, RG and Campbell, T and Cao, S and Caravaca
             Rodríguez, J and Cartwright, SL and Castillo, R and Catanesi, MG and Cervera, A and Cherdack, D and Chikuma, N and Christodoulou, G and Clifton, A and Coleman, J and Collazuol, G et al.},
   Title = {Measurement of Coherent π^{+} Production in Low Energy
             Neutrino-Carbon Scattering.},
   Journal = {Physical Review Letters},
   Volume = {117},
   Number = {19},
   Pages = {192501},
   Year = {2016},
   Month = {November},
   url = {http://dx.doi.org/10.1103/physrevlett.117.192501},
   Abstract = {We report the first measurement of the flux-averaged cross
             section for charged current coherent π^{+} production on
             carbon for neutrino energies less than 1.5 GeV, and with a
             restriction on the final state phase space volume in the T2K
             near detector, ND280. Comparisons are made with predictions
             from the Rein-Sehgal coherent production model and the model
             by Alvarez-Ruso et al., the latter representing the first
             implementation of an instance of the new class of
             microscopic coherent models in a neutrino interaction
             Monte Carlo event generator. We observe a clear event
             excess above background, disagreeing with the null results
             reported by K2K and SciBooNE in a similar neutrino energy
             region. The measured flux-averaged cross sections are below
             those predicted by both the Rein-Sehgal and Alvarez-Ruso
             et al.},
   Doi = {10.1103/physrevlett.117.192501},
   Key = {fds326463}
}

@article{fds326464,
   Author = {Abe, K and Haga, K and Hayato, Y and Ikeda, M and Iyogi, K and Kameda, J and Kishimoto, Y and Miura, M and Moriyama, S and Nakahata, M and Nakajima,
             T and Nakano, Y and Nakayama, S and Orii, A and Sekiya, H and Shiozawa, M and Takeda, A and Tanaka, H and Tasaka, S and Tomura, T and Akutsu, R and Kajita, T and Kaneyuki, K and Nishimura, Y and Richard, E and Okumura,
             K and Labarga, L and Fernandez, P and Blaszczyk, FDM and Gustafson, J and Kachulis, C and Kearns, E and Raaf, JL and Stone, JL and Sulak, LR and Berkman, S and Nantais, CM and Tobayama, S and Goldhaber, M and Kropp,
             WR and Mine, S and Weatherly, P et al.},
   Title = {SEARCH FOR NEUTRINOS IN SUPER-KAMIOKANDE ASSOCIATED WITH
             GRAVITATIONAL-WAVE EVENTS GW150914 AND GW151226},
   Journal = {Astrophysical Journal Letters},
   Volume = {830},
   Number = {1},
   Pages = {L11-L11},
   Year = {2016},
   Month = {October},
   url = {http://dx.doi.org/10.3847/2041-8205/830/1/L11},
   Doi = {10.3847/2041-8205/830/1/L11},
   Key = {fds326464}
}

@article{fds326488,
   Author = {Olive, KA},
   Title = {Review of Particle Physics},
   Journal = {Chinese Physics C},
   Volume = {40},
   Number = {10},
   Pages = {100001-100001},
   Year = {2016},
   Month = {October},
   url = {http://dx.doi.org/10.1088/1674-1137/40/10/100001},
   Doi = {10.1088/1674-1137/40/10/100001},
   Key = {fds326488}
}

@article{fds326465,
   Author = {Richard, E and Okumura, K and Abe, K and Haga, Y and Hayato, Y and Ikeda,
             M and Iyogi, K and Kameda, J and Kishimoto, Y and Miura, M and Moriyama, S and Nakahata, M and Nakajima, T and Nakano, Y and Nakayama, S and Orii, A and Sekiya, H and Shiozawa, M and Takeda, A and Tanaka, H and Tomura, T and Wendell, RA and Akutsu, R and Irvine, T and Kajita, T and Kaneyuki, K and Nishimura, Y and Labarga, L and Fernandez, P and Gustafson, J and Kachulis, C and Kearns, E and Raaf, JL and Stone, JL and Sulak, LR and Berkman, S and Nantais, CM and Tanaka, HA and Tobayama, S and Goldhaber,
             M and Kropp, WR and Mine, S et al.},
   Title = {Measurements of the atmospheric neutrino flux by
             Super-Kamiokande: Energy spectra, geomagnetic effects, and
             solar modulation},
   Journal = {Physical Review D},
   Volume = {94},
   Number = {5},
   Year = {2016},
   Month = {September},
   url = {http://dx.doi.org/10.1103/PhysRevD.94.052001},
   Doi = {10.1103/PhysRevD.94.052001},
   Key = {fds326465}
}

@article{fds326466,
   Author = {Abe, K and Haga, Y and Hayato, Y and Ikeda, M and Iyogi, K and Kameda, J and Kishimoto, Y and Marti, L and Miura, M and Moriyama, S and Nakahata, M and Nakajima, T and Nakayama, S and Orii, A and Sekiya, H and Shiozawa, M and Sonoda, Y and Takeda, A and Tanaka, H and Takenaga, Y and Tasaka, S and Tomura, T and Ueno, K and Yokozawa, T and Akutsu, R and Irvine, T and Kaji,
             H and Kajita, T and Kametani, I and Kaneyuki, K and Lee, KP and Nishimura,
             Y and McLachlan, T and Okumura, K and Richard, E and Labarga, L and Fernandez, P and Blaszczyk, FDM and Gustafson, J and Kachulis, C and Kearns, E and Raaf, JL and Stone, JL et al.},
   Title = {Solar neutrino measurements in Super-Kamiokande-IV},
   Journal = {Physical Review D},
   Volume = {94},
   Number = {5},
   Year = {2016},
   Month = {September},
   url = {http://dx.doi.org/10.1103/PhysRevD.94.052010},
   Doi = {10.1103/PhysRevD.94.052010},
   Key = {fds326466}
}

@article{fds318482,
   Author = {Abe, K and Haga, Y and Hayato, Y and Ikeda, M and Iyogi, K and Kameda, J and Kishimoto, Y and Miura, M and Moriyama, S and Nakahata, M and Nakano, Y and Nakayama, S and Sekiya, H and Shiozawa, M and Suzuki, Y and Takeda, A and Tanaka, H and Tomura, T and Ueno, K and Wendell, RA and Yokozawa, T and Irvine, T and Kajita, T and Kametani, I and Kaneyuki, K and Lee, KP and McLachlan, T and Nishimura, Y and Richard, E and Okumura, K and Labarga,
             L and Fernandez, P and Berkman, S and Tanaka, HA and Tobayama, S and Gustafson, J and Kearns, E and Raaf, JL and Stone, JL and Sulak, LR and Goldhaber, M and Carminati, G et al.},
   Title = {Real-time supernova neutrino burst monitor at
             Super-Kamiokande},
   Journal = {Astroparticle Physics},
   Volume = {81},
   Pages = {39-48},
   Year = {2016},
   Month = {August},
   url = {http://dx.doi.org/10.1016/j.astropartphys.2016.04.003},
   Doi = {10.1016/j.astropartphys.2016.04.003},
   Key = {fds318482}
}

@article{fds318483,
   Author = {Abe, K and Andreopoulos, C and Antonova, M and Aoki, S and Ariga, A and Assylbekov, S and Autiero, D and Barbi, M and Barker, GJ and Barr, G and Bartet-Friburg, P and Batkiewicz, M and Berardi, V and Berkman, S and Bhadra, S and Blondel, A and Bolognesi, S and Bordoni, S and Boyd, SB and Brailsford, D and Bravar, A and Bronner, C and Buizza Avanzini and M and Calland, RG and Cao, S and Caravaca Rodríguez and J and Cartwright, SL and Castillo, R and Catanesi, MG and Cervera, A and Cherdack, D and Chikuma,
             N and Christodoulou, G and Clifton, A and Coleman, J and Collazuol, G and Cremonesi, L and Dabrowska, A et al.},
   Title = {Measurement of double-differential muon neutrino
             charged-current interactions on without pions in the final
             state using the T2K off-axis beam},
   Journal = {Physical Review D},
   Volume = {93},
   Number = {11},
   Year = {2016},
   Month = {June},
   url = {http://dx.doi.org/10.1103/PhysRevD.93.112012},
   Doi = {10.1103/PhysRevD.93.112012},
   Key = {fds318483}
}

@article{fds318484,
   Author = {Abe, K and Andreopoulos, C and Antonova, M and Aoki, S and Ariga, A and Assylbekov, S and Autiero, D and Barbi, M and Barker, GJ and Barr, G and Bartet-Friburg, P and Batkiewicz, M and Bay, F and Berardi, V and Berkman, S and Bhadra, S and Blondel, A and Bolognesi, S and Bordoni, S and Boyd, SB and Brailsford, D and Bravar, A and Bronner, C and Buizza
             Avanzini, M and Calland, RG and Cao, S and Caravaca Rodríguez and J and Cartwright, SL and Castillo, R and Catanesi, MG and Cervera, A and Cherdack, D and Chikuma, N and Christodoulou, G and Clifton, A and Coleman, J and Collazuol, G and Cremonesi, L et
             al.},
   Title = {Measurement of Muon Antineutrino Oscillations with an
             Accelerator-Produced Off-Axis Beam.},
   Journal = {Physical Review Letters},
   Volume = {116},
   Number = {18},
   Pages = {181801},
   Year = {2016},
   Month = {May},
   url = {http://dx.doi.org/10.1103/physrevlett.116.181801},
   Abstract = {T2K reports its first measurements of the parameters
             governing the disappearance of ν[over ¯]_{μ} in an
             off-axis beam due to flavor change induced by neutrino
             oscillations. The quasimonochromatic ν[over ¯]_{μ} beam,
             produced with a peak energy of 0.6 GeV at J-PARC, is
             observed at the far detector Super-Kamiokande, 295 km away,
             where the ν[over ¯]_{μ} survival probability is expected
             to be minimal. Using a data set corresponding to
             4.01×10^{20} protons on target, 34 fully contained μ-like
             events were observed. The best-fit oscillation parameters
             are sin^{2}(θ[over ¯]_{23})=0.45 and |Δm[over
             ¯]_{32}^{2}|=2.51×10^{-3}  eV^{2} with 68% confidence
             intervals of 0.38-0.64 and 2.26-2.80×10^{-3}  eV^{2},
             respectively. These results are in agreement with existing
             antineutrino parameter measurements and also with the
             ν_{μ} disappearance parameters measured by
             T2K.},
   Doi = {10.1103/physrevlett.116.181801},
   Key = {fds318484}
}

@article{fds318485,
   Author = {Abe, K and Andreopoulos, C and Antonova, M and Aoki, S and Ariga, A and Assylbekov, S and Autiero, D and Barbi, M and Barker, GJ and Barr, G and Bartet-Friburg, P and Batkiewicz, M and Bay, F and Berardi, V and Berkman, S and Bhadra, S and Blondel, A and Bolognesi, S and Bordoni, S and Boyd, SB and Brailsford, D and Bravar, A and Bronner, C and Calland, RG and Cao, S and Caravaca Rodríguez and J and Cartwright, SL and Castillo, R and Catanesi, MG and Cervera, A and Cherdack, D and Chikuma, N and Christodoulou, G and Clifton, A and Coleman, J and Collazuol, G and Cremonesi, L and Dabrowska, A and De Rosa and G et
             al.},
   Title = {Measurement of the muon neutrino inclusive charged-current
             cross section in the energy range of 1–3 GeV with the T2K
             INGRID detector},
   Journal = {Physical Review D},
   Volume = {93},
   Number = {7},
   Year = {2016},
   Month = {April},
   url = {http://dx.doi.org/10.1103/PhysRevD.93.072002},
   Doi = {10.1103/PhysRevD.93.072002},
   Key = {fds318485}
}

@article{fds318487,
   Author = {Abe, K and Adam, J and Aihara, H and Akiri, T and Andreopoulos, C and Aoki,
             S and Ariga, A and Assylbekov, S and Autiero, D and Barbi, M and Barker,
             GJ and Barr, G and Bartet-Friburg, P and Bass, M and Batkiewicz, M and Bay,
             F and Berardi, V and Berger, BE and Berkman, S and Bhadra, S and Blaszczyk,
             FDM and Blondel, A and Bojechko, C and Bolognesi, S and Bordoni, S and Boyd, SB and Brailsford, D and Bravar, A and Bronner, C and Buchanan, N and Calland, RG and Caravaca Rodríguez and J and Cartwright, SL and Castillo, R and Catanesi, MG and Cervera, A and Cherdack, D and Chikuma,
             N and Christodoulou, G et al.},
   Title = {Upper bound on neutrino mass based on T2K neutrino timing
             measurements},
   Journal = {Physical Review D},
   Volume = {93},
   Number = {1},
   Year = {2016},
   Month = {January},
   url = {http://dx.doi.org/10.1103/PhysRevD.93.012006},
   Doi = {10.1103/PhysRevD.93.012006},
   Key = {fds318487}
}

@article{fds318486,
   Author = {Zhang, Y and Abe, K and Haga, Y and Hayato, Y and Ikeda, M and Iyogi, K and Kameda, J and Kishimoto, Y and Miura, M and Moriyama, S and Nakahata, M and Nakajima, T and Nakano, Y and Nakayama, S and Orii, A and Sekiya, H and Shiozawa, M and Takeda, A and Tanaka, H and Tomura, T and Wendell, RA and Irvine, T and Kajita, T and Kametani, I and Kaneyuki, K and Nishimura,
             Y and Richard, E and Okumura, K and Labarga, L and Fernandez, P and Gustafson, J and Kachulis, C and Kearns, E and Raaf, JL and Stone, JL and Sulak, LR and Berkman, S and Nantais, CM and Tanaka, HA and Tobayama, S and Goldhaber, M and Carminati, G et al.},
   Title = {First measurement of radioactive isotope production through
             cosmic-ray muon spallation in Super-Kamiokande
             IV},
   Journal = {Physical Review D},
   Volume = {93},
   Number = {1},
   Year = {2016},
   Month = {January},
   url = {http://dx.doi.org/10.1103/PhysRevD.93.012004},
   Doi = {10.1103/PhysRevD.93.012004},
   Key = {fds318486}
}

@article{fds326489,
   Author = {Rasmussen, A and Guyonnet, A and Lage, C and Antilogus, P and Astier, P and Doherty, P and Gilmore, K and Kotov, I and Lupton, R and Nomerotski, A and O'Connor, P and Stubbs, C and Tyson, A and Walter,
             C},
   Title = {High fidelity point-spread function retrieval in the
             presence of electrostatic, hysteretic pixel
             response},
   Journal = {Proceedings of SPIE - The International Society for Optical
             Engineering},
   Volume = {9915},
   Year = {2016},
   Month = {January},
   ISBN = {9781510602090},
   url = {http://dx.doi.org/10.1117/12.2234482},
   Abstract = {© 2016 SPIE. We employ electrostatic conversion drift
             calculations to match CCD pixel signal covariances observed
             in at field exposures acquired using candidate sensor
             devices for the LSST Camera. 1, 2 We thus constrain pixel
             geometry distortions present at the end of integration,
             based on signal images recorded. We use available data from
             several operational voltage parameter settings to validate
             our understanding. Our primary goal is to optimize flux
             point spread function (FPSF) estimation quantitatively, and
             thereby minimize sensor-induced errors which may limit
             performance in precision astronomy applications. We consider
             alternative compensation scenarios that will take maximum
             advantage of our understanding of this underlying mechanism
             in data processing pipelines currently under development. To
             quantitatively capture the pixel response in
             high-contrast/high dynamic range operational extrema, we
             propose herein some straightforward laboratory tests that
             involve altering the time order of source illumination on
             sensors, within individual test exposures. Hence the word
             hysteretic in the title of this paper.},
   Doi = {10.1117/12.2234482},
   Key = {fds326489}
}

@article{fds318488,
   Author = {Abe, K and Adam, J and Aihara, H and Akiri, T and Andreopoulos, C and Aoki,
             S and Ariga, A and Assylbekov, S and Autiero, D and Barbi, M and Barker,
             GJ and Barr, G and Bartet-Friburg, P and Bass, M and Batkiewicz, M and Bay,
             F and Berardi, V and Berger, BE and Berkman, S and Bhadra, S and Blaszczyk,
             FDM and Blondel, A and Bojechko, C and Bolognesi, S and Bordoni, S and Boyd, SB and Brailsford, D and Bravar, A and Bronner, C and Calland, RG and Caravaca Rodríguez and J and Cartwright, SL and Castillo, R and Catanesi, MG and Cervera, A and Cherdack, D and Chikuma, N and Christodoulou, G and Clifton, A et al.},
   Title = {Measurement of the charged-current quasielastic cross
             section on carbon with the ND280 detector at
             T2K},
   Journal = {Physical Review D - Particles, Fields, Gravitation, and
             Cosmology},
   Volume = {92},
   Number = {11},
   Year = {2015},
   Month = {December},
   url = {http://dx.doi.org/10.1103/PhysRevD.92.112003},
   Doi = {10.1103/PhysRevD.92.112003},
   Key = {fds318488}
}

@article{fds318489,
   Author = {Takhistov, V and Abe, K and Haga, Y and Hayato, Y and Ikeda, M and Iyogi,
             K and Kameda, J and Kishimoto, Y and Miura, M and Moriyama, S and Nakahata,
             M and Nakajima, T and Nakano, Y and Nakayama, S and Orii, A and Sekiya, H and Shiozawa, M and Takeda, A and Tanaka, H and Tomura, T and Wendell, RA and Irvine, T and Kajita, T and Kametani, I and Kaneyuki, K and Nishimura,
             Y and Richard, E and Okumura, K and Labarga, L and Fernandez, P and Gustafson, J and Kachulis, C and Kearns, E and Raaf, JL and Stone, JL and Sulak, LR and Berkman, S and Nantais, CM and Tanaka, HA and Tobayama, S and Goldhaber, M and Carminati, G et al.},
   Title = {Search for Nucleon and Dinucleon Decays with an Invisible
             Particle and a Charged Lepton in the Final State at the
             Super-Kamiokande Experiment.},
   Journal = {Physical Review Letters},
   Volume = {115},
   Number = {12},
   Pages = {121803},
   Year = {2015},
   Month = {September},
   url = {http://dx.doi.org/10.1103/physrevlett.115.121803},
   Abstract = {Search results for nucleon decays p→e^{+}X, p→μ^{+}X,
             n→νγ (where X is an invisible, massless particle) as
             well as dinucleon decays np→e^{+}ν, np→μ^{+}ν, and
             np→τ^{+}ν in the Super-Kamiokande experiment are
             presented. Using single-ring data from an exposure of
              273.4  kton·yr, a search for these decays yields a
             result consistent with no signal. Accordingly, lower limits
             on the partial lifetimes of τ_{p→e^{+}X}>7.9×10^{32} yr,
             τ_{p→μ^{+}X}>4.1×10^{32} yr, τ_{n→νγ}>5.5×10^{32}
             yr, τ_{np→e^{+}ν}>2.6×10^{32}  yr,
             τ_{np→μ^{+}ν}>2.2×10^{32} yr, and τ_{np→τ^{+}ν}>2.9×10^{31}
             yr at a 90% confidence level are obtained. Some of these
             searches are novel.},
   Doi = {10.1103/physrevlett.115.121803},
   Key = {fds318489}
}

@article{fds318490,
   Author = {Abe, K and Adam, J and Aihara, H and Andreopoulos, C and Aoki, S and Ariga,
             A and Assylbekov, S and Autiero, D and Barbi, M and Barker, GJ and Barr, G and Bartet-Friburg, P and Bass, M and Batkiewicz, M and Bay, F and Berardi,
             V and Berger, BE and Berkman, S and Bhadra, S and Blaszczyk, FDM and Blondel, A and Bolognesi, S and Bordoni, S and Boyd, SB and Brailsford,
             D and Bravar, A and Bronner, C and Buchanan, N and Calland, RG and Caravaca
             Rodríguez, J and Cartwright, SL and Castillo, R and Catanesi, MG and Cervera, A and Cherdack, D and Chikuma, N and Christodoulou, G and Clifton, A and Coleman, J et al.},
   Title = {Measurement of the charged current quasielastic cross
             section on carbon with the T2K on-axis neutrino
             beam},
   Journal = {Physical Review D - Particles, Fields, Gravitation, and
             Cosmology},
   Volume = {91},
   Number = {11},
   Year = {2015},
   Month = {June},
   url = {http://dx.doi.org/10.1103/PhysRevD.91.112002},
   Doi = {10.1103/PhysRevD.91.112002},
   Key = {fds318490}
}

@article{fds318491,
   Author = {Abe, K and Adam, J and Aihara, H and Andreopoulos, C and Aoki, S and Ariga,
             A and Assylbekov, S and Autiero, D and Barbi, M and Barker, GJ and Barr, G and Bartet-Friburg, P and Bass, M and Batkiewicz, M and Bay, F and Berardi,
             V and Berger, BE and Berkman, S and Bhadra, S and Blaszczyk, FDM and Blondel, A and Bolognesi, S and Bordoni, S and Boyd, SB and Brailsford,
             D and Bravar, A and Bronner, C and Buchanan, N and Calland, RG and Caravaca
             Rodríguez, J and Cartwright, SL and Castillo, R and Catanesi, MG and Cervera, A and Cherdack, D and Chikuma, N and Christodoulou, G and Clifton, A and Coleman, J et al.},
   Title = {Measurement of the electron neutrino charged-current
             interaction rate on water with the T2K ND280
             detector},
   Journal = {Physical Review D - Particles, Fields, Gravitation, and
             Cosmology},
   Volume = {91},
   Number = {11},
   Year = {2015},
   Month = {June},
   url = {http://dx.doi.org/10.1103/PhysRevD.91.112010},
   Doi = {10.1103/PhysRevD.91.112010},
   Key = {fds318491}
}

@article{fds318492,
   Author = {Abe, K and Aihara, H and Andreopoulos, C and Anghel, I and Ariga, A and Ariga, T and Asfandiyarov, R and Askins, M and Back, JJ and Ballett, P and Barbi, M and Barker, GJ and Barr, G and Bay, F and Beltrame, P and Berardi,
             V and Bergevin, M and Berkman, S and Berry, T and Bhadra, S and Blaszczyk,
             FDM and Blondel, A and Bolognesi, S and Boyd, SB and Bravar, A and Bronner,
             C and Cafagna, FS and Carminati, G and Cartwright, SL and Catanesi, MG and Choi, K and Choi, JH and Collazuol, G and Cowan, G and Cremonesi, L and Davies, G and De Rosa and G and Densham, C and Detwiler, J and Dewhurst, D and Di Lodovico and F et al.},
   Title = {Physics potential of a long-baseline neutrino oscillation
             experiment using a J-PARC neutrino beam and
             Hyper-Kamiokande},
   Journal = {Progress of Theoretical and Experimental
             Physics},
   Volume = {2015},
   Number = {5},
   Pages = {53C02},
   Year = {2015},
   Month = {May},
   url = {http://dx.doi.org/10.1093/ptep/ptv061},
   Doi = {10.1093/ptep/ptv061},
   Key = {fds318492}
}

@article{fds248693,
   Author = {Walter, CW},
   Title = {The Brighter-Fatter and other sensor effects in CCD
             simulations for precision astronomy},
   Journal = {Journal of Instrumentation},
   Volume = {10},
   Number = {05},
   Pages = {C05015-C05015},
   Year = {2015},
   Month = {May},
   url = {http://dx.doi.org/10.1088/1748-0221/10/05/C05015},
   Doi = {10.1088/1748-0221/10/05/C05015},
   Key = {fds248693}
}

@article{fds318493,
   Author = {Choi, K and Abe, K and Haga, Y and Hayato, Y and Iyogi, K and Kameda, J and Kishimoto, Y and Miura, M and Moriyama, S and Nakahata, M and Nakano, Y and Nakayama, S and Sekiya, H and Shiozawa, M and Suzuki, Y and Takeda, A and Tomura, T and Wendell, RA and Irvine, T and Kajita, T and Kametani, I and Kaneyuki, K and Lee, KP and Nishimura, Y and Okumura, K and McLachlan,
             T and Labarga, L and Kearns, E and Raaf, JL and Stone, JL and Sulak, LR and Berkman, S and Tanaka, HA and Tobayama, S and Goldhaber, M and Carminati, G and Kropp, WR and Mine, S and Renshaw, A and Smy, MB and Sobel, HW and Ganezer, KS and Hill, J et al.},
   Title = {Search for neutrinos from annihilation of captured low-mass
             dark matter particles in the sun by super-kamiokande.},
   Journal = {Physical Review Letters},
   Volume = {114},
   Number = {14},
   Pages = {141301},
   Year = {2015},
   Month = {April},
   url = {http://dx.doi.org/10.1103/physrevlett.114.141301},
   Abstract = {Super-Kamiokande (SK) can search for weakly interacting
             massive particles (WIMPs) by detecting neutrinos produced
             from WIMP annihilations occurring inside the Sun. In this
             analysis, we include neutrino events with interaction
             vertices in the detector in addition to upward-going muons
             produced in the surrounding rock. Compared to the previous
             result, which used the upward-going muons only, the signal
             acceptances for light (few-GeV/c^{2}-200-GeV/c^{2}) WIMPs
             are significantly increased. We fit 3903 days of SK data to
             search for the contribution of neutrinos from WIMP
             annihilation in the Sun. We found no significant excess over
             expected atmospheric-neutrino background and the result is
             interpreted in terms of upper limits on WIMP-nucleon elastic
             scattering cross sections under different assumptions about
             the annihilation channel. We set the current best limits on
             the spin-dependent WIMP-proton cross section for WIMP masses
             below 200  GeV/c^{2} (at 10  GeV/c^{2},
             1.49×10^{-39}  cm^{2} for χχ→bb[over ¯] and
             1.31×10^{-40}  cm^{2} for χχ→τ^{+}τ^{-}
             annihilation channels), also ruling out some fraction of
             WIMP candidates with spin-independent coupling in the
             few-GeV/c^{2} mass range.},
   Doi = {10.1103/physrevlett.114.141301},
   Key = {fds318493}
}

@article{fds318494,
   Author = {Abe, K and Adam, J and Aihara, H and Akiri, T and Andreopoulos, C and Aoki,
             S and Ariga, A and Assylbekov, S and Autiero, D and Barbi, M and Barker,
             GJ and Barr, G and Bartet-Friburg, P and Bass, M and Batkiewicz, M and Bay,
             F and Berardi, V and Berger, BE and Berkman, S and Bhadra, S and Blaszczyk,
             FDM and Blondel, A and Bojechko, C and Bordoni, S and Boyd, SB and Brailsford, D and Bravar, A and Bronner, C and Buchanan, N and Calland,
             RG and Caravaca Rodriguez and J and Cartwright, SL and Castillo, R and Catanesi, MG and Cervera, A and Cherdack, D and Christodoulou, G and Clifton, A and Coleman, J et al.},
   Title = {Neutrino oscillation physics potential of the T2K
             experiment},
   Journal = {Progress of Theoretical and Experimental
             Physics},
   Volume = {2015},
   Number = {4},
   Pages = {43C01},
   Year = {2015},
   Month = {April},
   url = {http://dx.doi.org/10.1093/ptep/ptv031},
   Doi = {10.1093/ptep/ptv031},
   Key = {fds318494}
}

@article{fds248694,
   Author = {Abe, K and Hayato, Y and Iida, T and Ishihara, K and Kameda, J and Koshio,
             Y and Minamino, A and Mitsuda, C and Miura, M and Moriyama, S and Nakahata,
             M and Obayashi, Y and Ogawa, H and Sekiya, H and Shiozawa, M and Suzuki, Y and Takeda, A and Takeuchi, Y and Ueshima, K and Watanabe, H and Higuchi, I and Ishihara, C and Ishitsuka, M and Kajita, T and Kaneyuki, K and Mitsuka,
             G and Nakayama, S and Nishino, H and Okumura, K and Saji, C and Takenaga,
             Y and Clark, S and Desai, S and Dufour, F and Herfurth, A and Kearns, E and Likhoded, S and Litos, M and Raaf, JL and Stone, JL and Sulak, LR and Wang,
             W and Goldhaber, M et al.},
   Title = {Search for oscillation in Super-Kamiokande},
   Journal = {Physical Review D - Particles, Fields, Gravitation, and
             Cosmology},
   Volume = {91},
   Number = {7},
   Pages = {072006},
   Year = {2015},
   Month = {April},
   ISSN = {1550-7998},
   url = {http://dx.doi.org/10.1103/PhysRevD.91.072006},
   Abstract = {A search for neutron-antineutron ($n-\bar{n}$) oscillation
             was undertaken in Super-Kamiokande using the 1489 live-day
             or $2.45 \times 10^{34}$ neutron-year exposure data. This
             process violates both baryon and baryon minus lepton numbers
             by an absolute value of two units and is predicted by a
             large class of hypothetical models where the seesaw
             mechanism is incorporated to explain the observed tiny
             neutrino masses and the matter-antimatter asymmetry in the
             Universe. No evidence for $n-\bar{n}$ oscillation was found,
             the lower limit of the lifetime for neutrons bound in
             ${}^{16}$O, in an analysis that included all of the
             significant sources of experimental uncertainties, was
             determined to be $1.9 \times 10^{32}$~years at the 90\%
             confidence level. The corresponding lower limit for the
             oscillation time of free neutrons was calculated to be $2.7
             \times 10^8$~s using a theoretical value of the nuclear
             suppression factor of $0.517 \times 10^{23}$~s$^{-1}$ and
             its uncertainty.},
   Doi = {10.1103/PhysRevD.91.072006},
   Key = {fds248694}
}

@article{fds248695,
   Author = {Abe, K and Adam, J and Aihara, H and Akiri, T and Andreopoulos, C and Aoki,
             S and Ariga, A and Assylbekov, S and Autiero, D and Barbi, M and Barker,
             GJ and Barr, G and Bartet-Friburg, P and Bass, M and Batkiewicz, M and Bay,
             F and Berardi, V and Berger, BE and Berkman, S and Bhadra, S and Blaszczyk,
             FDM and Blondel, A and Bolognesi, S and Bordoni, S and Boyd, SB and Brailsford, D and Bravar, A and Bronner, C and Buchanan, N and Calland,
             RG and Caravaca Rodríguez and J and Cartwright, SL and Castillo, R and Catanesi, MG and Cervera, A and Cherdack, D and Chikuma, N and Christodoulou, G and Clifton, A et al.},
   Title = {Measurements of neutrino oscillation in appearance and
             disappearance channels by the T2K experiment with protons on
             target},
   Journal = {Physical Review D - Particles, Fields, Gravitation, and
             Cosmology},
   Volume = {91},
   Number = {7},
   Year = {2015},
   Month = {April},
   ISSN = {1550-7998},
   url = {http://dx.doi.org/10.1103/PhysRevD.91.072010},
   Doi = {10.1103/PhysRevD.91.072010},
   Key = {fds248695}
}

@article{fds248696,
   Author = {Gustafson, J and Abe, K and Haga, Y and Hayato, Y and Ikeda, M and Iyogi,
             K and Kameda, J and Kishimoto, Y and Miura, M and Moriyama, S and Nakahata,
             M and Nakajima, T and Nakano, Y and Nakayama, S and Orii, A and Sekiya, H and Shiozawa, M and Takeda, A and Tanaka, H and Tomura, T and Wendell, RA and Irvine, T and Kajita, T and Kametani, I and Kaneyuki, K and Nishimura,
             Y and Richard, E and Okumura, K and Labarga, L and Fernandez, P and Berkman, S and Tanaka, HA and Tobayama, S and Kearns, E and Raaf, JL and Stone, JL and Sulak, LR and Goldhaber, M and Carminati, G and Kropp, WR and Mine, S and Weatherly, P et al.},
   Title = {Search for dinucleon decay into pions at
             Super-Kamiokande},
   Journal = {Physical Review D - Particles, Fields, Gravitation, and
             Cosmology},
   Volume = {91},
   Number = {7},
   Year = {2015},
   Month = {April},
   ISSN = {1550-7998},
   url = {http://dx.doi.org/10.1103/PhysRevD.91.072009},
   Doi = {10.1103/PhysRevD.91.072009},
   Key = {fds248696}
}

@article{fds248697,
   Author = {Abe, K and Haga, Y and Hayato, Y and Ikeda, M and Iyogi, K and Kameda, J and Kishimoto, Y and Miura, M and Moriyama, S and Nakahata, M and Nakano, Y and Nakayama, S and Sekiya, H and Shiozawa, M and Suzuki, Y and Takeda, A and Tanaka, H and Tomura, T and Ueno, K and Wendell, RA and Yokozawa, T and Irvine, T and Kajita, T and Kametani, I and Kaneyuki, K and Lee, KP and McLachlan, T and Nishimura, Y and Richard, E and Okumura, K and Labarga,
             L and Fernandez, P and Gustafson, J and Kearns, E and Raaf, JL and Stone,
             JL and Sulak, LR and Berkman, S and Tanaka, HA and Tobayama, S and Goldhaber, M and Carminati, G et al.},
   Title = {Limits on sterile neutrino mixing using atmospheric
             neutrinos in Super-Kamiokande},
   Journal = {Physical Review D - Particles, Fields, Gravitation, and
             Cosmology},
   Volume = {91},
   Number = {5},
   Year = {2015},
   Month = {March},
   ISSN = {1550-7998},
   url = {http://dx.doi.org/10.1103/PhysRevD.91.052019},
   Doi = {10.1103/PhysRevD.91.052019},
   Key = {fds248697}
}

@article{fds248698,
   Author = {Abe, K and Adam, J and Aihara, H and Akiri, T and Andreopoulos, C and Aoki,
             S and Ariga, A and Assylbekov, S and Autiero, D and Barbi, M and Barker,
             GJ and Barr, G and Bartet-Friburg, P and Bass, M and Batkiewicz, M and Bay,
             F and Berardi, V and Berger, BE and Berkman, S and Bhadra, S and Blaszczyk,
             FDM and Blondel, A and Bojechko, C and Bolognesi, S and Bordoni, S and Boyd, SB and Brailsford, D and Bravar, A and Bronner, C and Buchanan, N and Calland, RG and Caravaca Rodríguez and J and Cartwright, SL and Castillo, R and Catanesi, MG and Cervera, A and Cherdack, D and Christodoulou, G and Clifton, A et al.},
   Title = {Search for short baseline disappearance with the T2K near
             detector},
   Journal = {Physical Review D - Particles, Fields, Gravitation, and
             Cosmology},
   Volume = {91},
   Number = {5},
   Year = {2015},
   Month = {March},
   ISSN = {1550-7998},
   url = {http://dx.doi.org/10.1103/PhysRevD.91.051102},
   Doi = {10.1103/PhysRevD.91.051102},
   Key = {fds248698}
}

@article{fds248699,
   Author = {Abe, K and Haga, Y and Hayato, Y and Ikeda, M and Iyogi, K and Kameda, J and Kishimoto, Y and Miura, M and Moriyama, S and Nakahata, M and Nakano, Y and Nakayama, S and Sekiya, H and Shiozawa, M and Suzuki, Y and Takeda, A and Tanaka, H and Tomura, T and Ueno, K and Wendell, RA and Yokozawa, T and Irvine, T and Kajita, T and Kametani, I and Kaneyuki, K and Lee, KP and McLachlan, T and Nishimura, Y and Richard, E and Okumura, K and Labarga,
             L and Fernandez, P and Gustafson, J and Kearns, E and Raaf, JL and Stone,
             JL and Sulak, LR and Berkman, S and Tanaka, HA and Tobayama, S and Goldhaber, M and Carminati, G et al.},
   Title = {Test of Lorentz invariance with atmospheric
             neutrinos},
   Journal = {Physical Review D - Particles, Fields, Gravitation, and
             Cosmology},
   Volume = {91},
   Number = {5},
   Year = {2015},
   Month = {March},
   ISSN = {1550-7998},
   url = {http://dx.doi.org/10.1103/PhysRevD.91.052003},
   Doi = {10.1103/PhysRevD.91.052003},
   Key = {fds248699}
}

@article{Zhang:2013tua,
   Author = {Zhang, H and Abe, K and Hayato, Y and Iyogi, K and Kameda, J and Kishimoto,
             Y and Miura, M and Moriyama, S and Nakahata, M and Nakano, Y and Nakayama,
             S and Sekiya, H and Shiozawa, M and Suzuki, Y and Takeda, A and Takenaga,
             Y and Tomura, T and Ueno, K and Yokozawa, T and Wendell, RA and Kaji, H and Kajita, T and Kaneyuki, K and Lee, KP and Nishimura, Y and Okumura, K and McLachlan, T and Labarga, L and Barkman, S and Tanaka, TS and Tobayama,
             S and Kearns, E and Raaf, JL and Stone, JL and Sulak, LR and Goldhaber, M and Bays, K and Carminati, G and Kropp, WR and Mine, S and Renshaw, A and Smy,
             MB and Sobel, HW et al.},
   Title = {Supernova Relic Neutrino search with neutron tagging at
             Super-Kamiokande-IV},
   Journal = {Astroparticle Physics},
   Volume = {60},
   Pages = {41-46},
   Year = {2015},
   Month = {January},
   ISSN = {0927-6505},
   url = {http://arxiv.org/pdf/1311.3738},
   Abstract = {http://arxiv.org/abs/1311.3738},
   Doi = {10.1016/j.astropartphys.2014.05.004},
   Key = {Zhang:2013tua}
}

@article{fds248700,
   Author = {Abe, K and Adam, J and Aihara, H and Akiri, T and Andreopoulos, C and Aoki,
             S and Ariga, A and Assylbekov, S and Autiero, D and Barbi, M and Barker,
             GJ and Barr, G and Bass, M and Batkiewicz, M and Bay, F and Berardi, V and Berger, BE and Berkman, S and Bhadra, S and Blaszczyk, FDM and Blondel,
             A and Bojechko, C and Bordoni, S and Boyd, SB and Brailsford, D and Bravar,
             A and Bronner, C and Buchanan, N and Calland, RG and Caravaca
             Rodríguez, J and Cartwright, SL and Castillo, R and Catanesi, MG and Cervera, A and Cherdack, D and Christodoulou, G and Clifton, A and Coleman, J and Coleman, SJ and Collazuol, G et
             al.},
   Title = {Measurement of the inclusive electron neutrino charged
             current cross section on carbon with the T2K near
             detector.},
   Journal = {Physical Review Letters},
   Volume = {113},
   Number = {24},
   Pages = {241803},
   Year = {2014},
   Month = {December},
   ISSN = {0031-9007},
   url = {http://dx.doi.org/10.1103/physrevlett.113.241803},
   Abstract = {The T2K off-axis near detector ND280 is used to make the
             first differential cross-section measurements of electron
             neutrino charged current interactions at energies
             ∼1  GeV as a function of electron momentum, electron
             scattering angle, and four-momentum transfer of the
             interaction. The total flux-averaged ν(e) charged current
             cross section on carbon is measured to be
             ⟨σ⟩(ϕ)=1.11±0.10(stat)±0.18(syst)×10⁻³⁸
             cm²/nucleon. The differential and total cross-section
             measurements agree with the predictions of two leading
             neutrino interaction generators, NEUT and GENIE. The NEUT
             prediction is 1.23×10⁻³⁸ cm²/nucleon and the GENIE
             prediction is 1.08×10⁻³⁸ cm²/nucleon. The total ν(e)
             charged current cross-section result is also in agreement
             with data from the Gargamelle experiment.},
   Doi = {10.1103/physrevlett.113.241803},
   Key = {fds248700}
}

@article{Abe:2014dyd,
   Author = {Abe, K and Adam, J and Aihara, H and Akiri, T and Andreopoulos, C and Aoki,
             S and Ariga, A and Ariga, T and Assylbekov, S and Autiero, D and Barbi, M and Barker, GJ and Barr, G and Bass, M and Batkiewicz, M and Bay, F and Bentham, SW and Berardi, V and Berger, BE and Berkman, S and Bertram, I and Bhadra, S and Blaszczyk, FDM and Blondel, A and Bojechko, C and Bordoni,
             S and Boyd, SB and Brailsford, D and Bravar, A and Bronner, C and Buchanan,
             N and Calland, RG and Caravaca Rodríguez and J and Cartwright, SL and Castillo, R and Catanesi, MG and Cervera, A and Cherdack, D and Christodoulou, G and Clifton, A et al.},
   Title = {Measurement of the neutrino-oxygen neutral-current
             interaction cross section by observing nuclear deexcitation
             rays},
   Journal = {Physical Review D - Particles, Fields, Gravitation, and
             Cosmology},
   Volume = {90},
   Number = {7},
   Pages = {072012},
   Year = {2014},
   Month = {October},
   ISSN = {1550-7998},
   url = {http://arxiv.org/pdf/1403.3140},
   Abstract = {http://arxiv.org/abs/1403.3140},
   Doi = {10.1103/PhysRevD.90.072012},
   Key = {Abe:2014dyd}
}

@article{fds248702,
   Author = {Abe, K and Hayato, Y and Iyogi, K and Kameda, J and Miura, M and Moriyama,
             S and Nakahata, M and Nakayama, S and Wendell, RA and Sekiya, H and Shiozawa, M and Suzuki, Y and Takeda, A and Takenaga, Y and Ueno, K and Yokozawa, T and Kaji, H and Kajita, T and Kaneyuki, K and Lee, KP and Okumura, K and McLachlan, T and Labarga, L and Kearns, E and Raaf, JL and Stone, JL and Sulak, LR and Goldhaber, M and Bays, K and Carminati, G and Kropp, WR and Mine, S and Renshaw, A and Smy, MB and Sobel, HW and Ganezer,
             KS and Hill, J and Keig, WE and Jang, JS and Kim, JY and Lim, IT and Albert,
             JB and Scholberg, K and Walter, CW et al.},
   Title = {Search for proton decay via using data of
             Super-Kamiokande},
   Journal = {Physical Review D - Particles, Fields, Gravitation, and
             Cosmology},
   Volume = {90},
   Number = {7},
   Year = {2014},
   Month = {October},
   ISSN = {1550-7998},
   url = {http://dx.doi.org/10.1103/PhysRevD.90.072005},
   Doi = {10.1103/PhysRevD.90.072005},
   Key = {fds248702}
}

@article{fds248706,
   Author = {Abe, K and Hayato, Y and Iida, T and Iyogi, K and Kameda, J and Koshio, Y and Kozuma, Y and Marti, L and Miura, M and Moriyama, S and Nakahata, M and Nakayama, S and Obayashi, Y and Sekiya, H and Shiozawa, M and Suzuki, Y and Takeda, A and Takenaga, Y and Ueno, K and Ueshima, K and Yamada, S and Yokozawa, T and Ishihara, C and Kaji, H and Kajita, T and Kaneyuki, K and Lee, KP and McLachlan, T and Okumura, K and Shimizu, Y and Tanimoto, N and Labarga, L and Kearns, E and Litos, M and Raaf, JL and Stone, JL and Sulak,
             LR and Goldhaber, M and Bays, K and Kropp, WR and Mine, S and Regis, C and Renshaw, A and Smy, MB et al.},
   Title = {Search for nucleon decay via n→ν[over ¯]π0 and
             p→ν[over ¯]π+ in Super-Kamiokande.},
   Journal = {Physical Review Letters},
   Volume = {113},
   Number = {12},
   Pages = {121802},
   Year = {2014},
   Month = {September},
   ISSN = {0031-9007},
   url = {http://dx.doi.org/10.1103/physrevlett.113.121802},
   Abstract = {We present the results of searches for nucleon decay via
             n→ν[over ¯]π0 and p→ν[over ¯]π+ using data from a
             combined 172.8  kt·yr exposure of Super-Kamiokande-I,-II,
             and-III. We set lower limits on the partial lifetime for
             each of these modes: τn→ν[over ¯]π0>1.1×10(33) years
             and τp→ν[over ¯]π+>3.9×10(32) years at a 90%
             confidence level.},
   Doi = {10.1103/physrevlett.113.121802},
   Key = {fds248706}
}

@article{Abe:2014nox,
   Author = {Abe, K and Adam, J and Aihara, H and Akiri, T and Andreopoulos, C and Aoki,
             S and Ariga, A and Assylbekov, S and Autiero, D and Barbi, M and Barker,
             GJ and Barr, G and Bass, M and Batkiewicz, M and Bay, F and Berardi, V and Berger, BE and Berkman, S and Bhadra, S and Blaszczyk, FDM and Blondel,
             A and Bojechko, C and Bordoni, S and Boyd, SB and Brailsford, D and Bravar,
             A and Bronner, C and Buchanan, N and Calland, RG and Caravaca
             Rodríguez, J and Cartwright, SL and Castillo, R and Catanesi, MG and Cervera, A and Cherdack, D and Christodoulou, G and Clifton, A and Coleman, J and Coleman, SJ and Collazuol, G et
             al.},
   Title = {Measurement of the inclusive charged current cross section
             on iron and hydrocarbon in the T2K on-axis neutrino
             beam},
   Journal = {Physical Review D - Particles, Fields, Gravitation, and
             Cosmology},
   Volume = {90},
   Number = {5},
   Pages = {052010},
   Year = {2014},
   Month = {September},
   ISSN = {1550-7998},
   url = {http://arxiv.org/pdf/1407.4256},
   Abstract = {http://arxiv.org/abs/1407.4256},
   Doi = {10.1103/PhysRevD.90.052010},
   Key = {Abe:2014nox}
}

@article{fds248705,
   Author = {Takhistov, V and Abe, K and Haga, Y and Hayato, Y and Ikeda, M and Iyogi,
             K and Kameda, J and Kishimoto, Y and Miura, M and Moriyama, S and Nakahata,
             M and Nakano, Y and Nakayama, S and Sekiya, H and Shiozawa, M and Suzuki,
             Y and Takeda, A and Tanaka, H and Tomura, T and Ueno, K and Wendell, RA and Yokozawa, T and Irvine, T and Kajita, T and Kametani, I and Kaneyuki, K and Lee, KP and McLachlan, T and Nishimura, Y and Richard, E and Okumura, K and Labarga, L and Fernandez, P and Berkman, S and Tanaka, HA and Tobayama,
             S and Gustafson, J and Kearns, E and Raaf, JL and Stone, JL and Sulak, LR and Goldhaber, M et al.},
   Title = {Search for Trilepton Nucleon Decay via and in the
             Super-Kamiokande Experiment},
   Journal = {Physical Review Letters},
   Volume = {113},
   Number = {10},
   Pages = {101801},
   Year = {2014},
   Month = {September},
   ISSN = {0031-9007},
   url = {http://dx.doi.org/10.1103/PhysRevLett.113.101801},
   Abstract = {The trilepton nucleon decay modes p→e+νν and p→μ+νν
             violate |Δ(B-L)| by two units. Using data from a 273.4
             kt yr exposure of Super-Kamiokande a search for these
             decays yields a fit consistent with no signal. Accordingly,
             lower limits on the partial lifetimes of
             τp→e+νν>1.7×10(32) years and τp→μ+νν>2.2×10(32)
             years at a 90% confidence level are obtained. These limits
             can constrain Grand Unified Theories which allow for such
             processes.},
   Doi = {10.1103/PhysRevLett.113.101801},
   Key = {fds248705}
}

@article{Agashe:2014kda,
   Author = {Olive, KA},
   Title = {Review of Particle Physics},
   Journal = {Chinese Physics C},
   Volume = {38},
   Number = {9},
   Pages = {090001-090001},
   Year = {2014},
   Month = {August},
   url = {http://dx.doi.org/10.1088/1674-1137/38/9/090001},
   Abstract = {© 2014 Regents of the University of California. The Review
             summarizes much of particle physics and cosmology. Using
             data from previous editions, plus 3,283 new measurements
             from 899 papers, we list, evaluate, and average measured
             properties of gauge bosons and the recently discovered Higgs
             boson, leptons, quarks, mesons, and baryons. We summarize
             searches for hypothetical particles such as heavy neutrinos,
             supersymmetric and technicolor particles, axions, dark
             photons, etc. All the particle properties and search limits
             are listed in Summary Tables. We also give numerous tables,
             figures, formulae, and reviews of topics such as
             Supersymmetry, Extra Dimensions, Particle Detectors,
             Probability, and Statistics. Among the 112 reviews are many
             that are new or heavily revised including those on: Dark
             Energy, Higgs Boson Physics, Electroweak Model, Neutrino
             Cross Section Measurements, Monte Carlo Neutrino Generators,
             Top Quark, Dark Matter, Dynamical Electroweak Symmetry
             Breaking, Accelerator Physics of Colliders, High-Energy
             Collider Parameters, Big Bang Nucleosynthesis, Astrophysical
             Constants and Cosmological Parameters. A booklet is
             available containing the Summary Tables and abbreviated
             versions of some of the other sections of this full Review.
             All tables, listings, and reviews (and errata) are also
             available on the Particle Data Group website:
             http://pdg.Ibi.gov.},
   Doi = {10.1088/1674-1137/38/9/090001},
   Key = {Agashe:2014kda}
}

@article{Abe:2014ugx,
   Author = {Abe, K and Adam, J and Aihara, H and Akiri, T and Andreopoulos, C and Aoki,
             S and Ariga, A and Ariga, T and Assylbekov, S and Autiero, D and Barbi, M and Barker, GJ and Barr, G and Bass, M and Batkiewicz, M and Bay, F and Bentham, SW and Berardi, V and Berger, BE and Berkman, S and Bertram, I and Bhadra, S and Blaszczyk, FDM and Blondel, A and Bojechko, C and Bordoni,
             S and Boyd, SB and Brailsford, D and Bravar, A and Bronner, C and Buchanan,
             N and Calland, RG and Caravaca Rodríguez and J and Cartwright, SL and Castillo, R and Catanesi, MG and Cervera, A and Cherdack, D and Christodoulou, G and Clifton, A et al.},
   Title = {Precise measurement of the neutrino mixing parameter θ23
             from muon neutrino disappearance in an off-axis
             beam.},
   Journal = {Physical Review Letters},
   Volume = {112},
   Number = {18},
   Pages = {181801},
   Year = {2014},
   Month = {May},
   ISSN = {0031-9007},
   url = {http://arxiv.org/pdf/1403.1532},
   Abstract = {New data from the T2K neutrino oscillation experiment
             produce the most precise measurement of the neutrino mixing
             parameter θ23. Using an off-axis neutrino beam with a peak
             energy of 0.6 GeV and a data set corresponding to
             6.57×10(20) protons on target, T2K has fit the
             energy-dependent νμ oscillation probability to determine
             oscillation parameters. The 68% confidence limit on
             sin(2)(θ23) is 0.514(-0.056)(+0.055) (0.511±0.055),
             assuming normal (inverted) mass hierarchy. The best-fit
             mass-squared splitting for normal hierarchy is
             Δm32(2)=(2.51±0.10)×10(-3)  eV(2)/c(4) (inverted
             hierarchy: Δm13(2)=(2.48±0.10)×10(-3)  eV(2)/c(4)).
             Adding a model of multinucleon interactions that affect
             neutrino energy reconstruction is found to produce only
             small biases in neutrino oscillation parameter extraction at
             current levels of statistical uncertainty.},
   Doi = {10.1103/physrevlett.112.181801},
   Key = {Abe:2014ugx}
}

@article{Abe:2014usb,
   Author = {Abe, K and Adam, J and Aihara, H and Akiri, T and Andreopoulos, C and Aoki,
             S and Ariga, A and Ariga, T and Assylbekov, S and Autiero, D and Barbi, M and Barker, GJ and Barr, G and Bass, M and Batkiewicz, M and Bay, F and Bentham, SW and Berardi, V and Berger, BE and Berkman, S and Bertram, I and Bhadra, S and Blaszczyk, FDM and Blondel, A and Bojechko, C and Bordoni,
             S and Boyd, SB and Brailsford, D and Bravar, A and Bronner, C and Buchanan,
             N and Calland, RG and Caravaca Rodríguez and J and Cartwright, SL and Castillo, R and Catanesi, MG and Cervera, A and Cherdack, D and Christodoulou, G and Clifton, A et al.},
   Title = {Measurement of the intrinsic electron neutrino component in
             the T2K neutrino beam with the ND280 detector},
   Journal = {Physical Review D - Particles, Fields, Gravitation, and
             Cosmology},
   Volume = {89},
   Number = {9},
   Pages = {092003},
   Year = {2014},
   Month = {May},
   ISSN = {1550-7998},
   url = {http://arxiv.org/pdf/1403.2552},
   Abstract = {http://arxiv.org/abs/1403.2552},
   Doi = {10.1103/PhysRevD.89.092003},
   Key = {Abe:2014usb}
}

@article{fds326726,
   Author = {Abe, K},
   Title = {Publisher’s Note: Measurement of the intrinsic electron
             neutrino component in the T2K neutrino beam with the ND280
             detector [Phys. Rev. D 89, 092003 (2014)]},
   Journal = {Physical Review D - Particles, Fields, Gravitation, and
             Cosmology},
   Volume = {89},
   Number = {9},
   Year = {2014},
   Month = {May},
   url = {http://dx.doi.org/10.1103/PhysRevD.89.099902},
   Doi = {10.1103/PhysRevD.89.099902},
   Key = {fds326726}
}

@article{fds248710,
   Author = {Litos, M and Abe, K and Hayato, Y and Iida, T and Ikeda, M and Iyogi, K and Kameda, J and Kobayashi, K and Koshio, Y and Kozuma, Y and Miura, M and Moriyama, S and Nakahata, M and Nakayama, S and Obayashi, Y and Ogawa,
             H and Sekiya, H and Shiozawa, M and Suzuki, Y and Takeda, A and Takenaga,
             Y and Takeuchi, Y and Ueno, K and Ueshima, K and Watanabe, H and Yamada, S and Yokozawa, T and Hazama, S and Ishihara, C and Kaji, H and Kajita, T and Kaneyuki, K and McLachlan, T and Okumura, K and Shimizu, Y and Tanimoto,
             N and Vagins, MR and Kearns, E and Stone, JL and Sulak, LR and Dufour, F and Raaf, JL and Henning, B et al.},
   Title = {Search for dinucleon decay into kaons in
             Super-Kamiokande.},
   Journal = {Physical Review Letters},
   Volume = {112},
   Number = {13},
   Pages = {131803},
   Year = {2014},
   Month = {April},
   ISSN = {0031-9007},
   url = {http://dx.doi.org/10.1103/physrevlett.112.131803},
   Abstract = {A search for the dinucleon decay pp → K+ K+ has been
             performed using 91.6  kton·yr data from
             Super-Kamiokande-I. This decay provides a sensitive probe of
             the R-parity-violating parameter λ112''. A boosted decision
             tree analysis found no signal candidates in the data. The
             expected background was 0.28±0.19 atmospheric neutrino
             induced events and the estimated signal detection efficiency
             was 12.6%±3.2%. A lower limit of 1.7×10(32)  years has
             been placed on the partial lifetime of the decay O16 →
             C14K+ K+ at 90% C.L. A corresponding upper limit of
             7.8×10(-9) has been placed on the parameter
             λ112''.},
   Doi = {10.1103/physrevlett.112.131803},
   Key = {fds248710}
}

@article{Renshaw:2013dzu,
   Author = {Renshaw, A and Abe, K and Hayato, Y and Iyogi, K and Kameda, J and Kishimoto, Y and Miura, M and Moriyama, S and Nakahata, M and Nakano, Y and Nakayama, S and Sekiya, H and Shiozawa, M and Suzuki, Y and Takeda, A and Takenaga, Y and Tomura, T and Ueno, K and Yokozawa, T and Wendell, RA and Irvine, T and Kajita, T and Kaneyuki, K and Lee, KP and Nishimura, Y and Okumura, K and McLachlan, T and Labarga, L and Berkman, S and Tanaka,
             HA and Tobayama, S and Kearns, E and Raaf, JL and Stone, JL and Sulak, LR and Goldhabar, M and Bays, K and Carminati, G and Kropp, WR and Mine, S and Smy, MB and Sobel, HW and Ganezer, KS et al.},
   Title = {First indication of terrestrial matter effects on solar
             neutrino oscillation.},
   Journal = {Physical Review Letters},
   Volume = {112},
   Number = {9},
   Pages = {091805},
   Year = {2014},
   Month = {March},
   ISSN = {0031-9007},
   url = {http://arxiv.org/pdf/1312.5176},
   Abstract = {We report an indication that the elastic scattering rate of
             solar B8 neutrinos with electrons in the Super-Kamiokande
             detector is larger when the neutrinos pass through Earth
             during nighttime. We determine the day-night asymmetry,
             defined as the difference of the average day rate and
             average night rate divided by the average of those two
             rates, to be [-3.2 ± 1.1(stat) ± 0.5(syst)]%, which
             deviates from zero by 2.7 σ. Since the elastic scattering
             process is mostly sensitive to electron-flavored solar
             neutrinos, a nonzero day-night asymmetry implies that the
             flavor oscillations of solar neutrinos are affected by the
             presence of matter within the neutrinos' flight path.
             Super-Kamiokande's day-night asymmetry is consistent with
             neutrino oscillations for 4 × 10(-5)  eV(2) ≤ Δm 2(21)
             ≤ 7 × 10(-5) eV(2) and large mixing values of θ12, at
             the 68% C.L.},
   Doi = {10.1103/physrevlett.112.091805},
   Key = {Renshaw:2013dzu}
}

@article{Abe:2013hdq,
   Author = {Abe, K and Adam, J and Aihara, H and Akiri, T and Andreopoulos, C and Aoki,
             S and Ariga, A and Ariga, T and Assylbekov, S and Autiero, D and Barbi, M and Barker, GJ and Barr, G and Bass, M and Batkiewicz, M and Bay, F and Bentham, SW and Berardi, V and Berger, BE and Berkman, S and Bertram, I and Bhadra, S and Blaszczyk, FDM and Blondel, A and Bojechko, C and Bordoni,
             S and Boyd, SB and Brailsford, D and Bravar, A and Bronner, C and Buchanan,
             N and Calland, RG and Caravaca Rodríguez and J and Cartwright, SL and Castillo, R and Catanesi, MG and Cervera, A and Cherdack, D and Christodoulou, G and Clifton, A et al.},
   Title = {Observation of electron neutrino appearance in a muon
             neutrino beam.},
   Journal = {Physical Review Letters},
   Volume = {112},
   Number = {6},
   Pages = {061802},
   Year = {2014},
   Month = {February},
   ISSN = {0031-9007},
   url = {http://arxiv.org/pdf/1311.4750},
   Abstract = {The T2K experiment has observed electron neutrino appearance
             in a muon neutrino beam produced 295 km from the
             Super-Kamiokande detector with a peak energy of 0.6 GeV. A
             total of 28 electron neutrino events were detected with an
             energy distribution consistent with an appearance signal,
             corresponding to a significance of 7.3σ when compared to
             4.92±0.55 expected background events. In the
             Pontecorvo-Maki-Nakagawa-Sakata mixing model, the electron
             neutrino appearance signal depends on several parameters
             including three mixing angles θ12, θ23, θ13, a mass
             difference Δm(32)(2) and a CP violating phase δ(CP). In
             this neutrino oscillation scenario, assuming
             |Δm(32)(2)|=2.4×10(-3)  eV(2), sin(2)θ(23)=0.5, and
             Δm322>0 (Δm(32)(2)<0), a best-fit value of
             sin(2)2θ(13)=0.140(-0.032)(+0.038) (0.170(-0.037)(+0.045))
             is obtained at δ(CP)=0. When combining the result with the
             current best knowledge of oscillation parameters including
             the world average value of θ(13) from reactor experiments,
             some values of δ(CP) are disfavored at the 90%
             C.L.},
   Doi = {10.1103/physrevlett.112.061802},
   Key = {Abe:2013hdq}
}

@article{fds248713,
   Author = {Abe, K and Abgrall, N and Aihara, H and Akiri, T and Andreopoulos, C and Aoki, S and Ariga, A and Ariga, T and Assylbekov, S and Autiero, D and Barbi, M and Barker, GJ and Barr, G and Bass, M and Batkiewicz, M and Bay,
             F and Bentham, SW and Berardi, V and Berger, BE and Berkman, S and Bertram,
             I and Bhadra, S and Blaszczyk, FDM and Blondel, A and Bojechko, C and Boyd,
             SB and Brailsford, D and Bravar, A and Bronner, C and Buchanan, N and Calland, RG and Caravaca Rodríguez and J and Cartwright, SL and Castillo, R and Catanesi, MG and Cervera, A and Cherdack, D and Christodoulou, G and Clifton, A and Coleman, J et
             al.},
   Title = {Recent Results from the T2K Experiment},
   Journal = {Nuclear Physics, Section B: Proceedings Supplements},
   Volume = {246-247},
   Pages = {23-28},
   Year = {2014},
   Month = {January},
   ISSN = {0920-5632},
   url = {http://dx.doi.org/10.1016/j.nuclphysbps.2013.10.060},
   Doi = {10.1016/j.nuclphysbps.2013.10.060},
   Key = {fds248713}
}

@article{Abe:2014wla,
   Author = {Abe, K. and others},
   Title = {Test of Lorentz Invariance with Atmospheric Neutrinos
             [Submitted for Publication]},
   Year = {2014},
   url = {http://arxiv.org/pdf/1410.4267},
   Abstract = {http://arxiv.org/abs/1410.4267},
   Key = {Abe:2014wla}
}

@article{Takhistov:2014pfw,
   Author = {Takhistov, V. and others},
   Title = {Search for Trilepton Nucleon Decay via $p \rightarrow e^+
             \nu \nu$ and $p \rightarrow \mu^+ \nu \nu$ in the
             Super-Kamiokande Experiment},
   Journal = {Phys.Rev.Lett.},
   Volume = {113},
   Pages = {101801},
   Year = {2014},
   url = {http://arxiv.org/pdf/1409.1947},
   Abstract = {http://arxiv.org/abs/1409.1947},
   Doi = {10.1103/PhysRevLett.113.101801},
   Key = {Takhistov:2014pfw}
}

@article{Abe:2014mwa,
   Author = {Abe, K. and others},
   Title = {Search for Proton Decay via $p \rightarrow \nu K^{+}$ using
             260 kiloton$\cdot$year data of Super-Kamiokande},
   Journal = {Phys.Rev.},
   Volume = {D90},
   Pages = {072005},
   Year = {2014},
   url = {http://arxiv.org/pdf/1408.1195},
   Abstract = {http://arxiv.org/abs/1408.1195},
   Doi = {10.1103/PhysRevD.90.072005},
   Key = {Abe:2014mwa}
}

@article{Abe:2014oda,
   Author = {Abe, K. and others},
   Title = {Measurement of the $\nu_\mu$ CCQE cross section on carbon
             with the ND280 detector at T2K [Submitted for
             Publication]},
   Year = {2014},
   url = {http://arxiv.org/pdf/1411.6264},
   Abstract = {http://arxiv.org/abs/1411.6264},
   Key = {Abe:2014oda}
}

@article{Abe:2013lua,
   Author = {Abe, K. and others},
   Title = {A Search for Nucleon Decay via $n \rightarrow \bar{\nu}
             \pi^{0}$ and $p \rightarrow \bar{\nu} \pi^{+}$ in
             Super-Kamiokande},
   Journal = {Phys.Rev.Lett.},
   Volume = {113},
   Pages = {121802},
   Year = {2014},
   url = {http://arxiv.org/pdf/1305.4391},
   Abstract = {http://arxiv.org/abs/1305.4391},
   Doi = {10.1103/PhysRevLett.113.121802},
   Key = {Abe:2013lua}
}

@article{Abe:2014nuo,
   Author = {Abe, K. and others},
   Title = {Search for short baseline $\nu_e$ disappearance with the T2K
             near detector [Submitted for Publication]},
   Year = {2014},
   url = {http://arxiv.org/pdf/1410.8811},
   Abstract = {http://arxiv.org/abs/1410.8811},
   Key = {Abe:2014nuo}
}

@article{Abe:2014gda,
   Author = {Abe, K. and others},
   Title = {Limits on Sterile Neutrino Mixing using Atmospheric
             Neutrinos in Super-Kamiokande [Submitted for
             Publication]},
   Year = {2014},
   url = {http://arxiv.org/pdf/1410.2008},
   Abstract = {http://arxiv.org/abs/1410.2008},
   Key = {Abe:2014gda}
}

@article{Abe:2014agb,
   Author = {Abe, K. and others},
   Title = {Measurement of the Inclusive Electron Neutrino Charged
             Current Cross Section on Carbon with the T2K Near Detector
             [Submitted for Publication]},
   Year = {2014},
   url = {http://arxiv.org/pdf/1407.7389},
   Abstract = {http://arxiv.org/abs/1407.7389},
   Key = {Abe:2014agb}
}

@article{Abe:2014tzr,
   Author = {Abe, K. and others},
   Title = {Neutrino Oscillation Physics Potential of the T2K Experiment
             [Submitted for Publication]},
   Year = {2014},
   url = {http://arxiv.org/pdf/1409.7469},
   Abstract = {http://arxiv.org/abs/1409.7469},
   Key = {Abe:2014tzr}
}

@article{Abe:2013fuq,
   Author = {collaboration, T and Abe, K and Abgrall, N and Aihara, H and Akiri, T and Andreopoulos, C and Aoki, S and Ariga, A and Ariga, T and Assylbekov, S and Autiero, D and Barbi, M and Barker, GJ and Barr, G and Bass, M and Batkiewicz, M and Bay, F and Bentham, SW and Berardi, V and Berger, BE and Berkman, S and Bertram, I and Bhadra, S and Blaszczyk, FDM and Blondel,
             A and Bojechko, C and Boyd, SB and Brailsford, D and Bravar, A and Bronner,
             C and Buchanan, N and Calland, RG and Rodriguez, JC and Cartwright, SL and Castillo, R and Catanesi, MG and Cervera, A and Cherdack, D and Christodoulou, G and Clifton, A et al.},
   Title = {Measurement of Neutrino Oscillation Parameters from Muon
             Neutrino Disappearance with an Off-axis Beam},
   Journal = {Phys. Rev. Lett.},
   Volume = {111},
   Pages = {211803},
   Year = {2013},
   Month = {August},
   url = {http://arxiv.org/abs/1308.0465v2},
   Abstract = {The T2K collaboration reports a precision measurement of
             muon neutrino disappearance with an off-axis neutrino beam
             with a peak energy of 0.6 GeV. Near detector measurements
             are used to constrain the neutrino flux and cross section
             parameters. The Super-Kamiokande far detector, which is 295
             km downstream of the neutrino production target, collected
             data corresponding to $3.01 \times 10^{20}$ protons on
             target. In the absence of neutrino oscillations, $205 \pm
             17$ (syst.) events are expected to be detected and only 58
             muon neutrino event candidates are observed. A fit to the
             neutrino rate and energy spectrum assuming three neutrino
             flavors, normal mass hierarchy and $\theta_{23}\leq \pi/4$
             yields a best-fit mixing angle $\sin^2(2\theta_{23})=1.000$
             and mass splitting $|\Delta m^2_{32}| =2.44 \times 10^{-3}$
             eV$^2$/c$^4$. If $\theta_{23}\geq \pi/4$ is assumed, the
             best-fit mixing angle changes to $\sin^2(2\theta_{23})=0.999$
             and the mass splitting remains unchanged.},
   Doi = {10.1103/PhysRevLett.111.211803},
   Key = {Abe:2013fuq}
}

@article{Abe:2013gga,
   Author = {Abe, K and Hayato, Y and Iida, T and Iyogi, K and Kameda, J and Kishimoto,
             Y and Koshio, Y and Marti, L and Miura, M and Moriyama, S and Nakahata, M and Nakano, Y and Nakayama, S and Obayashi, Y and Sekiya, H and Shiozawa, M and Suzuki, Y and Takeda, A and Takenaga, Y and Tanaka, H and Tomura, T and Ueno, K and Wendell, RA and Yokozawa, T and Irvine, TJ and Kaji, H and Kajita, T and Kaneyuki, K and Lee, KP and Nishimura, Y and Okumura, K and McLachlan, T and Labarga, L and Kearns, E and Raaf, JL and Stone, JL and Sulak, LR and Berkman, S and Tanaka, HA and Tobayama, S and Goldhaber,
             M and Bays, K and Carminati, G et al.},
   Title = {Calibration of the Super-Kamiokande Detector},
   Journal = {Nuclear Inst. and Methods in Physics Research, A 737C
             (2014), pp. 253-272},
   Volume = {A737},
   Pages = {253-272},
   Year = {2013},
   Month = {June},
   url = {http://arxiv.org/abs/1307.0162v2},
   Abstract = {Procedures and results on hardware level detector
             calibration in Super-Kamiokande (SK) are presented in this
             paper. In particular, we report improvements made in our
             calibration methods for the experimental phase IV in which
             new readout electronics have been operating since 2008. The
             topics are separated into two parts. The first part
             describes the determination of constants needed to interpret
             the digitized output of our electronics so that we can
             obtain physical numbers such as photon counts and their
             arrival times for each photomultiplier tube (PMT). In this
             context, we developed an in-situ procedure to determine
             high-voltage settings for PMTs in large detectors like SK,
             as well as a new method for measuring PMT quantum efficiency
             and gain in such a detector. The second part describes the
             modeling of the detector in our Monte Carlo simulation,
             including in particular the optical properties of its water
             target and their variability over time. Detailed studies on
             the water quality are also presented. As a result of this
             work, we achieved a precision sufficient for physics
             analysis over a wide energy range (from a few MeV to above a
             TeV). For example, the charge determination was understood
             at the 1% level, and the timing resolution was 2.1 nsec at
             the one-photoelectron charge level and 0.5 nsec at the
             100-photoelectron charge level.},
   Doi = {10.1016/j.nima.2013.11.081},
   Key = {Abe:2013gga}
}

@article{Abe:2012jj,
   Author = {Abe, K and Hayato, Y and Iida, T and Iyogi, K and Kameda, J and Koshio, Y and Kozuma, Y and Marti, L and Miura, M and Moriyama, S and Nakahata, M and Nakayama, S and Obayashi, Y and Sekiya, H and Shiozawa, M and Suzuki, Y and Takeda, A and Takenaga, Y and Ueno, K and Ueshima, K and Yamada, S and Yokozawa, T and Ishihara, C and Kaji, H and Kajita, T and Kaneyuki, K and Lee, KP and McLachlan, T and Okumura, K and Shimizu, Y and Tanimoto, N and Labarga, L and Kearns, E and Litos, M and Raaf, JL and Stone, JL and Sulak,
             LR and Goldhaber, M and Bays, K and Kropp, WR and Mine, S and Regis, C and Renshaw, A and Smy, MB et al.},
   Title = {Evidence for the appearance of atmospheric tau neutrinos in
             super-Kamiokande.},
   Journal = {Physical Review Letters},
   Volume = {110},
   Number = {18},
   Pages = {181802},
   Year = {2013},
   Month = {May},
   url = {http://www.ncbi.nlm.nih.gov/pubmed/23683190},
   Abstract = {Super-Kamiokande atmospheric neutrino data were fit with an
             unbinned maximum likelihood method to search for the
             appearance of tau leptons resulting from the interactions of
             oscillation-generated tau neutrinos in the detector.
             Relative to the expectation of unity, the tau normalization
             is found to be 1.42 ± 0.35(stat)(-0.12)(+0.14)(syst)
             excluding the no-tau-appearance hypothesis, for which the
             normalization would be zero, at the 3.8σ level. We estimate
             that 180.1 ± 44.3(stat)(-15.2)(+17.8) (syst) tau leptons
             were produced in the 22.5 kton fiducial volume of the
             detector by tau neutrinos during the 2806 day running
             period. In future analyses, this large sample of selected
             tau events will allow the study of charged current tau
             neutrino interaction physics with oscillation produced tau
             neutrinos.},
   Doi = {10.1103/PhysRevLett.110.181802},
   Key = {Abe:2012jj}
}

@article{Abe:2013xua,
   Author = {Collaboration, T and Abgrall, N and Aihara, H and Akiri, T and Albert,
             JB and Andreopoulos, C and Aoki, S and Ariga, A and Ariga, T and Assylbekov, S and Autiero, D and Barbi, M and Barker, GJ and Barr, G and Bass, M and Batkiewicz, M and Bay, F and Bentham, SW and Berardi, V and Berger, BE and Berkman, S and Bertram, I and Beznosko, D and Bhadra, S and Blaszczyk, FDM and Blondel, A and Bojechko, C and Boyd, S and Brailsford, D and Bravar, A and Bronner, C and Brook-Roberge, DG and Buchanan, N and Calland, RG and Rodriguez, JC and Cartwright, SL and Castillo, R and Catanesi, MG and Cervera, A and Cherdack, D et
             al.},
   Title = {Evidence of Electron Neutrino Appearance in a Muon Neutrino
             Beam},
   Volume = {D88},
   Pages = {032002},
   Year = {2013},
   Month = {April},
   url = {http://arxiv.org/abs/1304.0841v2},
   Abstract = {The T2K collaboration reports evidence for electron neutrino
             appearance at the atmospheric mass splitting, |\Delta
             m_{32}^2|=2.4x10^{-3} eV^2. An excess of electron neutrino
             interactions over background is observed from a muon
             neutrino beam with a peak energy of 0.6 GeV at the
             Super-Kamiokande (SK) detector 295 km from the beam's
             origin. Signal and background predictions are constrained by
             data from near detectors located 280 m from the neutrino
             production target. We observe 11 electron neutrino candidate
             events at the SK detector when a background of
             3.3\pm0.4(syst.) events is expected. The background-only
             hypothesis is rejected with a p-value of 0.0009 (3.1\sigma),
             and a fit assuming \nu_{\mu}->\nu_e oscillations with
             sin^2(2\theta_{23})=1, \delta_{CP}=0 and |\Delta
             m_{32}^2|=2.4x10^{-3} eV^2 yields sin^2(2\theta_{13})=0.088^{+0.049}_{-0.039}(stat.+syst.).},
   Doi = {10.1103/PhysRevD.88.032002},
   Key = {Abe:2013xua}
}

@article{Abe:2013jth,
   Author = {Collaboration, T and Abe, K and Abgrall, N and Aihara, H and Akiri, T and Albert, JB and Andreopoulos, C and Aoki, S and Ariga, A and Ariga, T and Assylbekov, S and Autiero, D and Barbi, M and Barker, GJ and Barr, G and Bass, M and Batkiewicz, M and Bay, F and Bentham, SW and Berardi, V and Berger, BE and Berkman, S and Bertram, I and Beznosko, D and Bhadra, S and Blaszczyk, FDM and Blondel, A and Bojechko, C and Boyd, S and Brailsford, D and Bravar, A and Bronner, C and Brook-Roberge, DG and Buchanan, N and Calland, RG and Rodríguez, JC and Cartwright, SL and Castillo, R and Catanesi, MG and Cervera, A et
             al.},
   Title = {Measurement of the Inclusive NuMu Charged Current Cross
             Section on Carbon in the Near Detector of the T2K
             Experiment},
   Volume = {D87},
   Pages = {092003},
   Year = {2013},
   Month = {February},
   url = {http://arxiv.org/abs/1302.4908v2},
   Abstract = {T2K has performed the first measurement of \nu{\mu}
             inclusive charged current interactions on carbon at neutrino
             energies of ~1 GeV where the measurement is reported as a
             flux-averaged double differential cross section in muon
             momentum and angle. The flux is predicted by the beam Monte
             Carlo and external data, including the results from the
             NA61/SHINE experiment. The data used for this measurement
             were taken in 2010 and 2011, with a total of 10.8 x 10^{19}
             protons-on-target. The analysis is performed on 4485
             inclusive charged current interaction candidates selected in
             the most upstream fine-grained scintillator detector of the
             near detector. The flux-averaged total cross section is
             <\sigma_CC>_\phi =(6.91 +/- 0.13 (stat) +/- 0.84 (syst))
             x10^{-39} cm^2/nucleon for a mean neutrino energy of 0.85
             GeV.},
   Doi = {10.1103/PhysRevD.87.092003},
   Key = {Abe:2013jth}
}

@article{fds248715,
   Author = {Abe, K and Abgrall, N and Aihara, H and Akiri, T and Albert, JB and Andreopoulos, C and Aoki, S and Ariga, A and Ariga, T and Assylbekov, S and Autiero, D and Barbi, M and Barker, GJ and Barr, G and Bass, M and Batkiewicz, M and Bay, F and Bentham, SW and Berardi, V and Berger, BE and Berkman, S and Bertram, I and Beznosko, D and Bhadra, S and Blaszczyk,
             FDM and Blondel, A and Bojechko, C and Boyd, S and Bravar, A and Bronner,
             C and Brook-Roberge, DG and Buchanan, N and Calland, RG and Rodriguez,
             JC and Cartwright, SL and Castillo, R and Catanesi, M-G and Cervera, A and Cherdack, D and Christodoulou, G et al.},
   Title = {T2K neutrino flux prediction (vol 87, 012001,
             2013)},
   Journal = {Physical Review D - Particles, Fields, Gravitation, and
             Cosmology},
   Volume = {87},
   Number = {1},
   Year = {2013},
   Month = {January},
   ISSN = {1550-7998},
   url = {http://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcApp=PARTNER_APP&SrcAuth=LinksAMR&KeyUT=WOS:000314229300009&DestLinkType=FullRecord&DestApp=ALL_WOS&UsrCustomerID=47d3190e77e5a3a53558812f597b0b92},
   Doi = {10.1103/PhysRevD.87.019902},
   Key = {fds248715}
}

@article{Adams:2013qkq,
   Author = {Adams, C. and others},
   Title = {Scientific Opportunities with the Long-Baseline Neutrino
             Experiment},
   Year = {2013},
   url = {http://arxiv.org/pdf/1307.7335},
   Abstract = {http://arxiv.org/abs/1307.7335},
   Key = {Adams:2013qkq}
}

@article{deGouvea:2013onf,
   Author = {de Gouvea, A. and others},
   Title = {Neutrinos},
   Year = {2013},
   url = {http://arxiv.org/pdf/1310.4340},
   Abstract = {http://arxiv.org/abs/1310.4340},
   Key = {deGouvea:2013onf}
}

@article{Abe:2012av,
   Author = {Collaboration, T and Abe, K and Abgrall, N and Aihara, H and Akiri, T and Albert, JB and Andreopoulos, C and Aoki, S and Ariga, A and Ariga, T and Assylbekov, S and Autiero, D and Barbi, M and Barker, GJ and Barr, G and Bass, M and Batkiewicz, M and Bay, F and Bentham, SW and Berardi, V and Berger, BE and Berkman, S and Bertram, I and Beznosko, D and Bhadra, S and Blaszczyk, FDM and Blondel, A and Bojechko, C and Boyd, S and Bravar, A and Bronner, C and Brook-Roberge, DG and Buchanan, N and Calland, RG and Rodriguez, JC and Cartwright, SL and Castillo, R and Catanesi, MG and Cervera, A and Cherdack, D et al.},
   Title = {The T2K Neutrino Flux Prediction},
   Journal = {Phys. Rev. D},
   Volume = {87},
   Pages = {012001},
   Year = {2012},
   Month = {November},
   url = {http://arxiv.org/abs/1211.0469v3},
   Abstract = {The Tokai-to-Kamioka (T2K) experiment studies neutrino
             oscillations using an off-axis muon neutrino beam with a
             peak energy of about 0.6 GeV that originates at the J-PARC
             accelerator facility. Interactions of the neutrinos are
             observed at near detectors placed at 280 m from the
             production target and at the far detector --
             Super-Kamiokande (SK) -- located 295 km away. The flux
             prediction is an essential part of the successful prediction
             of neutrino interaction rates at the T2K detectors and is an
             important input to T2K neutrino oscillation and cross
             section measurements. A FLUKA and GEANT3 based simulation
             models the physical processes involved in the neutrino
             production, from the interaction of primary beam protons in
             the T2K target, to the decay of hadrons and muons that
             produce neutrinos. The simulation uses proton beam monitor
             measurements as inputs. The modeling of hadronic
             interactions is re-weighted using thin target hadron
             production data, including recent charged pion and kaon
             measurements from the NA61/SHINE experiment. For the first
             T2K analyses the uncertainties on the flux prediction are
             evaluated to be below 15% near the flux peak. The
             uncertainty on the ratio of the flux predictions at the far
             and near detectors is less than 2% near the flux
             peak.},
   Doi = {10.1103/PhysRevD.87.012001},
   Key = {Abe:2012av}
}

@article{Beringer:1900zz,
   Author = {Beringer, J and Arguin, J-F and Barnett, RM and Copic, K and Dahl, O and Groom, DE and Lin, C-J and Lys, J and Murayama, H and Wohl, CG and Yao,
             W-M and Zyla, PA and Amsler, C and Antonelli, M and Asner, DM and Baer, H and Band, HR and Basaglia, T and Bauer, CW and Beatty, JJ and Belousov, VI and Bergren, E and Bernardi, G and Bertl, W and Bethke, S and Bichsel, H and Biebel, O and Blucher, E and Blusk, S and Brooijmans, G and Buchmueller,
             O and Cahn, RN and Carena, M and Ceccucci, A and Chakraborty, D and Chen,
             M-C and Chivukula, RS and Cowan, G and D'Ambrosio, G and Damour, T and de
             Florian, D and de Gouvea, A et al.},
   Title = {REVIEW OF PARTICLE PHYSICS Particle Data
             Group},
   Journal = {Physical Review D - Particles, Fields, Gravitation, and
             Cosmology},
   Volume = {86},
   Number = {1},
   Pages = {010001},
   Year = {2012},
   Month = {July},
   ISSN = {1550-7998},
   url = {http://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcApp=PARTNER_APP&SrcAuth=LinksAMR&KeyUT=WOS:000306603100001&DestLinkType=FullRecord&DestApp=ALL_WOS&UsrCustomerID=47d3190e77e5a3a53558812f597b0b92},
   Doi = {10.1103/PhysRevD.86.010001},
   Key = {Beringer:1900zz}
}

@article{Abe:2011xv,
   Author = {Abe, K and Abgrall, N and Ajima, Y and Aihara, H and Albert, JB and others},
   Title = {Measurements of the T2K neutrino beam properties using the
             INGRID on-axis near detector},
   Journal = {Nucl.Instrum.Meth.},
   Volume = {A694},
   Pages = {211-223},
   Year = {2012},
   ISSN = {0168-9002},
   url = {http://arxiv.org/pdf/1111.3119},
   Abstract = {http://arxiv.org/abs/1111.3119},
   Doi = {10.1016/j.nima.2012.03.023},
   Key = {Abe:2011xv}
}

@article{:2012rv,
   Author = {Nishino, H and Abe, K and Hayato, Y and Iida, T and Ikeda, M and Kameda, J and Koshio, Y and Miura, M and Moriyama, S and Nakahata, M and Nakayama, S and Obayashi, Y and Sekiya, H and Shiozawa, M and Suzuki, Y and Takeda, A and Takenaga, Y and Takeuchi, Y and Ueno, K and Ueshima, K and Watanabe, H and Yamada, S and Hazama, S and Higuchi, I and Ishihara, C and Kaji, H and Kajita, T and Kaneyuki, K and Mitsuka, G and Okumura, K and Tanimoto, N and Dufour, F and Kearns, E and Litos, M and Raaf, JL and Stone, JL and Sulak,
             LR and Goldhaber, M and Bays, K and Cravens, JP and Kropp, WR and Mine, S and Regis, C and Smy, MB et al.},
   Title = {Search for nucleon decay into charged antilepton plus meson
             in Super-Kamiokande i and II},
   Journal = {Physical Review D - Particles, Fields, Gravitation, and
             Cosmology},
   Volume = {85},
   Number = {11},
   Pages = {112001},
   Year = {2012},
   ISSN = {1550-7998},
   url = {http://arxiv.org/pdf/1203.4030},
   Abstract = {Searches for a nucleon decay into a charged antilepton (e +
             or μ +) plus a light meson (π0, π -, η, ρ0, ρ -, ω)
             were performed using the Super-Kamiokande I and II data.
             Twelve nucleon decay modes were searched for. The total
             exposure is 140.9kiloton•years, which includes a
             91.7kiloton•year exposure (1489.2 live days) of
             Super-Kamiokande-I and a 49.2kiloton•year exposure (798.6
             live days) of Super-Kamiokande II. The number of candidate
             events in the data was consistent with the atmospheric
             neutrino background expectation. No significant evidence for
             a nucleon decay was observed in the data. Thus, lower limits
             on the nucleon partial lifetime at 90% confidence level were
             obtained. The limits range from 3.6×1031 to 8.2×1033years,
             depending on the decay modes. © 2012 American Physical
             Society.},
   Doi = {10.1103/PhysRevD.85.112001},
   Key = {:2012rv}
}

@article{Regis:2012sn,
   Author = {Regis, C and Abe, K and Hayato, Y and Iyogi, K and Kameda, J and Koshio, Y and Marti, L and Miura, M and Moriyama, S and Nakahata, M and Nakayama, S and Obayashi, Y and Sekiya, H and Shiozawa, M and Suzuki, Y and Takeda, A and Takenaga, Y and Ueno, K and Yokozawa, T and Kaji, H and Kajita, T and Kaneyuki, K and Lee, KP and Okumura, K and McLachlan, T and Labarga, L and Kearns, E and Raaf, JL and Stone, JL and Sulak, LR and Goldhaber, M and Bays, K and Carminati, G and Kropp, WR and Mine, S and Renshaw, A and Smy,
             MB and Sobel, HW and Ganezer, KS and Hill, J and Keig, WE and Jang, JS and Kim, JY and Lim, IT and Albert, JB et al.},
   Title = {Search for proton decay via p→μ+K0 in Super-Kamiokande I,
             II, and III},
   Journal = {Physical Review D - Particles, Fields, Gravitation, and
             Cosmology},
   Volume = {86},
   Number = {1},
   Pages = {012006},
   Year = {2012},
   ISSN = {1550-7998},
   url = {http://arxiv.org/pdf/1205.6538},
   Abstract = {We have searched for proton decay via p→μ +K0 using data
             from a 91.7kiloton•year exposure of Super-Kamiokande- I, a
             49.2kiloton•year exposure of Super-Kamiokande II, and a
             31.9kiloton•year exposure of Super-Kamiokande III. The
             number of candidate events in the data was consistent with
             the atmospheric neutrino background expectation and no
             evidence for proton decay in this mode was found. We set a
             partial lifetime lower limit of 1.6×1033years at the 90%
             confidence level. © 2012 American Physical
             Society.},
   Doi = {10.1103/PhysRevD.86.012006},
   Key = {Regis:2012sn}
}

@article{Abe:2012gx,
   Author = {Abe, and K, and others},
   Title = {First Muon-Neutrino Disappearance Study with an Off-Axis
             Beam},
   Journal = {Phys.Rev.},
   Volume = {D85},
   Number = {3},
   Pages = {031103},
   Year = {2012},
   ISSN = {1550-7998},
   url = {http://arxiv.org/pdf/1201.1386},
   Abstract = {http://arxiv.org/abs/1201.1386},
   Doi = {10.1103/PhysRevD.85.031103},
   Key = {Abe:2012gx}
}

@article{Ueno:2012md,
   Author = {Ueno, K and Abe, K and Hayato, Y and Iida, T and Iyogi, K and Kameda, J and Koshio, Y and Kozuma, Y and Miura, M and Moriyama, S and Nakahata, M and Nakayama, S and Obayashi, Y and Sekiya, H and Shiozawa, M and Suzuki, Y and Takeda, A and Takenaga, Y and Ueshima, K and Yamada, S and Yokozawa, T and Martens, K and Schuemann, J and Vagins, M and Ishihara, C and Kaji, H and Kajita, T and Kaneyuki, K and McLachlan, T and Okumura, K and Shimizu,
             Y and Tanimoto, N and Kearns, E and Litos, M and Raaf, JL and Stone, JL and Sulak, LR and Bays, K and Kropp, WR and Mine, S and Regis, C and Renshaw,
             A and Smy, MB and Sobel, HW et al.},
   Title = {Search for GUT monopoles at Super-Kamiokande},
   Journal = {Astroparticle Physics},
   Volume = {36},
   Number = {1},
   Pages = {131-136},
   Year = {2012},
   ISSN = {0927-6505},
   url = {http://arxiv.org/pdf/1203.0940},
   Abstract = {GUT monopoles captured by the Sun's gravitation are expected
             to catalyze proton decays via the Callan-Rubakov process. In
             this scenario, protons, which initially decay into pions,
             will ultimately produce νe, νμ and ν̄ μ. After
             undergoing neutrino oscillation, all neutrino species appear
             when they arrive at the Earth, and can be detected by a
             50,000 metric ton Water Cherenkov detector, Super-Kamiokande
             (SK). A search for low energy neutrinos in the electron
             total energy range from 19 to 55 MeV was carried out with SK
             and gives a monopole flux limit of F M( σ0/1mb)&lt;6.3×10
             -24( βM/10 -3) 2cm- 2s- 1sr- 1 at 90% C.L., where βM is
             the monopole velocity in units of the speed of light and σ0
             is the catalysis cross section at βM=1. The obtained limit
             is several orders of magnitude more stringent than the
             current best cosmic-ray supermassive monopole flux limit for
             βM&lt;10 -2 and also two orders of magnitude lower than the
             result of the Kamiokande experiment, which used a similar
             detection method.© 2012 Elsevier B.V. All rights
             reserved.},
   Doi = {10.1016/j.astropartphys.2012.05.008},
   Key = {Ueno:2012md}
}

@article{Bays:2011si,
   Author = {Bays, K and Iida, T and Abe, K and Hayato, Y and Iyogi, K and Kameda, J and Koshio, Y and Marti, L and Miura, M and Moriyama, S and Nakahata, M and Nakayama, S and Obayashi, Y and Sekiya, H and Shiozawa, M and Suzuki, Y and Takeda, A and Takenaga, Y and Ueno, K and Ueshima, K and Yamada, S and Yokozawa, T and Kaji, H and Kajita, T and Kaneyuki, K and McLachlan, T and Okumura, K and Lee, KP and Martens, K and Vagins, M and Labarga, L and Kearns, E and Litos, M and Raaf, JL and Stone, JL and Sulak, LR and Kropp,
             WR and Mine, S and Regis, C and Renshaw, A and Smy, MB and Sobel, HW and Ganezer, KS and Hill, J and Keig, WE et al.},
   Title = {Supernova relic neutrino search at super-Kamiokande},
   Journal = {Physical Review D - Particles, Fields, Gravitation, and
             Cosmology},
   Volume = {85},
   Number = {5},
   Pages = {052007},
   Year = {2012},
   ISSN = {1550-7998},
   url = {http://arxiv.org/pdf/1111.5031},
   Abstract = {A new Super-Kamiokande search for supernova relic neutrinos
             was conducted using 2853 live days of data. Sensitivity is
             now greatly improved compared to the 2003 Super-Kamiokande
             result, which placed a flux limit near many theoretical
             predictions. This more detailed analysis includes a variety
             of improvements such as increased efficiency, a lower energy
             threshold, and an expanded data set. New combined upper
             limits on supernova relic neutrino flux are between 2.8 and
             3.1ν ̄ecm -2s -1&gt;16MeV total positron energy (17.3MeV E
             ν). © 2012 American Physical Society.},
   Doi = {10.1103/PhysRevD.85.052007},
   Key = {Bays:2011si}
}

@article{fds287700,
   Author = {Beringer, J and Arguin, J-F and Barnett, RM and Copic, K and Dahl, O and Groom, DE and Lin, C-J and Lys, J and Murayama, H and Wohl, CG and Yao,
             W-M and Zyla, PA and Amsler, C and Antonelli, M and Asner, DM and Baer, H and Band, HR and Basaglia, T and Bauer, CW and Beatty, JJ and Belousov, VI and Bergren, E and Bernardi, G and Bertl, W and Bethke, S and Bichsel, H and Biebel, O and Blucher, E and Blusk, S and Brooijmans, G and Buchmueller,
             O and Cahn, RN and Carena, M and Ceccucci, A and Chakraborty, D and Chen,
             M-C and Chivukula, RS and Cowan, G and D'ambrosio, G and Damour, T and Florian, DD and Gouvêa, AD et al.},
   Title = {Review of particle physics},
   Journal = {Physical Review D - Particles, Fields, Gravitation, and
             Cosmology},
   Volume = {86},
   Number = {1},
   Year = {2012},
   ISSN = {1550-7998},
   url = {http://dx.doi.org/10.1103/PhysRevD.70.096011},
   Abstract = {This biennial Review summarizes much of particle physics.
             Using data from previous editions, plus 2658 new
             measurements from 644 papers, we list, evaluate, and average
             measured properties of gauge bosons, leptons, quarks,
             mesons, and baryons. We summarize searches for hypothetical
             particles such as Higgs bosons, heavy neutrinos, and
             supersymmetric particles. All the particle properties and
             search limits are listed in Summary Tables. We also give
             numerous tables, figures, formulae, and reviews of topics
             such as the Standard Model, particle detectors, probability,
             and statistics. Among the 112 reviews are many that are new
             or heavily revised including those on Heavy-Quark and
             Soft-Collinear Effective Theory, Neutrino Cross Section
             Measurements, Monte Carlo Event Generators, Lattice QCD,
             Heavy Quarkonium Spectroscopy, Top Quark, Dark Matter, V cb
             &amp; V ub, Quantum Chromodynamics, High-Energy Collider
             Parameters, Astrophysical Constants, Cosmological
             Parameters, and Dark Matter. A booklet is available
             containing the Summary Tables and abbreviated versions of
             some of the other sections of this full Review. All tables,
             listings, and reviews (and errata) are also available on the
             Particle Data Group website: http://pdg.lbl.gov/. The 2012
             edition of Review of Particle Physics is published for the
             Particle Data Group as article 010001 in volume 86 of
             Physical Review D. This edition should be cited as: J.
             Beringer et al. (Particle Data Group), Phys. Rev. D 86,
             010001 (2012). © 2012 Regents of the University of
             California.},
   Doi = {10.1103/PhysRevD.70.096011},
   Key = {fds287700}
}

@article{Abe:2011ph,
   Author = {Abe, K and Hayato, Y and Iida, T and Ikeda, M and Iyogi, K and Kameda, J and Koshio, Y and Kozuma, Y and Miura, M and Moriyama, S and Nakahata, M and Nakayama, S and Obayashi, Y and Sekiya, H and Shiozawa, M and Suzuki, Y and Takeda, A and Takenaga, Y and Takeuchi, Y and Ueno, K and Ueshima, K and Watanabe, H and Yamada, S and Yokozawa, T and Ishihara, C and Kaji, H and Lee, KP and Kajita, T and Kaneyuki, K and McLachlan, T and Okumura, K and Shimizu, Y and Tanimoto, N and Martens, K and Vagins, MR and Labarga, L and Magro, LM and Dufour, F and Kearns, E and Litos, M and Raaf, JL and Stone,
             JL and Sulak, LR et al.},
   Title = {Search for differences in oscillation parameters for
             atmospheric neutrinos and antineutrinos at
             Super-Kamiokande.},
   Journal = {Physical Review Letters},
   Volume = {107},
   Number = {24},
   Pages = {241801},
   Year = {2011},
   Month = {December},
   url = {http://www.ncbi.nlm.nih.gov/pubmed/22242990},
   Abstract = {We present a search for differences in the oscillations of
             antineutrinos and neutrinos in the Super-Kamiokande-I, -II,
             and -III atmospheric neutrino sample. Under a two-flavor
             disappearance model with separate mixing parameters between
             neutrinos and antineutrinos, we find no evidence for a
             difference in oscillation parameters. Best-fit antineutrino
             mixing is found to be at (Δm2,sin2 2θ)=(2.0×10(-3)  eV2,
             1.0) and is consistent with the overall Super-K
             measurement.},
   Doi = {10.1103/PhysRevLett.107.241801},
   Key = {Abe:2011ph}
}

@article{fds326727,
   Author = {Tremblin, P and Minier, V and Schneider, N and Durand, GA and Ashley,
             MCB and Lawrence, JS and Luong-Van, DM and Storey, JWV and Durand, GA and Reinert, Y and Veyssiere, C and Walter, C and Ade, P and Calisse, PG and Challita, Z and Fossat, E and Sabbatini, L and Pellegrini, A and Ricaud,
             P and Urban, J},
   Title = {Site testing for submillimetre astronomy at Dome C,
             Antarctica},
   Journal = {Astronomy and astrophysics},
   Volume = {535},
   Pages = {A112-A112},
   Year = {2011},
   Month = {November},
   url = {http://dx.doi.org/10.1051/0004-6361/201117345},
   Doi = {10.1051/0004-6361/201117345},
   Key = {fds326727}
}

@article{Mariani:2010ez,
   Author = {Mariani, C and Tornero-Lopez, A and Alcaraz, JL and Andringa, S and Aoki, S and Aoyama, Y and Argyriades, J and Asakura, K and Ashie, R and Berghaus, F and Berns, H and Bhang, H and Blondel, A and Borghi, S and Bouchez, J and Burguet-Castell, J and Casper, D and Catala, J and Cavata, C and Cervera, A and Chen, SM and Cho, KO and Choi, JH and Dore, U and Espinal, X and Fechner, M and Fernandez, E and Fujii, Y and Fukuda, Y and Gomez-Cadenas, J and Gran, R and Hara, T and Hasegawa, M and Hasegawa,
             T and Hayato, Y and Helmer, RL and Hiraide, K and Hosaka, J and Ichikawa,
             AK and Iinuma, M and Ikeda, A and Ishida, T et al.},
   Title = {Measurement of inclusive pi(0) production in the
             charged-current interactions of neutrinos in a 1.3-GeV wide
             band beam},
   Journal = {Physical Review D - Particles, Fields, Gravitation, and
             Cosmology},
   Volume = {83},
   Number = {5},
   Pages = {054023},
   Year = {2011},
   Month = {March},
   ISSN = {1550-7998},
   url = {http://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcApp=PARTNER_APP&SrcAuth=LinksAMR&KeyUT=WOS:000288448700003&DestLinkType=FullRecord&DestApp=ALL_WOS&UsrCustomerID=47d3190e77e5a3a53558812f597b0b92},
   Abstract = {http://arxiv.org/abs/1012.1794},
   Doi = {10.1103/PhysRevD.83.054023},
   Key = {Mariani:2010ez}
}

@article{Abe:2011ky,
   Author = {Abe, K. and others},
   Title = {The search for n-nbar oscillation in Super-Kamiokande
             I},
   Year = {2011},
   url = {http://arxiv.org/pdf/1109.4227},
   Abstract = {http://arxiv.org/abs/1109.4227},
   Key = {Abe:2011ky}
}

@article{Tanaka:2011uf,
   Author = {Tanaka, T. and others},
   Title = {An Indirect Search for WIMPs in the Sun using 3109.6 days of
             upward-going muons in Super-Kamiokande},
   Journal = {Astrophys. J.},
   Volume = {742},
   Pages = {78},
   Year = {2011},
   url = {http://arxiv.org/pdf/1108.3384},
   Abstract = {http://arxiv.org/abs/1108.3384},
   Doi = {10.1088/0004-637X/742/2/78},
   Key = {Tanaka:2011uf}
}

@article{fds248723,
   Author = {Walter, C},
   Title = {Cross-section effects in the super-kamiokande tau appearance
             analysis},
   Journal = {AIP Conference Proceedings},
   Volume = {1405},
   Pages = {186-191},
   Year = {2011},
   ISSN = {0094-243X},
   url = {http://dx.doi.org/10.1063/1.3661583},
   Abstract = {In this talk, I explain the search for tau neutrino
             appearance in the atmospheric neutrino flux at
             Super-Kamiokande with a particular emphasis on the effect
             deep inelastic cross section uncertainties have on
             interpreting the result. In particular, I explain why the
             normalization of the DIS cross-section also needs to be
             treated as a parameter in the fit of tau normalization, and
             show how a neural net based on event parameters can separate
             various cross-section modes in the background sample. ©
             2011 American Institute of Physics.},
   Doi = {10.1063/1.3661583},
   Key = {fds248723}
}

@article{Mitsuka:2011ty,
   Author = {Mitsuka, G and Abe, K and Hayato, Y and Iida, T and Ikeda, M and Kameda, J and Koshio, Y and Miura, M and Moriyama, S and Nakahata, M and Nakayama, S and Obayashi, Y and Sekiya, H and Shiozawa, M and Suzuki, Y and Takeda, A and Takenaga, Y and Takeuchi, Y and Ueno, K and Ueshima, K and Watanabe, H and Yamada, S and Hazama, S and Higuchi, I and Ishihara, C and Kaji, H and Kajita, T and Kaneyuki, K and Nishino, H and Okumura, K and Tanimoto, N and Dufour, F and Kearns, E and Litos, M and Raaf, JL and Stone, JL and Sulak,
             LR and Goldhaber, M and Bays, K and Cravens, JP and Kropp, WR and Mine, S and Regis, C and Smy, MB et al.},
   Title = {Study of nonstandard neutrino interactions with atmospheric
             neutrino data in Super-Kamiokande i and II},
   Journal = {Physical Review D - Particles, Fields, Gravitation, and
             Cosmology},
   Volume = {84},
   Number = {11},
   Pages = {113008},
   Year = {2011},
   ISSN = {1550-7998},
   url = {http://arxiv.org/pdf/1109.1889},
   Abstract = {In this paper we study nonstandard neutrino interactions as
             an example of physics beyond the standard model using
             atmospheric neutrino data collected during the
             Super-Kamiokande I (1996-2001) and II (2003-2005) periods.
             We focus on flavor-changing-neutral-currents (FCNC), which
             allow neutrino flavor transitions via neutral current
             interactions, and effects which violate lepton
             nonuniversality and give rise to different neutral-current
             interaction- amplitudes for different neutrino flavors. We
             obtain a limit on the FCNC coupling parameter, ε μτ, |ε
             μτ|&lt; 1.1×10 -2 at 90% C.L. and various constraints on
             other FCNC parameters as a function of the nonuniversality
             coupling, ε ee. We find no evidence of nonstandard neutrino
             interactions in the Super-Kamiokande atmospheric data. ©
             2011 American Physical Society.},
   Doi = {10.1103/PhysRevD.84.113008},
   Key = {Mitsuka:2011ty}
}

@article{Abe:2011ks,
   Author = {Abe, K and Abgrall, N and Aihara, H and Ajima, Y and Albert, JB and Allan,
             D and Amaudruz, P-A and Andreopoulos, C and Andrieu, B and Anerella, MD and Angelsen, C and Aoki, S and Araoka, O and Argyriades, J and Ariga, A and Ariga, T and Assylbekov, S and André, JPAMD and Autiero, D and Badertscher, A and Ballester, O and Barbi, M and Barker, GJ and Baron,
             P and Barr, G and Bartoszek, L and Batkiewicz, M and Bay, F and Bentham, S and Berardi, V and Berger, BE and Berns, H and Bertram, I and Besnier, M and Beucher, J and Beznosko, D and Bhadra, S and Birney, P and Bishop, D and Blackmore, E and Blaszczyk, FDM et al.},
   Title = {The T2K experiment},
   Journal = {Nuclear Instruments and Methods in Physics Research Section
             A: Accelerators, Spectrometers, Detectors and Associated
             Equipment},
   Volume = {659},
   Number = {1},
   Pages = {106-135},
   Year = {2011},
   ISSN = {0168-9002},
   url = {http://arxiv.org/pdf/1106.1238},
   Abstract = {The T2K experiment is a long baseline neutrino oscillation
             experiment. Its main goal is to measure the last unknown
             lepton sector mixing angle θ13 by observing νe appearance
             in a νμ beam. It also aims to make a precision measurement
             of the known oscillation parameters, Δ232+ and sin22θ23,
             via νμ disappearance studies. Other goals of the
             experiment include various neutrino cross-section
             measurements and sterile neutrino searches. The experiment
             uses an intense proton beam generated by the J-PARC
             accelerator in Tokai, Japan, and is composed of a neutrino
             beamline, a near detector complex (ND280), and a far
             detector (Super-Kamiokande) located 295 km away from J-PARC.
             This paper provides a comprehensive review of the
             instrumentation aspect of the T2K experiment and a summary
             of the vital information for each subsystem. © 2011
             Elsevier B.V. All rights reserved.},
   Doi = {10.1016/j.nima.2011.06.067},
   Key = {Abe:2011ks}
}

@article{fds248762,
   Author = {Tanaka, T and Abe, K and Hayato, Y and Iida, T and Kameda, J and Koshio, Y and Kouzuma, Y and Miura, M and Moriyama, S and Nakahata, M and Nakayama, S and Obayashi, Y and Sekiya, H and Shiozawa, M and Suzuki, Y and Takeda, A and Takenaga, Y and Ueno, K and Ueshima, K and Yamada, S and Yokozawa, T and Ishihara, C and Hazama, S and Kaji, H and Kajita, T and Kaneyuki, K and McLachlan, T and Okumura, K and Shimizu, Y and Tanimoto, N and Dufour,
             F and Kearns, E and Litos, M and Raaf, JL and Stone, JL and Sulak, LR and Cravens, JP and Bays, K and Kropp, WR and Mine, S and Regis, C and Smy, MB and Sobel, HW and Ganezer, KS et al.},
   Title = {An indirect search for weakly interacting massive particles
             in the sun using 3109.6days of upward-going muons in
             super-kamiokande},
   Journal = {The Astrophysical Journal},
   Volume = {742},
   Number = {2},
   Year = {2011},
   ISSN = {0004-637X},
   url = {http://dx.doi.org/10.1088/0004-637X/742/2/78},
   Abstract = {We present the result of an indirect search for high energy
             neutrinos from Weakly Interacting Massive Particle (WIMP)
             annihilation in the Sun using upward-going muon (upmu)
             events at Super-Kamiokande. Data sets from SKI-SKIII
             (3109.6days) were used for the analysis. We looked for an
             excess of neutrino signal from the Sun as compared with the
             expected atmospheric neutrino background in three upmu
             categories: stopping, non-showering, and showering. No
             significant excess was observed. The 90% C.L. upper limits
             of upmu flux induced by WIMPs of 100GeV c-2 were 6.4 ×
             10-15cm -2s-1 and 4.0 × 10-15cm -2s-1 for the soft and hard
             annihilation channels, respectively. These limits correspond
             to upper limits of 4.5 × 10 -39cm-2 and 2.7 × 10-40cm-2
             for spin-dependent WIMP-nucleon scattering cross sections in
             the soft and hard annihilation channels, respectively. ©
             2011. The American Astronomical Society. All rights
             reserved.},
   Doi = {10.1088/0004-637X/742/2/78},
   Key = {fds248762}
}

@article{Abe:2011sj,
   Author = {Abe, and K, and others},
   Title = {Indication of Electron Neutrino Appearance from an
             Accelerator-produced Off-axis Muon Neutrino
             Beam},
   Journal = {Phys. Rev. Lett.},
   Volume = {107},
   Number = {4},
   Pages = {041801},
   Year = {2011},
   url = {http://www.ncbi.nlm.nih.gov/pubmed/21866992},
   Abstract = {http://arxiv.org/abs/1106.2822},
   Doi = {10.1103/PhysRevLett.107.041801},
   Key = {Abe:2011sj}
}

@article{Abe:2010hy,
   Author = {Abe, K and Hayato, Y and Iida, T and Ikeda, M and Ishihara, C and Iyogi, K and Kameda, J and Kobayashi, K and Koshio, Y and Kozuma, Y and Miura, M and Moriyama, S and Nakahata, M and Nakayama, S and Obayashi, Y and Ogawa,
             H and Sekiya, H and Shiozawa, M and Suzuki, Y and Takeda, A and Takenaga,
             Y and Ueno, K and Ueshima, K and Watanabe, H and Yamada, S and Yokozawa, T and Hazama, S and Kaji, H and Kajita, T and Kaneyuki, K and McLachlan, T and Okumura, K and Shimizu, Y and Tanimoto, N and Vagins, MR and Labarga, L and Magro, LM and Dufour, F and Kearns, E and Litos, M and Raaf, JL and Stone,
             JL and Sulak, LR and Wang, W et al.},
   Title = {Solar neutrino results in Super-Kamiokande-III},
   Journal = {Physical Review D - Particles, Fields, Gravitation, and
             Cosmology},
   Volume = {83},
   Number = {5},
   Pages = {052010},
   Year = {2011},
   ISSN = {1550-7998},
   url = {http://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcApp=PARTNER_APP&SrcAuth=LinksAMR&KeyUT=WOS:000288787100001&DestLinkType=FullRecord&DestApp=ALL_WOS&UsrCustomerID=47d3190e77e5a3a53558812f597b0b92},
   Abstract = {The results of the third phase of the Super-Kamiokande solar
             neutrino measurement are presented and compared to the first
             and second phase results. With improved detector
             calibrations, a full detector simulation, and improved
             analysis methods, the systematic uncertainty on the total
             neutrino flux is estimated to be ±2.1%, which is about two
             thirds of the systematic uncertainty for the first phase of
             Super-Kamiokande. The observed B8 solar flux in the 5.0 to
             20 MeV total electron energy region is 2.32±0.04(stat)
             ±0.05(sys)×106cm-2sec-1 under the assumption of pure
             electron-flavor content, in agreement with previous
             measurements. A combined oscillation analysis is carried out
             using SK-I, II, and III data, and the results are also
             combined with the results of other solar neutrino
             experiments. The best-fit oscillation parameters are
             obtained to be sin2θ12=0.30-0.01+0.02(tan2θ
             12=0.42-0.02+0.04) and Δm212=6.2-1.9+1.1×10 -5eV2.
             Combined with KamLAND results, the best-fit oscillation
             parameters are found to be sin2θ12=0.31±0.
             01(tan2θ12=0.44±0.03) and Δm212=7.6±0.2×10-5eV2. The B8
             neutrino flux obtained from global solar neutrino
             experiments is 5.3±0.2(stat+sys) ×106cm-2s-1, while the B8
             flux becomes 5.1±0.1(stat+sys)×106cm-2s-1 by adding
             KamLAND results. In a three-flavor analysis combining all
             solar neutrino experiments, the upper limit of sin2θ13 is
             0.060 at 95% C.L.. After combination with KamLAND results,
             the upper limit of sin2θ13 is found to be 0.059 at 95% C.L.
             © 2011 American Physical Society.},
   Doi = {10.1103/PhysRevD.83.052010},
   Key = {Abe:2010hy}
}

@article{:2008ea,
   Author = {Mariani, C and Tornero-Lopez, A and Alcaraz, JL and Andringa, S and Aoki, S and Aoyama, Y and Argyriades, J and Asakura, K and Ashie, R and Berghaus, F and Berns, H and Bhang, H and Blondel, A and Borghi, S and Bouchez, J and Burguet-Castell, J and Casper, D and Catala, J and Cavata, C and Cervera, A and Chen, SM and Cho, KO and Choi, JH and Dore, U and Espinal, X and Fechner, M and Fernandez, E and Fujii, Y and Fukuda, Y and Gomez-Cadenas, J and Gran, R and Hara, T and Hasegawa, M and Hasegawa,
             T and Hayato, Y and Helmer, RL and Hiraide, K and Hosaka, J and Ichikawa,
             AK and Iinuma, M and Ikeda, A and Ishida, T et al.},
   Title = {Measurement of inclusive π0 production in the
             charged-current interactions of neutrinos in a 1.3-GeV wide
             band beam},
   Journal = {Physical Review D - Particles, Fields, Gravitation, and
             Cosmology},
   Volume = {83},
   Number = {5},
   Pages = {032003},
   Year = {2011},
   ISSN = {1550-7998},
   url = {http://arxiv.org/pdf/0805.0186},
   Abstract = {In this paper, we report on the measurement of the rate of
             inclusive π0 production induced by charged-current neutrino
             interactions in a C 8H8 target at a mean energy of 1.3 GeV
             in the K2K near detector. Out of a sample of 11606
             charged-current neutrino interactions, we select 479 π0
             events with two reconstructed photons. We find that the
             cross section for the inclusive π0 production relative to
             the charged-current quasielastic cross section is
             σCCπ0σCCQE=0. 426±0.032(stat)±0.035(syst). The
             energy-dependent cross section ratio is also measured. The
             results are consistent with previous experiments for
             exclusive channels on different targets. © 2011 American
             Physical Society.},
   Doi = {10.1103/PhysRevD.83.054023},
   Key = {:2008ea}
}

@article{fds327690,
   Author = {Scholberg, K},
   Title = {Experimentation of neutrino physics},
   Journal = {TASI 2008 - Proceedings of the 2008 Theoretical Advanced
             Study Institute in Elementary Particle Physics: The Dawn of
             the LHC Era},
   Pages = {565-622},
   Year = {2010},
   Month = {December},
   Abstract = {These lectures broadly describe experimental progress in
             neutrino physics over the past few decades. I will describe
             the basic picture, how we know what we now know, and the
             next steps for the future. Copyright © 2010 by World
             Scientific Publishing Co. Pte. Ltd.},
   Key = {fds327690}
}

@article{Nakamura:2010zzi,
   Author = {Nakamura, K and Hagiwara, K and Hikasa, K and Murayama, H and Tanabashi,
             M and Watari, T and Amsler, C and Antonelli, M and Asner, DM and Baer, H and Band, HR and Barnett, RM and Basaglia, T and Bergren, E and Beringer, J and Bernardi, G and Bertl, W and Bichsel, H and Biebel, O and Blucher, E and Blusk, S and Cahn, RN and Carena, M and Ceccucci, A and Chakraborty, D and Chen, M-C and Chivukula, RS and Cowan, G and Dahl, O and D'Ambrosio, G and Damour, T and de Florian, D and de Gouvea, A and DeGrand, T and Dissertori, G and Dobrescu, B and Doser, M and Drees, M and Edwards, DA and Eidelman, S and Erler, J et al.},
   Title = {REVIEW OF PARTICLE PHYSICS},
   Journal = {Journal of Physics G: Nuclear and Particle
             Physics},
   Volume = {37},
   Number = {7A},
   Pages = {1-5},
   Year = {2010},
   Month = {July},
   ISSN = {0954-3899},
   url = {http://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcApp=PARTNER_APP&SrcAuth=LinksAMR&KeyUT=WOS:000282072100001&DestLinkType=FullRecord&DestApp=ALL_WOS&UsrCustomerID=47d3190e77e5a3a53558812f597b0b92},
   Doi = {10.1088/0954-3899/37/7A/075021},
   Key = {Nakamura:2010zzi}
}

@article{fds248721,
   Author = {Iida, T and Bays, K},
   Title = {A Search for supernova relic neutrinos at
             Super-Kamiokande},
   Journal = {Journal of Physics},
   Volume = {203},
   Year = {2010},
   ISSN = {1742-6588},
   url = {http://dx.doi.org/10.1088/1742-6596/203/1/012088},
   Abstract = {Supernova relic neutrinos (SRN) are the diffuse supernova
             neutrino background from all past supernovae. No experiment
             has succeeded in detecting SRN yet. Currently, the
             Super-Kamiokande experiment has the world's best flux upper
             limit of 1.2 e/cm2/sec for Ev &lt; 19.3MeV. We have worked
             to improve this value by improving the data analysis. We
             have achieved better reduction efficiency and lowered the
             analysis energy threshold by developing a new spallation cut
             as well as optimizing other cuts. © 2010 IOP Publishing
             Ltd.},
   Doi = {10.1088/1742-6596/203/1/012088},
   Key = {fds248721}
}

@article{Choubey:2009zz,
   Author = {Choubey, S and Schwetz, T and Walter, C},
   Title = {Working group I report (theory)},
   Journal = {AIP Conference Proceedings},
   Volume = {1222},
   Pages = {65-74},
   Year = {2010},
   ISSN = {0094-243X},
   url = {http://dx.doi.org/10.1063/1.3399397},
   Abstract = {The summary of the talks and discussions in Working Group I
             (Neutrino Oscillation Physics) at the NuFact08 workshop is
             presented here. © 2010 American Institute of
             Physics.},
   Doi = {10.1063/1.3399397},
   Key = {Choubey:2009zz}
}

@article{Wendell:2010md,
   Author = {Wendell, R and Ishihara, C and Abe, K and Hayato, Y and Iida, T and Ikeda,
             M and Iyogi, K and Kameda, J and Kobayashi, K and Koshio, Y and Kozuma, Y and Miura, M and Moriyama, S and Nakahata, M and Nakayama, S and Obayashi,
             Y and Ogawa, H and Sekiya, H and Shiozawa, M and Suzuki, Y and Takeda, A and Takenaga, Y and Takeuchi, Y and Ueno, K and Ueshima, K and Watanabe, H and Yamada, S and Yokozawa, T and Hazama, S and Kaji, H and Kajita, T and Kaneyuki, K and McLachlan, T and Okumura, K and Shimizu, Y and Tanimoto,
             N and Vagins, MR and Dufour, F and Kearns, E and Litos, M and Raaf, JL and Stone, JL and Sulak, LR et al.},
   Title = {Atmospheric neutrino oscillation analysis with subleading
             effects in Super-Kamiokande I, II, and III},
   Journal = {Physical Review D - Particles, Fields, Gravitation, and
             Cosmology},
   Volume = {81},
   Number = {9},
   Pages = {092004},
   Year = {2010},
   ISSN = {1550-7998},
   url = {http://hdl.handle.net/10161/4274 Duke open
             access},
   Abstract = {We present a search for nonzero θ13 and deviations of
             sin2θ23 from 0.5 in the oscillations of atmospheric
             neutrino data from Super-Kamiokande I, II, and III. No
             distortions of the neutrino flux consistent with nonzero
             θ13 are found and both neutrino mass hierarchy hypotheses
             are in agreement with the data. The data are best fit at
             Δm2=2.1×10-3eV2, sin2θ13=0.0, and sin2θ23=0.5. In the
             normal (inverted) hierarchy θ13 and Δm2 are constrained at
             the one-dimensional 90% C.L. to sin2θ13&lt;0.04(0.09) and
             1.9(1.7)×10 -3&lt;Δm2&lt;2.6(2.7)×10-3eV2. The
             atmospheric mixing angle is within 0.407≤sin2θ23≤0.583
             at 90% C.L. © 2010 The American Physical
             Society.},
   Doi = {10.1103/PhysRevD.81.092004},
   Key = {Wendell:2010md}
}

@article{:2009gd,
   Author = {Nishino, H and Clark, S and Abe, K and Hayato, Y and Iida, T and Ikeda, M and Kameda, J and Kobayashi, K and Koshio, Y and Miura, M and Moriyama, S and Nakahata, M and Nakayama, S and Obayashi, Y and Ogawa, H and Sekiya, H and Shiozawa, M and Suzuki, Y and Takeda, A and Takenaga, Y and Takeuchi, Y and Ueno, K and Ueshima, K and Watanabe, H and Yamada, S and Hazama, S and Higuchi, I and Ishihara, C and Kajita, T and Kaneyuki, K and Mitsuka, G and Okumura, K and Tanimoto, N and Vagins, MR and Dufour, F and Kearns, E and Litos, M and Raaf, JL and Stone, JL and Sulak, LR and Wang, W and Goldhaber, M and Dazeley, S et al.},
   Title = {Search for proton decay via p-->e+pi0 and p-->micro+pi0 in a
             large water Cherenkov detector.},
   Journal = {Physical Review Letters},
   Volume = {102},
   Number = {14},
   Pages = {141801},
   Year = {2009},
   Month = {April},
   ISSN = {0031-9007},
   url = {http://www.ncbi.nlm.nih.gov/pubmed/19392425},
   Abstract = {We have searched for proton decays via p-->e;{+}pi;{0} and
             p-->micro;{+}pi;{0} using data from a 91.7 kt.yr exposure of
             Super-Kamiokande-I and a 49.2 kt.yr exposure of
             Super-Kamiokande-II. No candidate events were observed with
             expected backgrounds induced by atmospheric neutrinos of 0.3
             events for each decay mode. From these results, we set lower
             limits on the partial lifetime of 8.2 x 10;{33} and 6.6 x
             10;{33} years at 90% confidence level for p-->e;{+}pi;{0}
             and p-->micro;{+}pi;{0} modes, respectively.},
   Doi = {10.1103/PhysRevLett.102.141801},
   Key = {:2009gd}
}

@article{Bernstein:2009ms,
   Author = {Bernstein, Adam and others},
   Title = {Report on the Depth Requirements for a Massive Detector at
             Homestake},
   Year = {2009},
   url = {http://arxiv.org/pdf/0907.4183},
   Abstract = {http://arxiv.org/abs/0907.4183},
   Key = {Bernstein:2009ms}
}

@article{Andreopoulos:2009zza,
   Author = {Andreopoulos, C and Gallagher, H and Hayato, Y and Sobczyk, JT and Walter, C and Zeller, S},
   Title = {The path forward: Monte Carlo convergence
             discussion},
   Journal = {AIP Conference Proceedings},
   Volume = {1189},
   Pages = {312-319},
   Year = {2009},
   ISSN = {0094-243X},
   url = {http://dx.doi.org/10.1063/1.3274175},
   Abstract = {This is a summary of "the path forward" discussion session
             of the NuInt09 workshop which focused on Monte Carlo event
             generators. The main questions raised as part of this
             discussion are: how to make Monte Carlo generators more
             reliable and how important it is to work on a universal
             Monte Carlo generator of events? In this contribution,
             several experts in the field summarize their views, as
             presented at the workshop. © 2009 American Institute of
             Physics.},
   Doi = {10.1063/1.3274175},
   Key = {Andreopoulos:2009zza}
}

@article{Watanabe:2008ru,
   Author = {Watanabe, H and Zhang, H and Abe, K and Hayato, Y and Iida, T and Ikeda, M and Kameda, J and Kobayashi, K and Koshio, Y and Miura, M and Moriyama, S and Nakahata, M and Nakayama, S and Obayashi, Y and Ogawa, H and Sekiya, H and Shiozawa, M and Suzuki, Y and Takeda, A and Takenaga, Y and Takeuchi, Y and Ueno, K and Ueshima, K and Yamada, S and Hazama, S and Higuchi, I and Ishihara, C and Kajita, T and Kaneyuki, K and Mitsuka, G and Nishino, H and Okumura, K and Tanimoto, N and Clark, S and Desai, S and Dufour, F and Kearns, E and Likhoded, S and Litos, M and Raaf, J and Stone, JL and Sulak,
             LR and Wang, W and Goldhaber, M et al.},
   Title = {First study of neutron tagging with a water Cherenkov
             detector},
   Journal = {Astroparticle Physics},
   Volume = {31},
   Number = {4},
   Pages = {320-328},
   Year = {2009},
   ISSN = {0927-6505},
   url = {http://arxiv.org/pdf/0811.0735},
   Abstract = {A first study of neutron tagging is conducted in
             Super-Kamiokande, a 50,000 ton water Cherenkov detector. The
             tagging efficiencies of thermal neutrons are evaluated in a
             0.2% GdCl3-water solution and pure water. They are
             determined to be, respectively, 66.7% for events above 3 MeV
             and 20% with corresponding background probabilities of 2 ×
             10- 4 and 3 × 10- 2. This newly developed technique may
             enable water Cherenkov detectors to identify over(ν, ̄)e's
             from astrophysical sources as well as those produced by
             commercial reactors via the delayed coincidence scheme. ©
             2009 Elsevier B.V.},
   Doi = {10.1016/j.astropartphys.2009.03.002},
   Key = {Watanabe:2008ru}
}

@article{Thrane:2009tw,
   Author = {Thrane, E and Abe, K and Hayato, Y and Iida, T and Ikeda, M and Kameda, J and Kobayashi, K and Koshio, Y and Miura, M and Moriyama, S and Nakahata, M and Nakayama, S and Obayashi, Y and Ogawa, H and Sekiya, H and Shiozawa, M and Suzuki, Y and Takeda, A and Takenaga, Y and Takeuchi, Y and Ueno, K and Ueshima, K and Watanabe, H and Yamada, S and Vagins, MR and Hazama, S and Higuchi, I and Ishihara, C and Kajita, T and Kaneyuki, K and Mitsuka, G and Nishino, H and Okumura, K and Tanimoto, N and Dufour, F and Kearns, E and Litos, M and Raaf, JL and Stone, JL and Sulak, LR and Goldhaber, M and Bays, K and Casper, D et al.},
   Title = {Search for astrophysical neutrino point sources at
             super-kamiokande},
   Journal = {The Astrophysical Journal},
   Volume = {704},
   Number = {1},
   Pages = {503-512},
   Year = {2009},
   ISSN = {0004-637X},
   url = {http://arxiv.org/pdf/0907.1594},
   Abstract = {It has been hypothesized that large fluxes of neutrinos may
             be created in astrophysical "cosmic accelerators." The
             primary background for a search for astrophysical neutrinos
             comes from atmospheric neutrinos, which do not exhibit the
             pointlike directional clustering that characterizes a
             distant astrophysical signal. We perform a search for
             neutrino point sources using the upward-going muon data from
             three phases of operation (SK-I, SK-II, and SK-III) spanning
             2623 days of live time taken from 1996 April 1 to 2007
             August 11. The search looks for signals from suspected
             galactic and extragalactic sources, transient sources, and
             uncataloged sources. While we find interesting signatures
             from two objects - RX J1713.7-3946 (97.5% CL) and GRB
             991004D (95.3% CL) - these signatures lack compelling
             statistical significance given trial factors. We set limits
             on the flux and fluence of neutrino point sources above
             energies of 1.6 GeV. © 2009 The American Astronomical
             Society. All rights reserved.},
   Doi = {10.1088/0004-637X/704/1/503},
   Key = {Thrane:2009tw}
}

@article{Thrane:2009fj,
   Author = {Thrane, E and Abe, K and Hayato, Y and Iida, T and Ikeda, M and Kameda, J and Kobayashi, K and Koshio, Y and Miura, M and Moriyama, S and Nakahata, M and Nakayama, S and Obayashi, Y and Ogawa, H and Sekiya, H and Shiozawa, M and Suzuki, Y and Takeda, A and Takenaga, Y and Takeuchi, Y and Ueno, K and Ueshima, K and Watanabe, H and Yamada, S and Vagins, MR and Hazama, S and Higuchi, I and Ishihara, C and Kajita, T and Kaneyuki, K and Mitsuka, G and Nishino, H and Okumura, K and Tanimoto, N and Dufour, F and Kearns, E and Litos, M and Raaf, JL and Stone, JL and Sulak, LR and Goldhaber, M and Bays, K and Casper, D et al.},
   Title = {Search for neutrinos from GRB 080319B at
             super-kamiokande},
   Journal = {The Astrophysical Journal},
   Volume = {697},
   Number = {1},
   Pages = {730-734},
   Year = {2009},
   ISSN = {0004-637X},
   url = {http://arxiv.org/pdf/0903.0624},
   Abstract = {We perform a search for neutrinos coincident with GRB
             080319B - the brightest GRB observed to date - in a 1000 s
             window. No statistically significant coincidences were
             observed and we thereby obtain an upper limit on the fluence
             of neutrino-induced muons from this source. From this we
             apply reasonable assumptions to derive a limit on neutrino
             fluence from the GRB. © 2009. The American Astronomical
             Society. All rights reserved.},
   Doi = {10.1088/0004-637X/697/1/730},
   Key = {Thrane:2009fj}
}

@article{:2009dpa,
   Author = {Fechner, M and Abe, K and Hayato, Y and Iida, T and Ikeda, M and Kameda, J and Kobayashi, K and Koshio, Y and Miura, M and Moriyama, S and Nakahata, M and Nakayama, S and Obayashi, Y and Ogawa, H and Sekiya, H and Shiozawa, M and Suzuki, Y and Takeda, A and Takenaga, Y and Takeuchi, Y and Ueno, K and Ueshima, K and Watanabe, H and Yamada, S and Hazama, S and Higuchi, I and Ishihara, C and Kajita, T and Kaneyuki, K and Mitsuka, G and Nishino, H and Okumura, K and Tanimoto, N and Vagins, MR and Dufour, F and Kearns, E and Litos, M and Raaf, JL and Stone, JL and Sulak, LR and Wang, W and Goldhaber, M and Dazeley, S et al.},
   Title = {Kinematic reconstruction of atmospheric neutrino events in a
             large water Cherenkov detector with proton
             identification},
   Journal = {Physical Review D - Particles, Fields, Gravitation, and
             Cosmology},
   Volume = {79},
   Number = {11},
   Pages = {112010},
   Year = {2009},
   ISSN = {1550-7998},
   url = {http://arxiv.org/pdf/0901.1645},
   Abstract = {We report the development of a proton identification method
             for the Super-Kamiokande (SK) detector. This new tool is
             applied to the search for events with a single proton track,
             a high purity neutral current sample of interest for sterile
             neutrino searches. After selection using a neural network,
             we observe 38 events in the combined SK-I and SK-II data
             corresponding to 2285.1 days of exposure, with an estimated
             signal-to-background ratio of 1.6 to 1. Proton
             identification was also applied to a direct search for
             charged-current quasielastic (CCQE) events, obtaining a high
             precision sample of fully kinematically reconstructed
             atmospheric neutrinos, which has not been previously
             reported in water Cherenkov detectors. The CCQE fraction of
             this sample is 55%, and its neutrino (as opposed to
             antineutrino) fraction is 91.7±3%. We selected 78μ-like
             and 47 e-like events in the SK-I and SK-II data set. With
             this data, a clear zenith angle distortion of the neutrino
             direction itself is reported in a sub-GeV sample of μ
             neutrinos where the lepton angular correlation to the
             incoming neutrino is weak. Our fit to νμ→ντ
             oscillations using the neutrino LE distribution of the CCQE
             sample alone yields a wide acceptance region compatible with
             our previous results and excludes the no-oscillation
             hypothesis at 3-sigma. © 2009 The American Physical
             Society.},
   Doi = {10.1103/PhysRevD.79.112010},
   Key = {:2009dpa}
}

@article{Fechner:2009mq,
   Author = {Fechner, M and Walter, CW},
   Title = {The physics impact of proton track identification in future
             megaton-scale water Cherenkov detectors},
   Journal = {Journal of High Energy Physics},
   Volume = {2009},
   Number = {11},
   Pages = {040},
   Year = {2009},
   ISSN = {1126-6708},
   url = {http://arxiv.org/pdf/0901.1950},
   Abstract = {In this paper, we investigate the impact in future
             megaton-scale water Cherenkov detectors of identifying
             proton Cherenkov rings. We estimate the expected event rates
             for detected neutral current and charged current
             quasi-elastic neutrino interactions from atmospheric
             neutrinos in a megaton-scale Super-Kamiokande-like detector
             with both 40% and 20% photo-cathode coverage. With this
             sample we examine the prospects for measuring the neutrino
             oscillation pattern, and searching for sterile neutrinos. We
             also determine the size of selected charged current
             quasi-elastic samples in a 300-kton fiducial volume
             Super-Kamiokande-like detector from examples of both
             conventional super-beams and beta-beams proposed in the
             literature. With these samples, it is shown that full
             kinematic neutrino reconstruction using the outgoing proton
             can improve the reconstructed energy resolution, and give
             good neutrino versus anti-neutrino tagging capabilities,
             adding important capabilities to water Cherenkov detectors
             in future projects. We determine the beam parameters
             necessary to make use of this technique and present
             distributions of neutrino and anti-neutrino selection
             efficiencies. © 2009 SISSA.},
   Doi = {10.1088/1126-6708/2009/11/040},
   Key = {Fechner:2009mq}
}

@article{Walter:2008ar,
   Author = {Walter, Christopher W.},
   Title = {Experimental Neutrino Physics},
   Booktitle = {Proceeding of the XXXIV International Conference on High
             Energy Physics (ICHEP08), University of Pennsylvania, USA,
             August, 2008},
   Year = {2008},
   url = {http://arxiv.org/pdf/0810.3937},
   Abstract = {http://arxiv.org/abs/0810.3937},
   Key = {Walter:2008ar}
}

@article{Hernandez:2008zza,
   Author = {Hernández, P and Walter, CW and Yasuda, O},
   Title = {Summary of working group one},
   Journal = {AIP Conference Proceedings},
   Volume = {981},
   Pages = {135-138},
   Year = {2008},
   ISSN = {0094-243X},
   url = {http://dx.doi.org/10.1063/1.2898909},
   Abstract = {The theoretical and experimental issues discussed in working
             group one at Nufact07 are summarized. © 2008 American
             Institute of Physics.},
   Doi = {10.1063/1.2898909},
   Key = {Hernandez:2008zza}
}

@article{fds248719,
   Author = {Choubey, S and Hernández, P and Walter, CW},
   Title = {Summary of working group I: Theory},
   Journal = {10th International Workshop on Neutrino Factories, Super
             Beams and Beta Beams, NUFACT08},
   Year = {2008},
   Abstract = {We present the highlights of the parallel sessions of
             Working Group I at Nufact08. © owned by the
             author.},
   Key = {fds248719}
}

@article{fds304631,
   Author = {Mine, S and Alcaraz, JL and Andringa, S and Aoki, S and Argyriades, J and Asakura, K and Ashie, R and Berghaus, F and Berns, H and Bhang, H and Blondel, A and Borghi, S and Bouchez, J and Burguet-Castell, J and Casper, D and Catala, J and Cavata, C and Cervera, A and Chen, SM and Cho,
             KO and Choi, JH and Dore, U and Espinal, X and Fechner, M and Fernandez, E and Fujii, Y and Fukuda, Y and Gomez-Cadenas, J and Gran, R and Hara, T and Hasegawa, M and Hasegawa, T and Hayato, Y and Helmer, RL and Hiraide, K and Hosaka, J and Ichikawa, AK and Iinuma, M and Ikeda, A and Ishida, T and Ishihara, K and Ishii, T et al.},
   Title = {Experimental study of the atmospheric neutrino backgrounds
             for p→e+π0 searches in water Cherenkov
             detectors},
   Journal = {Physical Review D - Particles, Fields, Gravitation, and
             Cosmology},
   Volume = {77},
   Number = {3},
   Year = {2008},
   ISSN = {1550-7998},
   url = {http://dx.doi.org/10.1103/PhysRevD.77.032003},
   Abstract = {The atmospheric neutrino background for proton decay via
             p→e+π0 in ring imaging water Cherenkov detectors is
             studied with an artificial accelerator neutrino beam for the
             first time. In total, 3.14×105 neutrino events
             corresponding to about 10 megaton-years of atmospheric
             neutrino interactions were collected by a 1000 ton water
             Cherenkov detector (KT). The KT charged-current single π0
             production data are well reproduced by simulation programs
             of neutrino and secondary hadronic interactions used in the
             Super-Kamiokande (SK) proton decay search. The obtained
             p→e+π0 background rate by the KT data for SK from the
             atmospheric neutrinos whose energies are below 3 GeV is
             1.63-0.33+0.42(stat)-0.51+0.45(syst)(megaton-year)- 1. This
             result is also relevant to possible future, megaton-scale
             water Cherenkov detectors. © 2008 The American Physical
             Society.},
   Doi = {10.1103/PhysRevD.77.032003},
   Key = {fds304631}
}

@article{Mine:2008rt,
   Author = {Mine, and S, and others},
   Title = {Experimental study of the atmospheric neutrino backgrounds
             for proton decay to positron and neutral pion searches in
             water Cherenkov detectors},
   Journal = {Phys. Rev.},
   Volume = {D77},
   Number = {3},
   Pages = {032003},
   Year = {2008},
   ISSN = {1550-7998},
   url = {http://arxiv.org/pdf/0801.0182},
   Abstract = {http://arxiv.org/abs/0801.0182},
   Doi = {10.1103/PhysRevD.77.032003},
   Key = {Mine:2008rt}
}

@article{Abe:2008zza,
   Author = {Abe, K and Hayato, Y and Iida, T and Ikeda, M and Kameda, J and Koshio, Y and Minamino, A and Miura, M and Moriyama, S and Nakahata, M and Nakayama,
             S and Obayashi, Y and Ogawa, H and Sekiya, H and Shiozawa, M and Suzuki, Y and Takeda, A and Takeuchi, Y and Ueshima, K and Watanabe, H and Yamada, S and Higuchi, I and Ishihara, C and Kajita, T and Kaneyuki, K and Mitsuka, G and Nishino, H and Okumura, K and Saji, C and Takenaga, Y and Clark, S and Desai, S and Dufour, F and Kearns, E and Likhoded, S and Litos, M and Raaf,
             JL and Stone, JL and Sulak, LR and Wang, W and Goldhaber, M and Casper, D and Cravens, JP et al.},
   Title = {Search for matter-dependent atmospheric neutrino
             oscillations in Super-Kamiokande},
   Journal = {Physical Review D - Particles, Fields, Gravitation, and
             Cosmology},
   Volume = {77},
   Number = {5},
   Pages = {052001},
   Year = {2008},
   ISSN = {1550-7998},
   url = {http://arxiv.org/pdf/0801.0776},
   Abstract = {We consider νμ→ντ oscillations in the context of the
             mass varying neutrino (MaVaN) model, where the neutrino mass
             can vary depending on the electron density along the flight
             path of the neutrino. Our analysis assumes a mechanism with
             dependence only upon the electron density, hence ordinary
             matter density, of the medium through which the neutrino
             travels. Fully-contained, partially-contained and
             upward-going muon atmospheric neutrino data from the
             Super-Kamiokande detector, taken from the entire SK-I period
             of 1489 live days, are compared to MaVaN model predictions.
             We find that, for the case of 2-flavor oscillations, and for
             the specific models tested, oscillation independent of
             electron density is favored over density dependence.
             Assuming maximal mixing, the best-fit case and the
             density-independent case do not differ significantly. ©
             2008 The American Physical Society.},
   Doi = {10.1103/PhysRevD.77.052001},
   Key = {Abe:2008zza}
}

@article{Desai:2007ra,
   Author = {Desai, S and Abe, K and Hayato, Y and Iida, K and Ishihara, K and Kameda,
             J and Koshio, Y and Minamino, A and Mitsuda, C and Miura, M and Moriyama,
             S and Nakahata, M and Obayashi, Y and Ogawa, H and Shiozawa, M and Suzuki,
             Y and Takeda, A and Takeuchi, Y and Ueshima, K and Watanabe, H and Yamada,
             S and Higuchi, I and Ishihara, C and Ishitsuka, M and Kajita, T and Kaneyuki, K and Mitsuka, G and Nakayama, S and Nishino, H and Okumura,
             K and Saji, C and Takenaga, Y and Clark, ST and Dufour, F and Kearns, E and Likhoded, S and Raaf, JL and Stone, JL and Sulak, LR and Wang, W and Goldhaber, M and Casper, D and Cravens, JP et al.},
   Title = {Study of TeV neutrinos with upward showering muons in
             Super-Kamiokande},
   Journal = {Astroparticle Physics},
   Volume = {29},
   Number = {1},
   Pages = {42-54},
   Year = {2008},
   ISSN = {0927-6505},
   url = {http://arxiv.org/pdf/0711.0053},
   Abstract = {A subset of neutrino-induced upward through-going muons in
             the Super-Kamiokande detector consists of high-energy muons
             which lose energy through radiative processes such as
             bremsstrahlung, e+ e- pair production and photonuclear
             interactions. These "upward showering muons" comprise an
             event sample whose mean parent neutrino energy is
             approximately 1 TeV. We show that the zenith angle
             distribution of upward showering muons is consistent with
             negligible distortion due to neutrino oscillations, as
             expected of such a high-energy neutrino sample. We present
             astronomical searches using these high-energy events, such
             as those from WIMP annihilations in the Sun, Earth and
             Galactic Center, some suspected point sources, as well as
             searches for diffuse flux from the interstellar medium. ©
             2007 Elsevier B.V. All rights reserved.},
   Doi = {10.1016/j.astropartphys.2007.11.005},
   Key = {Desai:2007ra}
}

@article{:2008zn,
   Author = {Cravens, JP and Abe, K and Iida, T and Ishihara, K and Kameda, J and Koshio, Y and Minamino, A and Mitsuda, C and Miura, M and Moriyama, S and Nakahata, M and Nakayama, S and Obayashi, Y and Ogawa, H and Sekiya, H and Shiozawa, M and Suzuki, Y and Takeda, A and Takeuchi, Y and Ueshima, K and Watanabe, H and Yamada, S and Higuchi, I and Ishihara, C and Ishitsuka,
             M and Kajita, T and Kaneyuki, K and Mitsuka, G and Nishino, H and Okumura,
             K and Saji, C and Takenaga, Y and Clark, S and Desai, S and Dufour, F and Kearns, E and Likhoded, S and Litos, M and Raaf, JL and Stone, JL and Sulak, LR and Wang, W and Goldhaber, M et al.},
   Title = {Solar neutrino measurements in Super-Kamiokande-II},
   Journal = {Physical Review D - Particles, Fields, Gravitation, and
             Cosmology},
   Volume = {78},
   Number = {3},
   Pages = {032002},
   Year = {2008},
   ISSN = {1550-7998},
   url = {http://arxiv.org/pdf/0803.4312},
   Abstract = {The results of the second phase of the Super-Kamiokande
             solar neutrino measurement are presented and compared to the
             first phase. The solar neutrino flux spectrum and time
             variation as well as oscillation results are statistically
             consistent with the first phase and do not show spectral
             distortion. The time-dependent flux measurement of the
             combined first and second phases coincides with the full
             period of solar cycle 23 and shows no correlation with solar
             activity. The measured B8 total flux is (2.38±0.05(stat.)-0.15+0.16(sys.))×106cm-2s-1
             and the day-night difference is found to be
             (-6.3±4.2(stat.)±3.7(sys.))%. There is no evidence of
             systematic tendencies between the first and second phases.
             © 2008 The American Physical Society.},
   Doi = {10.1103/PhysRevD.78.032002},
   Key = {:2008zn}
}

@article{fds287699,
   Author = {Rodriguez, A and Whitehead, L and Alcaraz, JL and Andringa, S and Aoki,
             S and Argyriades, J and Asakura, K and Ashie, R and Berghaus, F and Berns,
             H and Bhang, H and Blondel, A and Borghi, S and Bouchez, J and Burguet-Castell, J and Casper, D and Catala, J and Cavata, C and Cervera, A and Chen, SM and Cho, KO and Choi, JH and Dore, U and Espinal,
             X and Fechner, M and Fernandez, E and Fujii, Y and Fukuda, Y and Gomez-Cadenas, J and Gran, R and Hara, T and Hasegawa, M and Hasegawa,
             T and Hayato, Y and Helmer, RL and Hiraide, K and Hosaka, J and Ichikawa,
             AK and Iinuma, M and Ikeda, A and Ishida, T and Ishihara, K et
             al.},
   Title = {Measurement of single charged pion production in the
             charged-current interactions of neutrinos in a 1.3GeV wide
             band beam},
   Journal = {Physical Review D - Particles, Fields, Gravitation, and
             Cosmology},
   Volume = {78},
   Number = {3},
   Year = {2008},
   ISSN = {1550-7998},
   url = {http://dx.doi.org/10.1103/PhysRevD.78.032003},
   Abstract = {Single charged pion production in charged-current muon
             neutrino interactions with carbon is studied using data
             collected in the K2K long-baseline neutrino experiment. The
             mean energy of the incident muon neutrinos is 1.3 GeV. The
             data used in this analysis are mainly from a fully active
             scintillator detector, SciBar. The cross section for single
             π+ production in the resonance region (W&lt;2GeV/c2)
             relative to the charged-current quasielastic cross section
             is found to be 0.734-0.153+0.140. The energy-dependent cross
             section ratio is also measured. The results are consistent
             with a previous experiment and the prediction of our model.
             © 2008 The American Physical Society.},
   Doi = {10.1103/PhysRevD.78.032003},
   Key = {fds287699}
}

@article{fds318497,
   Author = {Danzer, SC and Kotloski, RJ and Walter, C and Hughes, M and McNamara,
             JO},
   Title = {Altered morphology of hippocampal dentate granule cell
             presynaptic and postsynaptic terminals following conditional
             deletion of TrkB},
   Journal = {Hippocampus},
   Volume = {18},
   Number = {7},
   Pages = {668-678},
   Year = {2008},
   url = {http://dx.doi.org/10.1002/hipo.20426},
   Abstract = {Dentate granule cells play a critical role in the function
             of the entorhinal-hippocampal circuitry in health and
             disease. Dentate granule cells are situated to regulate the
             flow of information into the hippocampus, a structure
             required for normal learning and memory. Correspondingly,
             impaired granule cell function leads to memory deficits,
             and, interestingly, altered granule cell connectivity may
             contribute to the hyperexcitability of limbic epilepsy. It
             is important, therefore, to understand the molecular
             determinants of synaptic connectivity of these neurons.
             Brain-derived neurotrophic factor and its receptor TrkB are
             expressed at high levels in the dentate gyrus (DG) of the
             hippocampus, and are implicated in regulating neuronal
             development, neuronal plasticity, learning, and the
             development of epilepsy. Whether and how TrkB regulates
             granule cell structure, however, is incompletely understood.
             To begin to elucidate the role of TrkB in regulating granule
             cell morphology, here we examine conditional TrkB knockout
             mice crossed to mice expressing green fluorescent protein in
             subsets of dentate granule cells. In stratum lucidum, where
             granule cell mossy fiber axons project, the density of giant
             mossy fiber boutons was unchanged, suggesting similar output
             to CA3 pyramidal cell targets. However, filopodial
             extensions of giant boutons, which contact inhibitory
             interneurons, were increased in number in TrkB knockout mice
             relative to wildtype controls, predicting enhanced
             feedforward inhibition of CA3 pyramidal cells. In knockout
             animals, dentate granule cells possessed fewer primary
             dendrites and enlarged dendritic spines, indicative of
             disrupted excitatory synaptic input to the granule cells.
             Together, these findings demonstrate that TrkB is required
             for development and/or maintenance of normal synaptic
             connectivity of the granule cells, thereby implying an
             important role for TrkB in the function of the granule cells
             and hippocampal circuitry. © 2008 Wiley-Liss,
             Inc.},
   Doi = {10.1002/hipo.20426},
   Key = {fds318497}
}

@inproceedings{Walter:2007wf,
   Author = {Walter, CW},
   Title = {Why understanding neutrino interactions is important for
             oscillation physics},
   Journal = {AIP Conference Proceedings},
   Volume = {967},
   Pages = {3-8},
   Booktitle = {Proceedings of 5th International Workshop on
             Neutrino-Nucleus Interactions in the Few-GeV Region
             (NuInt07)},
   Year = {2007},
   ISSN = {0094-243X},
   url = {http://arxiv.org/pdf/arXiv:0709.3616 [hep-ex]},
   Abstract = {Uncertainties in knowledge of neutrino interactions directly
             impact the ability measure the parameters of neutrino
             oscillation. Experiments which make use of differing
             technologies and neutrino beams are sensitive to different
             uncertainties. © 2007 American Institute of
             Physics.},
   Doi = {10.1063/1.2834507},
   Key = {Walter:2007wf}
}

@article{Takenaga:2006nr,
   Author = {Takenaga, Y and Abe, K and Hayato, Y and Iida, T and Ishihara, K and Kameda, J and Koshio, Y and Minamino, A and Mitsuda, C and Miura, M and Moriyama, S and Nakahata, M and Obayashi, Y and Ogawa, H and Shiozawa,
             M and Suzuki, Y and Takeda, A and Takeuchi, Y and Ueshima, K and Watanabe,
             H and Yamada, S and Higuchi, I and Ishihara, C and Ishitsuka, M and Kajita,
             T and Kaneyuki, K and Mitsuka, G and Nakayama, S and Nishino, H and Okumura, K and Saji, C and Totsuka, Y and Clark, S and Desai, S and Dufour,
             F and Herfurth, A and Kearns, E and Likhoded, S and Litos, M and Raaf, JL and Stone, JL and Sulak, LR and Wang, W et al.},
   Title = {Search for neutral Q-balls in Super-Kamiokande
             II},
   Journal = {Physics Letters B},
   Volume = {647},
   Number = {1},
   Pages = {18-22},
   Year = {2007},
   ISSN = {0370-2693},
   url = {http://arxiv.org/pdf/hep-ex/0608057},
   Abstract = {A search for Q-balls has been carried out in
             Super-Kamiokande II with 541.7 days of live time. A neutral
             Q-ball passing through the detector can interact with nuclei
             to produce pions, generating a signal of successive
             contained pion events along a track. No candidate for
             successive contained event groups has been found in
             Super-Kamiokande II, so we obtain upper limits on the flux
             of such Q-balls. © 2007 Elsevier B.V. All rights
             reserved.},
   Doi = {10.1016/j.physletb.2007.01.047},
   Key = {Takenaga:2006nr}
}

@article{fds248743,
   Author = {Guillian, G and Hosaka, J and Ishihara, K and Kameda, J and Koshio, Y and Minamino, A and Mitsuda, C and Miura, M and Moriyama, S and Nakahata, M and Namba, T and Obayashi, Y and Ogawa, H and Shiozawa, M and Suzuki, Y and Takeda, A and Takeuchi, Y and Yamada, S and Higuchi, I and Ishitsuka, M and Kajita, T and Kaneyuki, K and Mitsuka, G and Nakayama, S and Nishino, H and Okada, A and Okumura, K and Saji, C and Takenaga, Y and Desai, S and Kearns, E and Stone, JL and Sulak, LR and Wang, W and Goldhaber, M and Casper, D and Gajewski, W and Griskevich, J and Kropp, WR and Liu, DW and Mine, S and Smy, MB and Sobel, HW et al.},
   Title = {Observation of the anisotropy of 10 TeV primary cosmic ray
             nuclei flux with the Super-Kamiokande-I detector},
   Journal = {Physical Review D - Particles, Fields, Gravitation, and
             Cosmology},
   Volume = {75},
   Number = {6},
   Year = {2007},
   ISSN = {1550-7998},
   url = {http://dx.doi.org/10.1103/PhysRevD.75.062003},
   Abstract = {The relative sidereal variation in the arrival direction of
             primary cosmic ray nuclei of median energy 10 TeV was
             measured using downward, through-going muons detected with
             the Super-Kamiokande-I detector. The projection of the
             anisotropy map onto the right ascension axis has a first
             harmonic amplitude of (6.64±0.98stat±0.55syst)×10-4 and a
             phase at maximum at (33.2°±8.2°stat±5.1°syst) right
             ascension. A sky map in equatorial coordinates indicates an
             excess region in the constellation of Taurus and a deficit
             region toward Virgo. The excess region is centered at
             (αT,δT)=(75°±7°,-5°±9°) with a half-opening angle
             χT=(39±7)°; the excess flux is (0.104±0.020)% above the
             isotropic expectation. The corresponding parameters for the
             deficit region are (αV,δV)= (205°±7°,5°±10°),
             χV=(54±7)°, and (-0.094±0.014)%. The data do not allow
             us to rule out a pure dipole form for the anisotropy
             (allowed at 13% confidence level); they are better described
             by the excess and deficit cones described above. We explored
             the implications under the assumption that the true
             anisotropy is not distorted too much by the analysis filter
             so that it is well-described by the observed excess and
             deficit cones. © 2007 The American Physical
             Society.},
   Doi = {10.1103/PhysRevD.75.062003},
   Key = {fds248743}
}

@article{Ikeda:2007sa,
   Author = {Ikeda, M and Takeda, A and Fukuda, Y and Vagins, MR and Abe, K and Iida, T and Ishihara, K and Kameda, J and Koshio, Y and Minamino, A and Mitsuda, C and Miura, M and Moriyama, S and Nakahata, M and Obayashi, Y and Ogawa, H and Sekiya, H and Shiozawa, M and Suzuki, Y and Takeuchi, Y and Ueshima, K and Watanabe, H and Yamada, S and Higuchi, I and Ishihara, C and Ishitsuka,
             M and Kajita, T and Kaneyuki, K and Mitsuka, G and Nakayama, S and Nishino,
             H and Okumura, K and Saji, C and Takenaga, Y and Clark, S and Desai, S and Dufour, F and Kearns, E and Likhoded, S and Litos, M and Raaf, JL and Stone, JL and Sulak, LR et al.},
   Title = {Search for supernova neutrino bursts at super-kamiokande},
   Journal = {The Astrophysical Journal},
   Volume = {669},
   Number = {1},
   Pages = {519-524},
   Year = {2007},
   ISSN = {0004-637X},
   url = {http://arxiv.org/pdf/arXiv:0706.2283 [astro-ph]},
   Abstract = {We report the results of a search for neutrino bursts from
             supernova explosions using the Super-Kamiokande detector.
             Super-Kamiokande is sensitive to core-collapse supernova
             explosions via observation of their neutrino emissions. The
             expected number of events comprising such a burst is ∼104,
             and the average energy of the neutrinos is in the range of a
             few tens of MeV for a core-collapse supernova explosion at a
             typical distance in our galaxy (10 kpc); this strong signal
             means that the detection efficiency anywhere within our
             galaxy and well past the Magellanic Clouds should be 100%.
             We examined a data set taken from 1996 May to 2001 July, and
             from 2002 December to 2005 October, corresponding to 2589.2
             live days. However, there is no evidence of such a supernova
             explosion during the data-taking period. The 90% CL. upper
             limit on the rate of core-collapse supernova explosions out
             to distances of 100 kpc is found to be 0.32 SN yr-1. ©
             2007. The American Astronomical Society. All rights
             reserved.},
   Doi = {10.1086/521547},
   Key = {Ikeda:2007sa}
}

@article{Abe:2006fu,
   Author = {Abe, K and Hayato, Y and Iida, T and Ishihara, K and Kameda, J and Koshio,
             Y and Minamino, A and Mitsuda, C and Miura, M and Moriyama, S and Nakahata,
             M and Obayashi, Y and Ogawa, H and Shiozawa, M and Suzuki, Y and Takeda, A and Takeuchi, Y and Ueshima, K and Higuchi, I and Ishihara, C and Ishitsuka,
             M and Kajita, T and Kaneyuki, K and Mitsuka, G and Nakayama, S and Nishino,
             H and Okumura, K and Saji, C and Takenaga, Y and Totsuka, Y and Clark, S and Desai, S and Dufour, F and Kearns, E and Likhoded, S and Litos, M and Raaf,
             JL and Stone, JL and Sulak, LR and Wang, W and Goldhaber, M and Casper, D and Cravens, JP et al.},
   Title = {Measurement of atmospheric neutrino flux consistent with tau
             neutrino appearance.},
   Journal = {Physical Review Letters},
   Volume = {97},
   Number = {17},
   Pages = {171801},
   Year = {2006},
   Month = {October},
   ISSN = {0031-9007},
   url = {http://www.ncbi.nlm.nih.gov/pubmed/17155460},
   Abstract = {A search for the appearance of tau neutrinos from nu(mu)
             <--> nu(tau) oscillations in the atmospheric neutrinos has
             been performed using 1489.2 days of atmospheric neutrino
             data from the Super-Kamiokande-I experiment. A best fit tau
             neutrino appearance signal of 138+/-48(stat)-32(+15)(syst)
             events is obtained with an expectation of 78+/-26(syst). The
             hypothesis of no tau neutrino appearance is disfavored by
             2.4 sigma.},
   Doi = {10.1103/PhysRevLett.97.171801},
   Key = {Abe:2006fu}
}

@article{fds304630,
   Author = {Yamamoto, S and Zalipska, J and Aliu, E and Andringa, S and Aoki, S and Argyriades, J and Asakura, K and Ashie, R and Berghaus, F and Berns, H and Bhang, H and Blondel, A and Borghi, S and Bouchez, J and Burguet-Castell, J and Casper, D and Catala, J and Cavata, C and Cervera, A and Chen, SM and Cho, KO and Choi, JH and Dore, U and Espinal,
             X and Fechner, M and Fernandez, E and Fukuda, Y and Gomez-Cadenas, J and Gran, R and Hara, T and Hasegawa, M and Hasegawa, T and Hayashi, K and Hayato, Y and Helmer, RL and Hiraide, K and Hosaka, J and Ichikawa, AK and Iinuma, M and Ikeda, A and Inagaki, T and Ishida, T et
             al.},
   Title = {Improved search for nu(mu) --> nu(e) oscillation in a
             long-baseline accelerator experiment.},
   Journal = {Physical Review Letters},
   Volume = {96},
   Number = {18},
   Pages = {181801},
   Year = {2006},
   Month = {May},
   ISSN = {0031-9007},
   url = {http://www.ncbi.nlm.nih.gov/pubmed/16712358},
   Abstract = {We performed an improved search for nu(mu) --> nu(e)
             oscillation with the KEK to Kamioka (K2K) long-baseline
             neutrino oscillation experiment, using the full data sample
             of 9.2 x 10(19) protons on target. No evidence for a nu(e)
             appearance signal was found, and we set bounds on the nu(mu)
             --> nu(e) oscillation parameters. At Deltam(2)=2.8 x 10(-3)
             eV(2), the best-fit value of the K2Knu(mu) disappearance
             analysis, we set an upper limit of sin(2)2theta(mue) < 0.13
             at a 90% confidence level.},
   Doi = {10.1103/PhysRevLett.96.181801},
   Key = {fds304630}
}

@article{fds248703,
   Author = {Cravens, P and Hosaka, J and Ishihara, K and Kameda, J and Koshio, Y and Minamino, A and Mitsuda, G and Miura, M and Moriyama, S and Nakahata, M and Namba, T and Obayashi, Y and Shiozawa, M and Suzuki, Y and Takeda, A and Takeuchi, Y and Yamada, S and Higuchi, I and Ishitsuka, M and Kajita, T and Kaneyuki, K and Mitsuka, G and Nakayama, S and Nishino, H and Okada, A and Okumura, K and Saji, C and Takenaga, Y and Clark, S and Desai, S and Kearns, E and Likhoded, S and Stone, JL and Sulak, LR and Wang, W and Goldhaber, M and Casper, D and Cravens, JP and Kropp, WR and Liu, DW and Mine, S and Regis, C and Smy, MB et al.},
   Title = {Current status of solar neutrinos at super-kamiokande},
   Journal = {Annual Meeting of the Division of Particles and Fields of
             the American Physical Society, DPF 2006, and the Annual Fall
             Meeting of the Japan Particle Physics Community},
   Publisher = {American Physical Society},
   Year = {2006},
   Abstract = {• SK-III has been started and is taking data • SK-II
             data has been updated to its final 791d • Oscillation
             analysis with SK-I, SK-II data has been performed and shows
             consistency with final SK-I data set • SK-II shows
             consistency within the global analysis • Hope to see
             energy spectrum distortion in SK-III.},
   Key = {fds248703}
}

@article{Hosaka:2005um,
   Author = {Hosaka, J and Ishihara, K and Kameda, J and Koshio, Y and Minamino, A and Mitsuda, C and Miura, M and Moriyama, S and Nakahata, M and Namba, T and Obayashi, Y and Sakurai, N and Sarrat, A and Shiozawa, M and Suzuki, Y and Takeuchi, Y and Yamada, S and Higuchi, I and Ishitsuka, M and Kajita, T and Kaneyuki, K and Mitsuka, G and Nakayama, S and Nishino, H and Okada, A and Okumura, K and Saji, C and Takenaga, Y and Clark, S and Desai, S and Kearns, E and Likhoded, S and Stone, JL and Sulak, LR and Wang, W and Goldhaber, M and Casper, D and Cravens, JP and Kropp, WR and Liu, DW and Mine, S and Smy, MB and Sobel, HW et al.},
   Title = {Solar neutrino measurements in Super-Kamiokande-I},
   Journal = {Physical Review D - Particles, Fields, Gravitation, and
             Cosmology},
   Volume = {73},
   Number = {11},
   Pages = {112001},
   Year = {2006},
   ISSN = {1550-7998},
   url = {http://arxiv.org/pdf/hep-ex/0508053},
   Abstract = {The details of Super-Kamiokande-I's solar neutrino analysis
             are given. Solar neutrino measurement in Super-Kamiokande is
             a high statistics collection of B8 solar neutrinos via
             neutrino-electron scattering. The analysis method and
             results of the 1496 day data sample are presented. The final
             oscillation results for the data are presented also. © 2006
             The American Physical Society.},
   Doi = {10.1103/PhysRevD.73.112001},
   Key = {Hosaka:2005um}
}

@article{Swanson:2006gm,
   Author = {Swanson, MEC and Abe, K and Hosaka, J and Iida, T and Ishihara, K and Kameda, J and Koshio, Y and Minamino, A and Mitsuda, C and Miura, M and Moriyama, S and Nakahata, M and Obayashi, Y and Ogawa, H and Shiozawa,
             M and Suzuki, Y and Takeda, A and Takeuchi, Y and Ueshima, K and Higuchi,
             I and Ishihara, C and Ishitsuka, M and Kajita, T and Kaneyuki, K and Mitsuka, G and Nakayama, S and Nishino, H and Okada, A and Okumura, K and Saji, C and Takenaga, Y and Clark, S and Desai, S and Dufour, F and Kearns,
             E and Likhoded, S and Litos, M and Raaf, JL and Stone, JL and Sulak, LR and Wang, W and Goldhaber, M and Casper, D et al.},
   Title = {Search for diffuse astrophysical neutrino flux using
             ultra-high-energy upward-going muons in super-kamiokande
             I},
   Journal = {The Astrophysical Journal},
   Volume = {652},
   Number = {1 I},
   Pages = {206-215},
   Year = {2006},
   ISSN = {0004-637X},
   url = {http://arxiv.org/pdf/astro-ph/0606126},
   Abstract = {Many astrophysical models predict a diffuse flux of
             high-energy neutrinos from active galactic nuclei and other
             extragalactic sources. At muon energies above 1 TeV, the
             upward-going muon flux induced by neutrinos from active
             galactic nuclei is expected to exceed the flux due to
             atmospheric neutrinos. We have performed a search for this
             astrophysical neutrino flux by looking for upward-going
             muons in the highest energy data sample from the
             Super-Kamiokande detector using 1679.6 live days of data. We
             found one extremely high energy upward-going muon event,
             compared with an expected atmospheric neutrino background of
             0.46 ± 0.23 events. Using this result, we set an upper
             limit on the diffuse flux of upward-going muons due to
             neutrinos from astrophysical sources in the muon energy
             range 3.16-100 TeV. © 2006. The American Astronomical
             Society. All rights reserved.},
   Doi = {10.1086/507983},
   Key = {Swanson:2006gm}
}

@article{Hosaka:2006zd,
   Author = {Hosaka, J and Ishihara, K and Kameda, J and Koshio, Y and Minamino, A and Mitsuda, C and Miura, M and Moriyama, S and Nakahata, M and Namba, T and Obayashi, Y and Shiozawa, M and Suzuki, Y and Takeda, A and Takeuchi, Y and Yamada, S and Higuchi, I and Ishitsuka, M and Kajita, T and Kaneyuki, K and Mitsuka, G and Nakayama, S and Nishino, H and Okada, A and Okumura, K and Saji, C and Takenaga, Y and Clark, S and Desai, S and Kearns, E and Likhoded, S and Stone, JL and Sulak, LR and Wang, W and Goldhaber, M and Casper, D and Cravens, JP and Kropp, WR and Liu, DW and Mine, S and Regis,
             C and Smy, MB and Sobel, HW et al.},
   Title = {Three flavor neutrino oscillation analysis of atmospheric
             neutrinos in Super-Kamiokande},
   Journal = {Physical Review D - Particles, Fields, Gravitation, and
             Cosmology},
   Volume = {74},
   Number = {3},
   Pages = {032002},
   Year = {2006},
   ISSN = {1550-7998},
   url = {http://arxiv.org/pdf/hep-ex/0604011},
   Abstract = {We report on the results of a three-flavor oscillation
             analysis using Super-Kamiokande I atmospheric neutrino data,
             with the assumption of one mass scale dominance (Δm122=0).
             No significant flux change due to matter effect, which
             occurs when neutrinos propagate inside the Earth for
             θ13≠0, has been seen either in a multi-GeV νe-rich
             sample or in a νμ-rich sample. Both normal and inverted
             mass hierarchy hypotheses are tested and both are consistent
             with observation. Using Super-Kamiokande data only,
             2-dimensional 90% confidence allowed regions are obtained:
             mixing angles are constrained to sin 2θ13&lt;0.14 and
             0.37&lt;sin 2θ23&lt;0.65 for the normal mass hierarchy.
             Weaker constraints, sin 2θ13&lt;0.27 and 0.37&lt;sin
             2θ23&lt;0.69, are obtained for the inverted mass hierarchy
             case. © 2006 The American Physical Society.},
   Doi = {10.1103/PhysRevD.74.032002},
   Key = {Hosaka:2006zd}
}

@article{Abe:2006at,
   Author = {Abe, K and Hosaka, J and Iida, T and Ishihara, K and Kameda, J and Koshio,
             Y and Minamino, A and Mitsuda, C and Miura, M and Moriyama, S and Nakahata,
             M and Obayashi, Y and Ogawa, H and Shiozawa, M and Suzuki, Y and Takeda, A and Takeuchi, Y and Higuchi, I and Ishihara, C and Ishitsuka, M and Kajita,
             T and Kaneyuki, K and Mitsuka, G and Nakayama, S and Nishino, H and Okada,
             A and Okumura, K and Saji, C and Takenaga, Y and Clark, S and Desai, S and Dufour, F and Kearns, E and Likhoded, S and Litos, M and Raaf, JL and Stone, JL and Sulak, LR and Wang, W and Goldhaber, M and Casper, D and Cravens, JP and Dunmore, J et al.},
   Title = {High-energy neutrino astronomy using upward-going MUONS in
             super-kamiokande I},
   Journal = {The Astrophysical Journal},
   Volume = {652},
   Number = {1 I},
   Pages = {198-205},
   Year = {2006},
   ISSN = {0004-637X},
   url = {http://arxiv.org/pdf/astro-ph/0606413},
   Abstract = {We present the results from several studies used to search
             for astrophysical sources of high-energy neutrinos using the
             Super-Kamiokande I (1996 April-2001 July) neutrino-induced
             upward-going muon data. The data set consists of 2359 events
             with minimum energy 1.6 GeV, of which 1892 are through-going
             and 467 stop within the detector. The results of several
             independent analyses are presented, including searches for
             point sources using directional and temporal information and
             a search for signatures of cosmic-ray interactions with the
             interstellar medium in the upward-going muons. No
             statistically significant evidence for point sources or any
             diffuse flux from the plane of the Galaxy was found, so
             specific limits on fluxes from likely point sources are
             calculated. The 90% confidence level (CL) upper limits on
             upward-going muon flux from astronomical sources that are
             located in the southern hemisphere and always under the
             horizon for Super-Kamiokande are ∼(1-4) × 10-15 cm-2 s-1.
             © 2006. The American Astronomical Society. All rights
             reserved.},
   Doi = {10.1086/508016},
   Key = {Abe:2006at}
}

@article{Ahn:2006zz,
   Author = {Ahn, MH and Aliu, E and Andringa, S and Aoki, S and Aoyama, Y and Argyriades, J and Asakura, K and Ashie, R and Berghaus, F and Berns, HG and Bhang, H and Blondel, A and Borghi, S and Bouchez, J and Boyd, SC and Burguet-Castell, J and Casper, D and Catala, J and Cavata, C and Cervera, A and Chen, SM and Cho, KO and Choi, JH and Dore, U and Echigo, S and Espinal, X and Fechner, M and Fernandez, E and Fujii, K and Fujii, Y and Fukuda, S and Fukuda, Y and Gomez-Cadenas, J and Gran, R and Hara, T and Hasegawa, M and Hasegawa, T and Hayashi, K and Hayato, Y and Helmer, RL and Higuchi, I and Hill, J and Hiraide, K et al.},
   Title = {Measurement of neutrino oscillation by the K2K
             experiment},
   Journal = {Physical Review D - Particles, Fields, Gravitation, and
             Cosmology},
   Volume = {74},
   Number = {7},
   Pages = {072003},
   Year = {2006},
   ISSN = {1550-7998},
   url = {http://arxiv.org/pdf/hep-ex/0606032},
   Abstract = {We present measurements of νμ disappearance in K2K, the
             KEK to Kamioka long-baseline neutrino oscillation
             experiment. One-hundred and twelve beam-originated neutrino
             events are observed in the fiducial volume of
             Super-Kamiokande with an expectation of 158.1-8.6+9.2 events
             without oscillation. A distortion of the energy spectrum is
             also seen in 58 single-ring muonlike events with
             reconstructed energies. The probability that the
             observations are explained by the expectation for no
             neutrino oscillation is 0.0015% (4.3σ). In a two-flavor
             oscillation scenario, the allowed Δm2 region at sin 22θ=1
             is between 1.9 and 3.5×10-3eV2 at the 90% C.L. with a
             best-fit value of 2.8×10-3eV2. © 2006 The American
             Physical Society.},
   Doi = {10.1103/PhysRevD.74.072003},
   Key = {Ahn:2006zz}
}

@article{Gran:2006jn,
   Author = {Gran, and R, and others},
   Title = {Measurement of the quasi-elastic axial vector mass in
             neutrino oxygen interactions},
   Journal = {Phys.Rev.D74},
   Volume = {D74},
   Pages = {052002},
   Year = {2006},
   url = {http://arxiv.org/pdf/hep-ex/0603034},
   Abstract = {http://arxiv.org/abs/hep-ex/0603034},
   Key = {Gran:2006jn}
}

@article{Yamamoto:2006ty,
   Author = {Yamamoto, and S, and others},
   Title = {An improved search for nu/mu -> nu/e oscillation in a
             long-baseline accelerator experiment},
   Journal = {Phys. Rev. Lett},
   Volume = {96},
   Number = {18},
   Pages = {181801},
   Year = {2006},
   ISSN = {0031-9007},
   url = {http://www.ncbi.nlm.nih.gov/pubmed/16712358},
   Abstract = {We performed an improved search for nu(mu) --> nu(e)
             oscillation with the KEK to Kamioka (K2K) long-baseline
             neutrino oscillation experiment, using the full data sample
             of 9.2 x 10(19) protons on target. No evidence for a nu(e)
             appearance signal was found, and we set bounds on the nu(mu)
             --> nu(e) oscillation parameters. At Deltam(2)=2.8 x 10(-3)
             eV(2), the best-fit value of the K2Knu(mu) disappearance
             analysis, we set an upper limit of sin(2)2theta(mue) < 0.13
             at a 90% confidence level.},
   Doi = {10.1103/PhysRevLett.96.181801},
   Key = {Yamamoto:2006ty}
}

@article{fds287698,
   Author = {Gran, R and Jeon, EJ and Aliu, E and Andringa, S and Aoki, S and Argyriades, J and Asakura, K and Ashie, R and Berghaus, F and Berns, H and Bhang, H and Blondel, A and Borghi, S and Bouchez, J and Burguet-Castell, J and Casper, D and Catala, J and Cavata, C and Cervera, A and Chen, SM and Cho, KO and Choi, JH and Dore, U and Espinal,
             X and Fechner, M and Fernandez, E and Fukuda, Y and Gomez-Cadenas, J and Hara, T and Hasegawa, M and Hasegawa, T and Hayashi, K and Hayato, Y and Helmer, RL and Hiraide, K and Hosaka, J and Ichikawa, AK and Iinuma, M and Ikeda, A and Inagaki, T and Ishida, T and Ishihara, K and Ishii, T et
             al.},
   Title = {Measurement of the quasielastic axial vector mass in
             neutrino interactions on oxygen},
   Journal = {Physical Review D - Particles, Fields, Gravitation, and
             Cosmology},
   Volume = {74},
   Number = {5},
   Year = {2006},
   ISSN = {1550-7998},
   url = {http://dx.doi.org/10.1103/PhysRevD.74.052002},
   Abstract = {The weak nucleon axial-vector form factor for quasielastic
             interactions is determined using neutrino interaction data
             from the K2K Scintillating Fiber detector in the neutrino
             beam at KEK. More than 12000 events are analyzed, of which
             half are charged-current quasielastic interactions
             νμn→μ-p occurring primarily in oxygen nuclei. We use a
             relativistic Fermi gas model for oxygen and assume the form
             factor is approximately a dipole with one parameter, the
             axial-vector mass MA, and fit to the shape of the
             distribution of the square of the momentum transfer from the
             nucleon to the nucleus. Our best fit result for
             MA=1.20±0.12GeV. Furthermore, this analysis includes
             updated vector form factors from recent electron scattering
             experiments and a discussion of the effects of the nucleon
             momentum on the shape of the fitted distributions. © 2006
             The American Physical Society.},
   Doi = {10.1103/PhysRevD.74.052002},
   Key = {fds287698}
}

@article{Hasegawa:2005td,
   Author = {Hasegawa, M and Aliu, E and Andringa, S and Aoki, S and Argyriades, J and Asakura, K and Ashie, R and Berns, H and Bhang, H and Blondel, A and Borghi, S and Bouchez, J and Burguet-Castell, J and Casper, D and Cavata, C and Cervera, A and Chen, SM and Cho, KO and Choi, JH and Dore, U and Espinal, X and Fechner, M and Fernandez, E and Fukuda, Y and Gomez-Cadenas, J and Gran, R and Hara, T and Hasegawa, T and Hayashi, K and Hayato, Y and Helmer, RL and Hill, J and Hiraide, K and Hosaka, J and Ichikawa, AK and Iinuma, M and Ikeda, A and Inagaki, T and Ishida, T and Ishihara, K and Ishii, T and Ishitsuka, M and Itow, Y et
             al.},
   Title = {Search for coherent charged pion production in
             neutrino-carbon interactions.},
   Journal = {Physical Review Letters},
   Volume = {95},
   Number = {25},
   Pages = {252301},
   Year = {2005},
   Month = {December},
   ISSN = {0031-9007},
   url = {http://www.ncbi.nlm.nih.gov/pubmed/16384451},
   Abstract = {We report the result from a search for charged-current
             coherent pion production induced by muon neutrinos with a
             mean energy of 1.3 GeV. The data are collected with a fully
             active scintillator detector in the K2K long-baseline
             neutrino oscillation experiment. No evidence for coherent
             pion production is observed, and an upper limit of is set on
             the cross section ratio of coherent pion production to the
             total charged-current interaction at 90% confidence level.
             This is the first experimental limit for coherent charged
             pion production in the energy region of a few
             GeV.},
   Doi = {10.1103/PhysRevLett.95.252301},
   Key = {Hasegawa:2005td}
}

@article{Aliu:2004sq,
   Author = {Aliu, E and Andringa, S and Aoki, S and Argyriades, J and Asakura, K and Ashie, R and Berns, H and Bhang, H and Blondel, A and Borghi, S and Bouchez, J and Burguet-Castell, J and Casper, D and Cavata, C and Cervera, A and Cho, KO and Choi, JH and Dore, U and Espinal, X and Fechner,
             M and Fernandez, E and Fukuda, Y and Gomez-Cadenas, J and Gran, R and Hara,
             T and Hasegawa, M and Hasegawa, T and Hayashi, K and Hayato, Y and Helmer,
             RL and Hill, J and Hiraide, K and Hosaka, J and Ichikawa, AK and Iinuma, M and Ikeda, A and Inagaki, T and Ishida, T and Ishihara, K and Ishii, T and Ishitsuka, M and Itow, Y and Iwashita, T et al.},
   Title = {Evidence for muon neutrino oscillation in an
             accelerator-based experiment.},
   Journal = {Physical Review Letters},
   Volume = {94},
   Number = {8},
   Pages = {081802},
   Year = {2005},
   Month = {March},
   ISSN = {0031-9007},
   url = {http://www.ncbi.nlm.nih.gov/pubmed/15783876},
   Abstract = {We present results for nu(mu) oscillation in the KEK to
             Kamioka (K2K) long-baseline neutrino oscillation experiment.
             K2K uses an accelerator-produced nu(mu) beam with a mean
             energy of 1.3 GeV directed at the Super-Kamiokande detector.
             We observed the energy-dependent disappearance of nu(mu),
             which we presume have oscillated to nu(tau). The probability
             that we would observe these results if there is no neutrino
             oscillation is 0.0050% (4.0 sigma).},
   Doi = {10.1103/PhysRevLett.94.081802},
   Key = {Aliu:2004sq}
}

@article{fds318498,
   Author = {Yoshizawa, T and Sakuda, M and Nakano, I and Iwashita, H and Keppel, C and Walter, C and Gran, R and JLAB, E-C},
   Title = {26pZB-2 Measurement of electron-nucleous quasi-elastic cross
             section and N^*(1232) production cross section using 1GeV
             electron beam.},
   Volume = {60},
   Number = {1},
   Pages = {30 pages},
   Publisher = {The Physical Society of Japan (JPS)},
   Year = {2005},
   Month = {March},
   Key = {fds318498}
}

@article{Guillian:2005wp,
   Author = {Guillian, G. and others},
   Title = {Observation of the anisotropy of 10-TeV primary cosmic ray
             nuclei flux with the Super-Kamiokande-I detector},
   Year = {2005},
   url = {http://arxiv.org/pdf/astro-ph/0508468},
   Abstract = {http://arxiv.org/abs/astro-ph/0508468},
   Key = {Guillian:2005wp}
}

@article{Ashie:2005ik,
   Author = {Ashie, Y. and others},
   Title = {A measurement of atmospheric neutrino oscillation parameters
             by Super-Kamiokande I},
   Journal = {Phys. Rev.},
   Volume = {D71},
   Pages = {112005},
   Year = {2005},
   url = {http://arxiv.org/pdf/hep-ex/0501064},
   Abstract = {http://arxiv.org/abs/hep-ex/0501064},
   Key = {Ashie:2005ik}
}

@article{fds248786,
   Author = {Ashie, Y and Hosaka, J and Ishihara, K and Itow, Y and Kameda, J and Koshio, Y and Minamino, A and Mitsuda, C and Miura, M and Moriyama, S and Nakahata, M and Namba, T and Nambu, R and Obayashi, Y and Shiozawa, M and Suzuki, Y and Takeuchi, Y and Taki, K and Yamada, S and Ishitsuka, M and Kajita, T and Kaneyuki, K and Nakayama, S and Okada, A and Okumura, K and Saji, C and Takenaga, Y and Clark, ST and Desai, S and Kearns, E and Likhoded, S and Stone, JL and Sulak, LR and Wang, W and Goldhaber, M and Casper, D and Cravens, JP and Gajewski, W and Kropp, WR and Liu, DW and Mine, S and Smy, MB and Sobel, HW and Sterner, CW et
             al.},
   Title = {Measurement of atmospheric neutrino oscillation parameters
             by Super-Kamiokande I},
   Journal = {Physical Review D - Particles, Fields, Gravitation and
             Cosmology},
   Volume = {71},
   Number = {11},
   Year = {2005},
   url = {http://dx.doi.org/10.1103/PhysRevD.71.112005},
   Abstract = {We present a combined analysis of fully-contained,
             partially-contained and upward-going muon atmospheric
             neutrino data from a 1489d exposure of the Super-Kamiokande
             detector. The data samples span roughly five decades in
             neutrino energy, from 100MeV to 10eV. A detailed Monte Carlo
             comparison is described and presented. The data is fit to
             the Monte Carlo expectation, and is found to be consistent
             with neutrino oscillations of νμντ with sin22θ&gt;0.92
             and 1.5×10-3&lt;Δm2&lt;3.4×10-3eV2 at 90% confidence
             level. © 2005 The American Physical Society.},
   Doi = {10.1103/PhysRevD.71.112005},
   Key = {fds248786}
}

@article{Kobayashi:2005pe,
   Author = {Kobayashi, K and Earl, M and Ashie, Y and Hosaka, J and Ishihara, K and Itow, Y and Kameda, J and Koshio, Y and Minamino, A and Mitsuda, C and Miura, M and Moriyama, S and Nakahata, M and Namba, T and Nambu, R and Obayashi, Y and Shiozawa, M and Suzuki, Y and Takeuchi, Y and Taki, K and Yamada, S and Ishitsuka, M and Kajita, T and Kaneyuki, K and Nakayama,
             S and Okada, A and Okumura, K and Ooyabu, T and Saji, C and Takenaga, Y and Desai, S and Kearns, E and Likhoded, S and Stone, JL and Sulak, LR and Wang, W and Goldhaber, M and Casper, D and Cravens, JP and Gajewski, W and Kropp, WR and Liu, DW and Mine, S and Smy, MB et al.},
   Title = {Search for nucleon decay via modes favored by supersymmetric
             grand unification models in Super-Kamiokande-I},
   Journal = {Physical Review D - Particles, Fields, Gravitation, and
             Cosmology},
   Volume = {72},
   Number = {5},
   Pages = {052007},
   Year = {2005},
   ISSN = {1550-7998},
   url = {http://arxiv.org/pdf/hep-ex/0502026},
   Abstract = {We report the results for nucleon decay searches via modes
             favored by supersymmetric grand unified models in
             Super-Kamiokande. Using 1489 days of full Super-Kamiokande-I
             data, we searched for p→ν̄K+, n→ν̄K0, p→μ+K0, and
             p→e+K0 modes. We found no evidence for nucleon decay in
             any of these modes. We set lower limits of partial nucleon
             lifetime 2.3×1033, 1.3×1032, 1.3×1033, and 1.0×1033years
             at 90% confidence level for p→ν̄K+, n→ν̄K0,
             p→μ+K0, and p→e+K0 modes, respectively. These results
             give a strong constraint on supersymmetric grand unification
             models. © 2005 The American Physical Society.},
   Doi = {10.1103/PhysRevD.72.052007},
   Key = {Kobayashi:2005pe}
}

@article{Nakayama:2004dp,
   Author = {Nakayama, S and Mauger, C and Ahn, MH and Aoki, S and Ashie, Y and Bhang,
             H and Boyd, S and Casper, D and Choi, JH and Fukuda, S and Fukuda, Y and Gran,
             R and Hara, T and Hasegawa, M and Hasegawa, T and Hayashi, K and Hayato, Y and Hill, J and Ichikawa, AK and Ikeda, A and Inagaki, T and Ishida, T and Ishii, T and Ishitsuka, M and Itow, Y and Iwashita, T and Jang, HI and Jang, JS and Jeon, EJ and Joo, KK and Jung, CK and Kajita, T and Kameda, J and Kaneyuki, K and Kato, I and Kearns, E and Kibayashi, A and Kielczewska,
             D and Kim, BJ and Kim, CO and Kim, JY and Kim, SB and Kobayashi, K and Kobayashi, T and Koshio, Y et al.},
   Title = {Measurement of single π0 production in neutral
             current neutrino interactions with water by a 1.3 GeV wide
             band muon neutrino beam},
   Journal = {Physics Letters, Section B: Nuclear, Elementary Particle and
             High-Energy Physics},
   Volume = {619},
   Number = {3-4},
   Pages = {255-262},
   Year = {2005},
   url = {http://arxiv.org/pdf/hep-ex/0408134},
   Abstract = {Neutral current single π0 production induced by neutrinos
             with a mean energy of 1.3 GeV is measured using a 1000 ton
             water Cherenkov detector in the K2K long baseline neutrino
             experiment. The cross section for this process relative to
             the total charged current cross section is measured to be
             0.064±0.001(stat.)±0.007(sys.). The momentum distribution
             of neutral current π0s from a water target is measured with
             high statistics for the first time. © 2005 Elsevier B.V.
             All rights reserved.},
   Doi = {10.1016/j.physletb.2005.05.044},
   Key = {Nakayama:2004dp}
}

@article{fds326728,
   Author = {Desai, S and Ashie, Y and Fukuda, S and Fukuda, Y and Ishihara, K and Itow,
             Y and Koshio, Y and Minamino, A and Miura, M and Moriyama, S and Nakahata,
             M and Namba, T and Nambu, R and Obayashi, Y and Sakurai, N and Shiozawa, M and Suzuki, Y and Takeuchi, H and Takeuchi, Y and Yamada, S and Ishitsuka,
             M and Kajita, T and Kaneyuki, K and Nakayama, S and Okada, A and Ooyabu, T and Saji, C and Earl, M and Kearns, E and Stone, JL and Sulak, LR and Walter,
             CW and Wang, W and Goldhaber, M and Barszczak, T and Casper, D and Cravens,
             JP and Gajewski, W and Kropp, WR and Mine, S and Liu, DW and Smy, MB and Sobel, HW and Sterner, CW et al.},
   Title = {Publisher's Note: Search for dark matter WIMPs using upward
             through-going muons in Super-Kamiokande [Phys. Rev. D 70 ,
             083523 (2004)]},
   Journal = {Physical Review D - Particles, Fields, Gravitation, and
             Cosmology},
   Volume = {70},
   Number = {10},
   Year = {2004},
   Month = {November},
   url = {http://dx.doi.org/10.1103/PhysRevD.70.109901},
   Doi = {10.1103/PhysRevD.70.109901},
   Key = {fds326728}
}

@article{Ashie:2004mr,
   Author = {Ashie, Y and Hosaka, J and Ishihara, K and Itow, Y and Kameda, J and Koshio, Y and Minamino, A and Mitsuda, C and Miura, M and Moriyama, S and Nakahata, M and Namba, T and Nambu, R and Obayashi, Y and Shiozawa, M and Suzuki, Y and Takeuchi, Y and Taki, K and Yamada, S and Ishitsuka, M and Kajita, T and Kaneyuki, K and Nakayama, S and Okada, A and Okumura, K and Ooyabu, T and Saji, C and Takenaga, Y and Desai, S and Kearns, E and Likhoded, S and Stone, JL and Sulak, LR and Walter, CW and Wang, W and Goldhaber, M and Casper, D and Cravens, JP and Gajewski, W and Kropp,
             WR and Liu, DW and Mine, S and Smy, MB and Sobel, HW et
             al.},
   Title = {Evidence for an oscillatory signature in atmospheric
             neutrino oscillations.},
   Journal = {Physical Review Letters},
   Volume = {93},
   Number = {10},
   Pages = {101801},
   Year = {2004},
   Month = {September},
   ISSN = {0031-9007},
   url = {http://www.ncbi.nlm.nih.gov/pubmed/15447395},
   Abstract = {Muon neutrino disappearance probability as a function of
             neutrino flight length L over neutrino energy E was studied.
             A dip in the L/E distribution was observed in the data, as
             predicted from the sinusoidal flavor transition probability
             of neutrino oscillation. The observed L/E distribution
             constrained nu(micro)<-->nu(tau) neutrino oscillation
             parameters; 1.9x10(-3)<Deltam(2)<3.0x10(-3) eV(2) and
             sin((2)2theta>0.90 at 90% confidence level.},
   Doi = {10.1103/PhysRevLett.93.101801},
   Key = {Ashie:2004mr}
}

@article{Ahn:2004te,
   Author = {Ahn, MH and Aoki, S and Ashie, Y and Bhang, H and Boyd, S and Casper, D and Choi, JH and Fukuda, S and Fukuda, Y and Gran, R and Hara, T and Hasegawa,
             M and Hasegawa, T and Hayashi, K and Hayato, Y and Hill, J and Ichikawa,
             AK and Ikeda, A and Inagaki, T and Ishida, T and Ishii, T and Ishitsuka, M and Itow, Y and Iwashita, T and Jang, HI and Jang, JS and Jeon, EJ and Joo, KK and Jung, CK and Kajita, T and Kameda, J and Kaneyuki, K and Kato, I and Kearns, E and Kibayashi, A and Kielczewska, D and Kim, BJ and Kim, CO and Kim, JY and Kim, SB and Kobayashi, K and Kobayashi, T and Koshio, Y and Kropp, WR and Learned, JG and Lim, SH et al.},
   Title = {Search for electron neutrino appearance in a 250 km
             long-baseline experiment.},
   Journal = {Physical Review Letters},
   Volume = {93},
   Number = {5},
   Pages = {051801},
   Year = {2004},
   Month = {July},
   ISSN = {0031-9007},
   url = {http://www.ncbi.nlm.nih.gov/pubmed/15323684},
   Abstract = {We present a search for electron neutrino appearance from
             accelerator-produced muon neutrinos in the K2K long-baseline
             neutrino experiment. One candidate event is found in the
             data corresponding to an exposure of 4.8 x 10(19) protons on
             target. The expected background in the absence of neutrino
             oscillations is estimated to be 2.4+/-0.6 events and is
             dominated by misidentification of events from neutral
             current pi(0) production. We exclude the nu(micro) to nu(e)
             oscillations at 90% C.L. for the effective mixing angle in
             the 2-flavor approximation of sin((2)2theta(microe)(
             approximately 1/2sin((2)2theta(13))>0.15 at
             Deltam(2)(microe)=2.8 x 10(-3) eV(2), the best-fit value of
             the nu(micro) disappearance analysis in K2K. The most
             stringent limit of sin((2)2theta(microe)<0.09 is obtained at
             Deltam(2)(microe)=6 x 10(-3) eV(2).},
   Doi = {10.1103/PhysRevLett.93.051801},
   Key = {Ahn:2004te}
}

@article{Liu:2004ny,
   Author = {Liu, DW and Ashie, Y and Fukuda, S and Fukuda, Y and Ishihara, K and Itow,
             Y and Koshio, Y and Minamino, A and Miura, M and Moriyama, S and Nakahata,
             M and Namba, T and Nambu, R and Obayashi, Y and Sakurai, N and Shiozawa, M and Suzuki, Y and Takeuchi, H and Takeuchi, Y and Yamada, S and Ishitsuka,
             M and Kajita, T and Kaneyuki, K and Nakayama, S and Okada, A and Ooyabu, T and Saji, C and Desai, S and Earl, M and Kearns, E and Messier, MD and Stone,
             JL and Sulak, LR and Walter, CW and Wang, W and Barszczak, T and Casper, D and Cravens, JP and Gajewski, W and Kropp, WR and Mine, S and Smy, MB and Sobel, HW and Sterner, CW et al.},
   Title = {Limits on the neutrino magnetic moment using 1496 days of
             Super-Kamiokande-I solar neutrino data.},
   Journal = {Physical Review Letters},
   Volume = {93},
   Number = {2},
   Pages = {021802},
   Year = {2004},
   Month = {July},
   ISSN = {0031-9007},
   url = {http://www.ncbi.nlm.nih.gov/pubmed/15323899},
   Abstract = {A search for a nonzero neutrino magnetic moment has been
             conducted using 1496 live days of solar neutrino data from
             Super-Kamiokande-I. Specifically, we searched for
             distortions to the energy spectrum of recoil electrons
             arising from magnetic scattering due to a nonzero neutrino
             magnetic moment. In the absence of a clear signal, we found
             micro(nu)</=(3.6x10(-10))micro(B) at 90% C.L. by fitting to
             the Super-Kamiokande day-night spectra. The fitting took
             into account the effect of neutrino oscillation on the
             shapes of energy spectra. With additional information from
             other solar neutrino and KamLAND experiments constraining
             the oscillation region, a limit of micro(nu)</=(1.1x10(-10))micro(B)
             at 90% C.L. was obtained.},
   Doi = {10.1103/PhysRevLett.93.021802},
   Key = {Liu:2004ny}
}

@article{Smy:2003jf,
   Author = {Smy, MB and Ashie, Y and Fukuda, S and Fukuda, Y and Ishihara, K and Itow,
             Y and Koshio, Y and Minamino, A and Miura, M and Moriyama, S and Nakahata,
             M and Namba, T and Nambu, R and Obayashi, Y and Sakurai, N and Shiozawa, M and Suzuki, Y and Takeuchi, H and Takeuchi, Y and Yamada, S and Ishitsuka,
             M and Kajita, T and Kaneyuki, K and Nakayama, S and Okada, A and Ooyabu, T and Saji, C and Desai, S and Earl, M and Kearns, E and Messier, MD and Stone,
             JL and Sulak, LR and Walter, CW and Wang, W and Goldhaber, M and Barszczak,
             T and Casper, D and Gajewski, W and Kropp, WR and Mine, S and Liu, DW and Sobel, HW and Vagins, MR et al.},
   Title = {Precise measurement of the solar neutrino day-night and
             seasonal variation in Super-Kamiokande-I},
   Journal = {Physical Review D: Particles, Fields, Gravitation and
             Cosmology},
   Volume = {69},
   Number = {1},
   Pages = {011104},
   Year = {2004},
   ISSN = {0556-2821},
   url = {http://arxiv.org/pdf/hep-ex/0309011},
   Abstract = {The time variation of the elastic scattering rate of solar
             neutrinos with electrons in Super-Kamiokande-I was fit to
             the variations expected from active two-neutrino
             oscillations. The best fit in the large mixing angle
             solution has a mixing angle of tan2θ=0.55 and a mass
             squared difference of Δm2 = 6.3×10-5 eV2 between the two
             neutrino mass eigenstates. The fitted day-night asymmetry of
             -1.8±1.6(stat)-12+13(syst)% has improved statistical
             precision over previous measurements and agrees well with
             the expected asymmetry of -2.1%. © 2004 The American
             Physical Society.},
   Doi = {10.1103/PhysRevD.69.011104},
   Key = {Smy:2003jf}
}

@article{Aglietta:2003hq,
   Author = {Aglietta, and M, and others},
   Title = {The primary cosmic ray composition between 10**15-eV and
             10**16-eV from extensive air showers electromagnetic and TeV
             muon data},
   Journal = {Astropart. Phys.},
   Volume = {20},
   Number = {6},
   Pages = {641-652},
   Year = {2004},
   ISSN = {0927-6505},
   url = {http://arxiv.org/pdf/astro-ph/0305325},
   Abstract = {http://arxiv.org/abs/astro-ph/0305325},
   Doi = {10.1016/j.astropartphys.2003.10.004},
   Key = {Aglietta:2003hq}
}

@article{Ambrosio:2004fq,
   Author = {Ambrosio, M and Antolini, R and Baldini, A and Barbarino, GC and Barish,
             BC and Battistoni, G and Bellotti, R and Bemporad, C and Bernardini, P and Bilokon, H and Bloise, C and Bower, C and Brigida, M and Bussino, S and Cafagna, F and Campana, D and Carboni, M and Cecchini, S and Cei, F and Chiarella, V and Choudhary, BC and Coutu, S and Cozzi, M and Cataldo,
             GD and Dekhissi, H and Marzo, CD and Mitri, ID and Derkaoui, J and Vincenzi, MD and Credico, AD and Favuzzi, C and Forti, C and Fusco, P and Giacomelli, G and Giannini, G and Giglietto, N and Giorgini, M and Grassi, M and Grillo, A and Gustavino, C et al.},
   Title = {Search for stellar gravitational collapses with the MACRO
             detector},
   Journal = {The European Physical Journal C - Particles and
             Fields},
   Volume = {37},
   Number = {3},
   Pages = {265-272},
   Year = {2004},
   ISSN = {1434-6044},
   url = {http://dx.doi.org/10.1140/epjc/s2004-01981-3},
   Abstract = {We present the final results of the search for stellar
             gravitational collapses obtained by the MACRO experiment.
             The detector was active for a stellar collapse search for
             more than 11 years and it was sensitive to collapses
             occurring all over in our galaxy for 8.6 years. A real time
             system for a prompt recognition of neutrino bursts was
             developed and was operating on-line for almost the whole
             life of the experiment. No signal compatible with a neutrino
             burst from a galactic supernova was observed. ©
             Springer-Verlag / Società Italiana di Fisica
             2004.},
   Doi = {10.1140/epjc/s2004-01981-3},
   Key = {Ambrosio:2004fq}
}

@article{Desai:2004pq,
   Author = {Desai, S and Ashie, Y and Fukuda, S and Fukuda, Y and Ishihara, K and Itow,
             Y and Koshio, Y and Minamino, A and Miura, M and Moriyama, S and Nakahata,
             M and Namba, T and Nambu, R and Obayashi, Y and Sakurai, N and Shiozawa, M and Suzuki, Y and Takeuchi, H and Takeuchi, Y and Yamada, S and Ishitsuka,
             M and Kajita, T and Kaneyuki, K and Nakayama, S and Okada, A and Ooyabu, T and Saji, C and Earl, M and Kearns, E and Stone, JL and Sulak, LR and Walter,
             CW and Wang, W and Goldhaber, M and Barszczak, T and Casper, D and Cravens,
             JP and Gajewski, W and Kropp, WR and Mine, S and Liu, DW and Smy, MB and Sobel, HW and Sterner, CW et al.},
   Title = {Search for dark matter WIMPs using upward through-going
             muons in Super-Kamiokande},
   Journal = {Physical Review D: Particles, Fields, Gravitation and
             Cosmology},
   Volume = {70},
   Number = {8},
   Pages = {083523-1-083523-11},
   Year = {2004},
   ISSN = {0556-2821},
   url = {http://arxiv.org/pdf/hep-ex/0404025},
   Abstract = {We present the results of indirect searches for Weakly
             Interacting Massive Particles (WIMPs), with 1679.6 live days
             of data from the Super-Kamiokande detector using
             neutrino-induced upward through-going muons. The search is
             performed by looking for an excess of high energy muon
             neutrinos from WIMP annihilations in the Sun, the core of
             the Earth, and the Galactic Center, as compared to the
             number expected from the atmospheric neutrino background. No
             statistically significant excess was seen. We calculate the
             flux limits in various angular cones around each of the
             above celestial objects. We obtain conservative
             model-independent upper limits on the WIMP-nucleon cross
             section as a function of WIMP mass, and compare these
             results with the corresponding results from direct dark
             matter detection experiments.},
   Doi = {10.1103/PhysRevD.70.083523},
   Key = {Desai:2004pq}
}

@article{Aglietta:2004ws,
   Author = {Aglietta, M and Alessandro, B and Antonioli, P and Arneodo, F and Bergamasco, L and Bertaina, M and Castagnoli, C and Castellina, A and Chiavassa, A and Cini, G and Piazzoli, BD and Sciascio, GD and Fulgione,
             W and Galeotti, P and Ghia, PL and Iacovacci, M and Mannocchi, G and Morello, C and Navarra, G and Saavedra, O and Stamerra, A and Trinchero,
             GC and Valchierotti, S and Vallania, P and Vernetto, S and Vigorito, C and Ambrosio, M and Antolini, R and Baldini, A and Barbarino, GC and Barish,
             BC and Battistoni, G and Becherini, Y and Bellotti, R and Bemporad, C and Bernardini, P and Bilokon, H et al.},
   Title = {The cosmic ray proton, helium and CNO fluxes in the 100 TeV
             energy region from TeV muons and EAS atmospheric Cherenkov
             light observations of MACRO and EAS-TOP},
   Journal = {Astroparticle Physics},
   Volume = {21},
   Number = {3},
   Pages = {223-240},
   Year = {2004},
   ISSN = {0927-6505},
   url = {http://dx.doi.org/10.1016/j.astropartphys.2004.01.005},
   Abstract = {The primary cosmic ray (CR) proton, helium and CNO fluxes in
             the energy range 80-300 TeV are studied at the National Gran
             Sasso Laboratories by means of EAS-TOP (Campo Imperatore,
             2005 m a.s.l.) and MACRO (deep underground, 3100 m w.e., the
             surface energy threshold for a muon reaching the detector
             being Eμth≈1.3 TeV). The measurement is based on: (a) the
             selection of primaries based on their energy/nucleon (i.e.,
             with energy/nucleon sufficient to produce a muon with energy
             larger than 1.3 TeV) and the reconstruction of the shower
             geometry by means of the muons recorded by MACRO in the deep
             underground laboratories; (b) the detection of the
             associated atmospheric Cherenkov light (C.l.) signals by
             means of the C.l. detector of EAS-TOP. The C.l. density at
             core distance r&gt;100 m is directly related to the total
             primary energy E0. Proton and helium ("p + He") and proton,
             helium and CNO ("p + He + CNO") primaries are thus selected
             at E0≃80 TeV, and at E0≃250 TeV, respectively. Their
             flux is measured: Jp+He(80 Tev= (1.8±0.4)×10-6 m-2 s-1
             sr-1 TeV-1, and Jp+He+CNO(250 TeV)=(1.1±0.3)×10-7 m-2 s-1
             sr-1 TeV-1, their relative weights being: Jp+He/Jp+He+CNO
             (250 TeV)=0.78±0.17. By using the measurements of the
             proton spectrum obtained from the direct experiments and
             hadron flux data in the atmosphere, we obtain for the
             relative weights of the three components at 250 TeV:
             Jp:JHe:JCNO =(0.20±0.08): (0.58±0.19):(0.22±0.17). This
             corresponds to the dominance of helium over proton primaries
             at 100-1000 TeV, and a possible non-negligible contribution
             from CNO.The lateral distribution of Cherenkov light in
             Extensive Air Showers (EASs), which is related to the rate
             of energy deposit of the primary in the atmosphere, is
             measured for a selected proton and helium primary beam, and
             good agreement is found when compared with the one
             calculated with the CORSIKA/QGSJET simulation model. © 2004
             Elsevier B.V. All rights reserved.},
   Doi = {10.1016/j.astropartphys.2004.01.005},
   Key = {Aglietta:2004ws}
}

@article{Ambrosio:2004ig,
   Author = {Ambrosio, M and Antolini, R and Bakari, D and Baldini, A and Barbarino,
             GC and Barish, BC and Battistoni, G and Becherini, Y and Bellotti, R and Bemporad, C and Bernardini, P and Bilokon, H and Bloise, C and Bower, C and Brigida, M and Cafagna, F and Campana, D and Carboni, M and Cecchini, S and Cei, F and Chiarella, V and Choudhary, BC and Cosson, D and Coutu, S and Cataldo, GD and Dekhissi, H and Marzo, CD and Mitri, ID and Denni, U and Derkauoi, J and Vincenzi, MD and Credico, AD and Favuzzi, C and Forti,
             C and Frani, A and Fusco, P and Giacomelli, G and Giannini, G and Giglietto, N and Giorgini, M et al.},
   Title = {Measurements of atmospheric muon neutrino oscillations,
             global analysis of the data collected with MACRO
             detector},
   Journal = {The European Physical Journal C - Particles and
             Fields},
   Volume = {36},
   Number = {3},
   Pages = {323-339},
   Year = {2004},
   ISSN = {1434-6044},
   url = {http://dx.doi.org/10.1140/epjc/s2004-01951-9},
   Abstract = {The final analysis of atmospheric neutrino events collected
             with the MACRO detector is presented. Three different
             classes of events, generated by neutrinos in different
             energy ranges, are studied looking at rates, angular
             distributions and estimated energies. The results are
             consistent for all the subsamples and indicate a flux
             deficit that depends on energy and path-length of neutrinos.
             The no-oscillation hypothesis is excluded at ∼ 5σ, while
             the hypothesis of vμ → vτ oscillation gives a
             satisfactory description of all data. The parameters with
             highest probability in a two flavor scenario are sin2 2θm =
             1 and Δm2 = 0.0023 eV2. This result is independent of the
             absolute normalization of the atmospheric neutrino fluxes.
             The data can also be used to put experimental constrain on
             this normalization. © Springer-Verlag / Società Italiana
             di Fisica 2004.},
   Doi = {10.1140/epjc/s2004-01951-9},
   Key = {Ambrosio:2004ig}
}

@article{fds304629,
   Author = {Aglietta, M and Alessandro, B and Antonioli, P and Arneodo, F and Bergamasco, L and Bertaina, M and Castagnoli, C and Castellina, A and Chiavassa, A and Cini, G and Piazzoli, BD and Sciascio, GD and Fulgione,
             W and Galeotti, P and Ghia, PL and Iacovacci, M and Mannocchi, G and Morello, C and Navarra, G and Saavedra, O and Stamerra, A and Trinchero,
             GC and Valchierotti, S and Vallania, P and Vernetto, S and Vigorito, C and Ambrosio, M and Antolini, R and Baldini, A and Barbarino, GC and Barish,
             BC and Battistoni, G and Becherini, Y and Bellotti, R and Bemporad, C and Bernardini, P and Bilokon, H et al.},
   Title = {The cosmic ray primary composition between 1015
             and 1016 eV from Extensive Air Showers
             electromagnetic and TeV muon data},
   Journal = {Astroparticle Physics},
   Volume = {20},
   Number = {6},
   Pages = {641-652},
   Year = {2004},
   ISSN = {0927-6505},
   url = {http://dx.doi.org/10.1016/j.astropartphys.2003.10.004},
   Abstract = {The cosmic ray primary composition in the energy range
             between 1015 and 1016 eV, i.e., around the "knee" of the
             primary spectrum, has been studied through the combined
             measurements of the EAS-TOP air shower array (2005 m a.s.l.,
             105 m2 collecting area) and the MACRO underground detector
             (963 m a.s.l., 3100 m w.e. of minimum rock overburden, 920
             m2 effective area) at the National Gran Sasso Laboratories.
             The used observables are the air shower size (Ne) measured
             by EAS-TOP and the muon number (Nμ) recorded by MACRO. The
             two detectors are separated on average by 1200 m of rock,
             and located at a respective zenith angle of about 30°. The
             energy threshold at the surface for muons reaching the MACRO
             depth is approximately 1.3 TeV. Such muons are produced in
             the early stages of the shower development and in a
             kinematic region quite different from the one relevant for
             the usual Nμ-Ne studies. The measurement leads to a primary
             composition becoming heavier at the knee of the primary
             spectrum, the knee itself resulting from the steepening of
             the spectrum of a primary light component (p, He) of Δγ=
             0.7±0.4 at E0∼4×1015 eV. The result confirms the ones
             reported from the observation of the low energy muons at the
             surface (typically in the GeV energy range), showing that
             the conclusions do not depend on the production region
             kinematics. Thus, the hadronic interaction model used
             (CORSIKA/QGSJET) provides consistent composition results
             from data related to secondaries produced in a rapidity
             region exceeding the central one. Such an evolution of the
             composition in the knee region supports the "standard"
             galactic acceleration/propagation models that imply rigidity
             dependent breaks of the different components, and therefore
             breaks occurring at lower energies in the spectra of the
             light nuclei. © 2003 Elsevier B.V. All rights
             reserved.},
   Doi = {10.1016/j.astropartphys.2003.10.004},
   Key = {fds304629}
}

@article{Walter:2004de,
   Author = {Walter, CW and McConnel, K and Sakuda, M},
   Title = {Low energy neutrino-nucleus interactions},
   Journal = {AIP Conference Proceedings},
   Volume = {721},
   Pages = {247-251},
   Year = {2004},
   ISBN = {0-7354-0201-9},
   Key = {Walter:2004de}
}

@article{Gando:2002ub,
   Author = {Gando, Y and Fukuda, S and Fukuda, Y and Ishitsuka, M and Itow, Y and Kajita, T and Kameda, J and Kaneyuki, K and Kobayashi, K and Koshio, Y and Miura, M and Moriyama, S and Nakahata, M and Nakayama, S and Namba, T and Obayashi, Y and Okada, A and Ooyabu, T and Saji, C and Sakurai, N and Shiozawa, M and Suzuki, Y and Takeuchi, H and Takeuchi, Y and Totsuka,
             Y and Yamada, S and Desai, S and Earl, M and Kearns, E and Messier, MD and Stone, JL and Sulak, LR and Walter, CW and Goldhaber, M and Barszczak,
             T and Casper, D and Gajewski, W and Kropp, WR and Mine, S and Liu, DW and Smy,
             MB and Sobel, HW and Vagins, MR and Gago, A et al.},
   Title = {Search for nu(e) from the sun at Super-Kamiokande-I.},
   Journal = {Physical Review Letters},
   Volume = {90},
   Number = {17},
   Pages = {171302},
   Year = {2003},
   Month = {May},
   ISSN = {0031-9007},
   url = {http://www.ncbi.nlm.nih.gov/pubmed/12786067},
   Abstract = {We present the results of a search for low energy nu(e) from
             the Sun using 1496 days of data from Super-Kamiokande-I. We
             observe no significant excess of events and set an upper
             limit for the conversion probability to nu(e) of the 8B
             solar neutrino. This conversion limit is 0.8% (90% C.L.) of
             the standard solar model's neutrino flux for total
             energy=8-20 MeV. We also set a flux limit for monochromatic
             nu(e) for E(nu(e))=10-17 MeV.},
   Doi = {10.1103/PhysRevLett.90.171302},
   Key = {Gando:2002ub}
}

@article{Malek:2002ns,
   Author = {Malek, M and Morii, M and Fukuda, S and Fukuda, Y and Ishitsuka, M and Itow, Y and Kajita, T and Kameda, J and Kaneyuki, K and Kobayashi, K and Koshio, Y and Miura, M and Moriyama, S and Nakahata, M and Nakayama, S and Namba, T and Okada, A and Ooyabu, T and Saji, C and Sakurai, N and Shiozawa, M and Suzuki, Y and Takeuchi, H and Takeuchi, Y and Totsuka,
             Y and Yamada, S and Desai, S and Earl, M and Kearns, E and Messier, MD and Stone, JL and Sulak, LR and Walter, CW and Goldhaber, M and Barszczak,
             T and Casper, D and Gajewski, W and Kropp, WR and Mine, S and Liu, DW and Smy,
             MB and Sobel, HW and Vagins, MR and Gago, A et al.},
   Title = {Search for supernova relic neutrinos at Super-Kamiokande.},
   Journal = {Physical Review Letters},
   Volume = {90},
   Number = {6},
   Pages = {061101},
   Year = {2003},
   Month = {February},
   ISSN = {0031-9007},
   url = {http://www.ncbi.nlm.nih.gov/pubmed/12633283},
   Abstract = {A search for the relic neutrinos from all past core-collapse
             supernovae was conducted using 1496 days of data from the
             Super-Kamiokande detector. This analysis looked for
             electron-type antineutrinos that had produced a positron
             with an energy greater than 18 MeV. In the absence of a
             signal, 90% C.L. upper limits on the total flux were set for
             several theoretical models; these limits ranged from 20 to
             130 macro nu(e) cm(-2) s(-1). Additionally, an upper bound
             of 1.2 macro nu(e) cm(-2) s(-1) was set for the supernova
             relic neutrino flux in the energy region E(nu)>19.3
             MeV.},
   Doi = {10.1103/PhysRevLett.90.061101},
   Key = {Malek:2002ns}
}

@article{fds248716,
   Author = {Walter, CW},
   Title = {Recent results from the K2K experiment},
   Journal = {Nuclear Physics, Section B: Proceedings Supplements},
   Volume = {123},
   Pages = {260-266},
   Booktitle = {Fundamental Interactions, Proceedings of the 17th Lake
             Louise Winter Institute},
   Publisher = {World Scientific Publishing Co. Pte. Ltd.},
   Year = {2003},
   ISSN = {0920-5632},
   url = {http://dx.doi.org/10.1016/S0920-5632(03)02186-8},
   Abstract = {The K2K experiment has collected approximately half of its
             allocated protons on target between June of 1999 and July of
             2001. These proceedings give a short introduction to the
             experiment and summarize some of the recent
             results.},
   Doi = {10.1016/S0920-5632(03)02186-8},
   Key = {fds248716}
}

@article{fds248736,
   Author = {Togo, V and Ambrosio, M and Antolini, R and Auriemma, G and Bakari, D and Baldini, A and Barbarino, GC and Barish, BC and Battistoni, G and Becherini, Y and Bellotti, R and Bemporad, C and Bernardini, P and Bilokon, H and Bloise, C and Bower, C and Brigida, M and Bussino, S and Cafagna, F and Calicchio, M and Campana, D and Carboni, M and Caruso, R and Cecchini, S and Cei, F and Chiarella, V and Chiarusi, T and Choudhary,
             BC and Coutu, S and Cozzi, M and Cataldo, GD and Dekhissi, H and Marzo, CD and Mitri, ID and Derkaoui, J and Vincenzi, MD and Credico, AD and Erriquez,
             O and Favuzzi, C and Forti, C et al.},
   Title = {Calibrations of CR39 and Makrofol nuclear track detectors
             and search for exotic particles},
   Journal = {Nuclear Physics, Section B: Proceedings Supplements},
   Volume = {125},
   Pages = {217-221},
   Year = {2003},
   ISSN = {0920-5632},
   url = {http://dx.doi.org/10.1016/S0920-5632(03)90994-7},
   Abstract = {We present the final results of the search for exotic
             massive particles in the cosmic radiation performed with the
             MACRO underground experiment. Magnetic monopoles and
             nuclearites flux upper limits obtained with the CR39 nuclear
             track subdetector, the scintillation and streamer tube
             subdetectors are given. Searches at high altitude with the
             SLIM experiment are in progress.},
   Doi = {10.1016/S0920-5632(03)90994-7},
   Key = {fds248736}
}

@article{Walter:2003zj,
   Author = {Walter, CW},
   Title = {Distinguishing νμ→ντ
             oscillations and exotic oscillation/decay hypotheses using
             Super-K atmospheric neutrino data},
   Journal = {Nuclear Instruments and Methods in Physics Research Section
             A: Accelerators, Spectrometers, Detectors and Associated
             Equipment},
   Volume = {503},
   Number = {1-2},
   Pages = {110-113},
   Year = {2003},
   ISSN = {0168-9002},
   url = {http://dx.doi.org/10.1016/S0168-9002(03)00649-1},
   Abstract = {In this talk, I will review the Super-K analysis to
             distinguish between the νμ→ντ oscillation hypothesis
             and other exotic oscillation/decay scenarios. All of the
             tested exotic hypotheses are excluded by the Super-K
             atmospheric neutrino data at the greater than 4σ level. A
             limit is placed on the admixture of νsterile states in a
             ντ, νsterile mixture to be less than 25% at 90% CL. In
             addition, a 2.2σ tau lepton appearance signal is reported
             which is consistent with our expectation of νμ→ντ
             oscillations. © 2003 Elsevier Science B.V. All rights
             reserved.},
   Doi = {10.1016/S0168-9002(03)00649-1},
   Key = {Walter:2003zj}
}

@article{Ambrosio:2002db,
   Author = {Ambrosio, M and Antolini, R and Baldini, A and Barbarino, GC and Barish,
             BC and Battistoni, G and Becherini, Y and Bellotti, R and Bemporad, C and Bernardini, P and Bilokon, H and Bower, C and Brigida, M and Bussino, S and Cafagna, F and Calicchio, M and Campana, D and Carboni, M and Caruso, R and Cecchini, S and Cei, F and Chiarella, V and Chiarusi, T and Choudhary,
             BC and Coutu, S and Cozzi, M and Cataldo, GD and Dekhissi, H and Marzo, CD and Mitri, ID and Derkaoui, J and Vincenzi, MD and Credico, AD and Erriquez,
             O and Favuzzi, C and Forti, C and Fusco, P and Giacomelli, G and Giannini,
             G and Giglietto, N et al.},
   Title = {Search for the sidereal and solar diurnal modulations in the
             total MACRO muon data set},
   Journal = {Physical Review D: Particles, Fields, Gravitation and
             Cosmology},
   Volume = {67},
   Number = {4},
   Pages = {042002},
   Year = {2003},
   ISSN = {0556-2821},
   url = {http://arxiv.org/pdf/astro-ph/0211119},
   Abstract = {We have analyzed 44.3M single muons collected by MACRO from
             1991 through 2000 in 2145 live days of operation. We have
             searched for the solar diurnal, apparent sidereal, and
             pseudosidereal modulation of the underground muon rate by
             computing hourly deviations of the muon rate from 6 month
             averages. We find evidence for statistically significant
             modulations with the solar diurnal and the sidereal periods.
             The amplitudes of these modulations are &lt;0.1%, and are at
             the limit of the detector statistics. The pseudosidereal
             modulation is not statistically significant. The solar
             diurnal modulation is due to the daily atmospheric
             temperature variations at 20 km, the altitude of primary
             cosmic ray interactions with the atmosphere; MACRO is the
             deepest experiment to report this result. The sidereal
             modulation is in addition to the expected Compton-Getting
             modulation due to solar system motion relative to the local
             standard of rest; it represents motion of the solar system
             with respect to the galactic cosmic rays toward the galactic
             plane. © 2003 The American Physical Society.},
   Doi = {10.1103/PhysRevD.67.042002},
   Key = {Ambrosio:2002db}
}

@article{Ambrosio:2003mz,
   Author = {Ambrosio, M and Antolini, R and Baldini, A and Barbarino, GC and Barish,
             BC and Battistoni, G and Becherini, Y and Bellotti, R and Bemporad, C and Bernardini, P and Bilokon, H and Bower, C and Brigida, M and Bussino, S and Cafagna, F and Calicchio, M and Campana, D and Carboni, M and Caruso, R and Cecchini, S and Cei, F and Chiarella, V and Chiarusi, T and Choudhary,
             BC and Coutu, S and Cozzi, M and Cataldo, GD and Dekhissi, H and Marzo, CD and Mitri, ID and Derkaoui, J and Vincenzi, MD and Credico, AD and Erriquez,
             O and Favuzzi, C and Forti, C and Fusco, P and Giacomelli, G and Giannini,
             G and Giglietto, N et al.},
   Title = {Moon and Sun shadowing effect in the MACRO
             detector},
   Journal = {Astroparticle Physics},
   Volume = {20},
   Number = {2},
   Pages = {145-156},
   Year = {2003},
   ISSN = {0927-6505},
   url = {http://arxiv.org/pdf/astro-ph/0302586},
   Abstract = {Using data collected by the MACRO experiment from 1989 to
             the end of its operations in 2000, we have studied in the
             underground muon flux the shadowing effects due to both the
             Moon and the Sun. We have observed the shadow cast by the
             Moon at its apparent position with a significance of 6.5σ.
             The Moon shadowing effect has been used to verify the
             pointing capability of the detector and to determine the
             instrument resolution for the search of muon excesses from
             any direction of the celestial sphere. The dependence of the
             effect on the geomagnetic field is clearly shown by
             splitting the data sample in day and night observations. The
             Sun shadow, observed with a significance of 4.6σ is
             displaced by about 0.6° from its apparent position. In this
             case however the explanation resides in the configuration of
             the Solar and Interplanetary Magnetic Fields, which affect
             the propagation of cosmic ray particles between the Sun, and
             the Earth. The displacement of the Sun shadow with respect
             to the real Sun position has been used to establish an upper
             limit on the antimatter flux in cosmic rays of about 48% at
             68% c.l. and primary energies of about 20 TeV. © 2003
             Elsevier B.V. All rights reserved.},
   Doi = {10.1016/S0927-6505(03)00169-5},
   Key = {Ambrosio:2003mz}
}

@article{Kim:2002pa,
   Author = {Kim, BJ and Iwashita, T and Ishida, T and Jeon, EJ and Yokoyama, H and Aoki, S and Berns, HG and Bhang, HC and Boyd, S and Fujii, K and Hara, T and Hayato, Y and Hill, J and Ishii, T and Ishino, H and Jung, CK and Kearns,
             E and Kim, HI and Kim, JH and Kim, JY and Kim, SB and Kobayashi, T and Kume,
             G and Matsuno, S and Mine, S and Nakamura, K and Nakamura, M and Nishikawa,
             K and Onchi, M and Otaki, T and Oyama, Y and Park, H and Sakuda, M and Sato,
             K and Scholberg, K and Sharkey, E and Stone, JL and Suzuki, A and Takenaka,
             K and Tamura, N and Tanaka, Y and Takatsuki, M and Walter, CW and Wilkes,
             J and Yoo, J and Yoshida, M},
   Title = {Tracking performance of the scintillating fiber detector in
             the K2K experiment},
   Journal = {Nuclear Instruments and Methods in Physics Research Section
             A: Accelerators, Spectrometers, Detectors and Associated
             Equipment},
   Volume = {497},
   Number = {2-3},
   Pages = {450-466},
   Year = {2003},
   ISSN = {0168-9002},
   url = {http://arxiv.org/pdf/hep-ex/0206041},
   Abstract = {Tracking performance of the scintillating fiber detector
             (SciFi) in the K2K experiment was studied. SciFi was used to
             reconstruct charged particles produced in neutrino
             interactions in the near detector. The track reconstruction
             algorithm and the performance of SciFi was also described
             after three years of operation.},
   Doi = {10.1016/S0168-9002(02)01980-0},
   Key = {Kim:2002pa}
}

@article{Ambrosio:2002ma,
   Author = {Ambrosio, M and Antolini, R and Auriemma, G and Bakari, D and Baldini,
             A and Barbarino, GC and Barish, BC and Battistoni, G and Becherini, Y and Bellotti, R and Bemporad, C and Bernardini, P and Bilokon, H and Bloise,
             C and Bower, C and Brigida, M and Bussino, S and Cafagna, F and Calicchio,
             M and Campana, D and Carboni, M and Caruso, R and Cecchini, S and Cei, F and Chiarella, V and Choudhary, BC and Coutu, S and Cozzi, M and Cataldo,
             GD and Dekhissi, H and Marzo, CD and Mitri, ID and Derkaoui, J and Vincenzi, MD and Credico, AD and Erriquez, O and Favuzzi, C and Forti,
             C and Fusco, P and Giacomelli, G et al.},
   Title = {Search for diffuse neutrino flux from astrophysical sources
             with MACRO},
   Journal = {Astroparticle Physics},
   Volume = {19},
   Number = {1},
   Pages = {1-13},
   Year = {2003},
   ISSN = {0927-6505},
   url = {http://arxiv.org/pdf/astro-ph/0203181},
   Abstract = {Many galactic and extragalactic astrophysical sources are
             currently considered promising candidates as high-energy
             neutrino emitters. Astrophysical neutrinos can be detected
             as upward-going muons produced in charged-current
             interactions with the medium surrounding the detector. The
             expected neutrino fluxes from various models start to
             dominate on the atmospheric neutrino background at neutrino
             energies above some tens of TeV. We present the results of a
             search for an excess of high-energy upward-going muons among
             the sample of data collected by MACRO during ∼5.8 years of
             effective running time. No significant evidence for this
             signal was found. As a consequence, an upper limit on the
             flux of upward-going muons from high-energy neutrinos was
             set at the level of 1.7 × 10-14 cm-2 s-1 sr-1. The
             corresponding upper limit for the diffuse neutrino flux was
             evaluated assuming a neutrino power law spectrum. Our result
             was compared with theoretical predictions and upper limits
             from other experiments. © 2002 Elsevier Science B.V. All
             rights reserved.},
   Doi = {10.1016/S0927-6505(02)00190-1},
   Key = {Ambrosio:2002ma}
}

@article{Ambrosio:2002wr,
   Author = {Ambrosio, M and Antolini, R and Auriemma, G and Bakari, D and Baldini,
             A and Barbarino, GC and Barish, BC and Battistoni, G and Becherini, Y and Bellotti, R and Bemporad, C and Bernardini, P and Bilokon, H and Bloise,
             C and Bower, C and Brigida, M and Bussino, S and Cafagna, F and Calicchio,
             M and Campana, D and Carboni, M and Caruso, R and Cecchini, S and Cei, F and Chiarella, V and Choudhary, BC and Coutu, S and Cozzi, M and Cataldo,
             GD and Dekhissi, H and Marzo, CD and Mitri, ID and Derkaoui, J and Vincenzi, MD and Credico, AD and Erriquez, O and Favuzzi, C and Forti,
             C and Fusco, P and Giacomelli, G et al.},
   Title = {Search for cosmic ray sources using muons detected by the
             MACRO experiment},
   Journal = {Astroparticle Physics},
   Volume = {18},
   Number = {6},
   Pages = {615-627},
   Year = {2003},
   ISSN = {0927-6505},
   url = {http://arxiv.org/pdf/hep-ph/0204188},
   Abstract = {The MACRO underground detector at Gran Sasso Laboratory
             recorded 60 million secondary cosmic ray muons from February
             1989 until December 2000. Different techniques were used to
             analyze this sample in search for density excesses from
             astrophysical point-like sources. No evidence for DC
             excesses for any source in an all-sky survey is reported. In
             addition, searches for muon excess correlated with the known
             binary periods of Cygnus X-3 and Hercules X-1, and searches
             for statistically significant bursting episodes from known
             γ-ray sources are also proved negative. © 2002 Elsevier
             Science B.V. All rights reserved.},
   Doi = {10.1016/S0927-6505(02)00164-0},
   Key = {Ambrosio:2002wr}
}

@article{Ambrosio:2002id,
   Author = {Ambrosio, M and Antolini, R and Baldini, A and Barbarino, GC and Barish,
             BC and Battistoni, G and Becherini, Y and Bellotti, R and Bemporad, C and Bernardini, P and Bilokon, H and Bower, C and Brigida, M and Bussino, S and Cafagna, F and Calicchio, M and Campana, D and Carboni, M and Caruso, R and Cecchini, S and Cei, F and Chiarella, V and Choudhary, BC and Coutu, S and Cozzi, M and Cataldo, GD and Dekhissi, H and Marzo, CD and Mitri, ID and Derkaoui, J and Vincenzi, MD and Credico, AD and Erriquez, O and Favuzzi, C and Forti, C and Fusco, P and Giacomelli, G and Giannini, G and Giglietto, N and Giorgini, M et al.},
   Title = {Measurement of the residual energy of muons in the Gran
             Sasso underground laboratories},
   Journal = {Astroparticle Physics},
   Volume = {19},
   Number = {3},
   Pages = {313-328},
   Year = {2003},
   ISSN = {0927-6505},
   url = {http://arxiv.org/pdf/hep-ex/0207043},
   Abstract = {The MACRO detector was located in the Hall B of the Gran
             Sasso underground laboratories under an average rock
             overburden of 3700 hg/cm2. A transition radiation detector
             composed of three identical modules, covering a total
             horizontal area of 36 m2, was installed inside the empty
             upper part of the detector in order to measure the residual
             energy of muons. This paper presents the measurement of the
             residual energy of single and double muons crossing the
             apparatus. Our data show that double muons are more
             energetic than single ones. This measurement is performed
             over a standard rock depth range from 3000 to 6500 hg/cm2.
             © 2002 Elsevier Science B.V. All rights
             reserved.},
   Doi = {10.1016/S0927-6505(02)00217-7},
   Key = {Ambrosio:2002id}
}

@article{Ambrosio:2003yz,
   Author = {Ambrosio, M and Antolini, R and Bakari, D and Baldini, A and Barbarino,
             GC and Barish, BC and Battistoni, G and Becherini, Y and Bellotti, R and Bemporad, C and Bernardini, P and Bilokon, H and Bloise, C and Bower, C and Brigida, M and Bussino, S and Cafagna, F and Calicchio, M and Campana,
             D and Carboni, M and Caruso, R and Cecchini, S and Cei, F and Chiarella, V and Chiarusi, T and Choudhary, BC and Coutu, S and Cozzi, M and Cataldo, GD and Dekhissi, H and Marzo, CD and Mitri, ID and Derkaoui, J and Vincenzi,
             MD and Credico, AD and Favuzzi, C and Forti, C and Fusco, P and Giacomelli,
             G and Giannini, G et al.},
   Title = {Atmospheric neutrino oscillations from upward throughgoing
             muon multiple scattering in MACRO},
   Journal = {Physics Letters B},
   Volume = {566},
   Number = {1-2},
   Pages = {35-44},
   Year = {2003},
   ISSN = {0370-2693},
   url = {http://arxiv.org/pdf/hep-ex/0304037},
   Abstract = {The energy of atmospheric neutrinos detected by MACRO was
             estimated using multiple Coulomb scattering of upward
             throughgoing muons. This analysis allows a test of
             atmospheric neutrino oscillations, relying on the distortion
             of the muon energy distribution. These results have been
             combined with those coming from the upward throughgoing muon
             angular distribution only. Both analyses are independent of
             the neutrino flux normalization and provide strong evidence,
             above the 4σ level, in favour of neutrino oscillations. ©
             2003 Published by Elsevier B.V.},
   Doi = {10.1016/S0370-2693(03)00806-2},
   Key = {Ambrosio:2003yz}
}

@article{Fukuda:2002uc,
   Author = {Fukuda, S and Fukuda, Y and Hayakawa, T and Ichihara, E and Ishitsuka,
             M and Itow, Y and Kajita, T and Kameda, J and Kaneyuki, K and Kasuga, S and Kobayashi, K and Kobayashi, Y and Koshio, Y and Miura, M and Moriyama,
             S and Nakahata, M and Nakayama, S and Namba, T and Obayashi, Y and Okada,
             A and Oketa, M and Okumura, K and Oyabu, T and Sakurai, N and Shiozawa, M and Suzuki, Y and Takeuchi, Y and Toshito, T and Totsuka, Y and Yamada, S and Desai, S and Earl, M and Hong, JT and Kearns, E and Masuzawa, M and Messier, MD and Stone, JL and Sulak, LR and Walter, CW and Wang, W and Scholberg, K and Barszczak, T et al.},
   Title = {The Super-Kamiokande detector},
   Journal = {Nuclear Instruments and Methods in Physics Research Section
             A: Accelerators, Spectrometers, Detectors and Associated
             Equipment},
   Volume = {501},
   Number = {2-3},
   Pages = {418-462},
   Year = {2003},
   ISSN = {0168-9002},
   url = {http://dx.doi.org/10.1016/S0168-9002(03)00425-X},
   Abstract = {Super-Kamiokande is the world's largest water Cherenkov
             detector, with net mass 50,000 tons. During the period
             April, 1996 to July, 2001, Super-Kamiokande I collected 1678
             live-days of data, observing neutrinos from the Sun, Earth's
             atmosphere, and the K2K long-baseline neutrino beam with
             high efficiency. These data provided crucial information for
             our current understanding of neutrino oscillations, as well
             as setting stringent limits on nucleon decay. In this paper,
             we describe the detector in detail, including its site,
             configuration, data acquisition equipment, online and
             offline software, and calibration systems which were used
             during Super-Kamiokande I. © 2003 Elsevier Science B.V. All
             rights reserved.},
   Doi = {10.1016/S0168-9002(03)00425-X},
   Key = {Fukuda:2002uc}
}

@article{Ahn:2002up,
   Author = {Ahn, MH and Aoki, S and Bhang, H and Boyd, S and Casper, D and Choi, JH and Fukuda, S and Fukuda, Y and Gajewski, W and Hara, T and Hasegawa, M and Hasegawa, T and Hayato, Y and Hill, J and Ichikawa, AK and Ikeda, A and Inagaki, T and Ishida, T and Ishii, T and Ishitsuka, M and Itow, Y and Iwashita, T and Jang, HI and Jang, JS and Jeon, EJ and Jung, CK and Kajita,
             T and Kameda, J and Kaneyuki, K and Kato, I and Kearns, E and Kibayashi, A and Kielczewska, D and Kobayashi, K and Kim, BJ and Kim, CO and Kim, JY and Kim, SB and Kobayashi, T and Kohama, M and Koshio, Y and Kropp, WR and Learned, JG and Lim, SH and Lim, IT et al.},
   Title = {Indications of neutrino oscillation in a 250 km
             long-baseline experiment},
   Journal = {Physical Review Letters},
   Volume = {90},
   Number = {4},
   Pages = {418011-418015},
   Year = {2003},
   ISSN = {0031-9007},
   url = {http://www.ncbi.nlm.nih.gov/pubmed/12570410},
   Abstract = {A study was performed on Kamioka long-baseline neutrino
             oscillation experiment (K2K). The indications of neutrino
             oscillation such as a reduction of flux together with a
             distortion of the energy spectrum were observed in the
             experiment. In Super Kamiokande (SK), 250 km from the
             neutrino production point, fifty-six beam neutrino events
             were observed. It was found that the probability that the
             measurements at SK is explained by statistical fluctuation
             without neutrino oscillation is less than
             1%.},
   Doi = {10.1103/PhysRevLett.90.041801},
   Key = {Ahn:2002up}
}

@article{Yoo:2003rc,
   Author = {Yoo, J and Ashie, Y and Fukuda, S and Fukuda, Y and Ishihara, K and Itow,
             Y and Koshio, Y and Minamino, A and Miura, M and Moriyama, S and Nakahata,
             M and Namba, T and Nambu, R and Obayashi, Y and Sakurai, N and Shiozawa, M and Suzuki, Y and Takeuchi, H and Takeuchi, Y and Yamada, S and Ishitsuka,
             M and Kajita, T and Kaneyuki, K and Nakayama, S and Okada, A and Ooyabu, T and Saji, C and Desai, S and Earl, M and Kearns, E and Messier, MD and Stone,
             JL and Sulak, LR and Walter, CW and Goldhaber, M and Barszczak, T and Casper, D and Gajewski, W and Kropp, WR and Mine, S and Liu, DW and Smy,
             MB and Sobel, HW and Vagins, MR et al.},
   Title = {Search for periodic modulations of the solar neutrino flux
             in Super-Kamiokande-I},
   Journal = {Physical Review D: Particles, Fields, Gravitation and
             Cosmology},
   Volume = {68},
   Number = {9},
   Pages = {092002},
   Year = {2003},
   ISSN = {0556-2821},
   url = {http://arxiv.org/pdf/hep-ex/0307070},
   Abstract = {A search for periodic modulations of the solar neutrino flux
             was performed using the Super-Kamiokande-I data taken from
             31 May 1996 to 15 July 2001. The detector's capability of
             measuring the exact time of events, combined with a
             relatively high yield of solar neutrino events, allows a
             search for short-time variations in the observed flux. We
             employed the Lomb test to look for periodic modulations of
             the observed solar neutrino flux. The obtained periodogram
             is consistent with statistical fluctuation and no
             significant periodicity was found. © 2003 The American
             Physical Society.},
   Doi = {10.1103/PhysRevD.68.092002},
   Key = {Yoo:2003rc}
}

@article{Ambrosio:2002qq,
   Author = {Ambrosio, M and Antolini, R and Auriemma, G and Bakari, D and Baldini,
             A and Barbarino, GC and Barish, BC and Battistoni, G and Becherini, Y and Bellotti, R and Bemporad, C and Bernardini, P and Bilokon, H and Bloise,
             C and Bower, C and Brigida, M and Bussino, S and Cafagna, F and Calicchio,
             M and Campana, D and Carboni, M and Caruso, R and Cecchini, S and Cei, F and Chiarella, V and Chiarusi, T and Choudhary, BC and Coutu, S and Cozzi,
             M and De Cataldo and G and Dekhissi, H and De Marzo and C and De Mitri and I and Derkaoui, J and De Vincenzi and M and Di Credico and A and Erriquez, O and Favuzzi, C and Forti, C et al.},
   Title = {Final results of magnetic monopole searches with the MACRO
             experiment},
   Journal = {The European Physical Journal C - Particles and
             Fields},
   Volume = {25},
   Number = {4},
   Pages = {511-522},
   Year = {2002},
   Month = {November},
   ISSN = {1434-6044},
   url = {http://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcApp=PARTNER_APP&SrcAuth=LinksAMR&KeyUT=WOS:000179928900002&DestLinkType=FullRecord&DestApp=ALL_WOS&UsrCustomerID=47d3190e77e5a3a53558812f597b0b92},
   Abstract = {We present the final results obtained by the MACRO
             experiment in the search for GUT magnetic monopoles in the
             penetrating cosmic radiation, for the range 4 × 10-5 &lt;
             β &lt; 1. Several searches with all the MACRO sub-detectors
             (i.e. scintillation counters, limited streamer tubes and
             nuclear track detectors) were performed, both in stand alone
             and combined ways. No candidates were detected and a 90%
             Confidence Level (C.L.) upper limit to the local magnetic
             monopole flux was set at the level of 1.4 × 10-16 cm-2 s-1
             sr-1. This result is the first experimental limit obtained
             in direct searches which is well below the Parker bound in
             the whole β range in which GUT magnetic monopoles are
             expected.},
   Doi = {10.1140/epjc/s2002-01046-9},
   Key = {Ambrosio:2002qq}
}

@article{Ambrosio:2002mb,
   Author = {Ambrosio, M and Antolini, R and Assiro, R and Auriemma, G and Bakari, D and Baldini, A and Barbarino, GC and Barbarito, E and Barish, BC and Battistoni, G and Becherini, Y and Bellotti, R and Bemporad, C and Bernardini, P and Bilokon, H and Bisi, V and Bloise, C and Bottazzi, E and Bower, C and Brigida, M and Bussino, S and Cafagna, F and Calicchio, M and Campana, D and Candela, A and Carboni, M and Cecchini, S and Cei, F and Ceres, A and Chiarella, V and Choudhary, BC and Coutu, S and Cozzi, M and Creti, P and De Cataldo and G and Degli Esposti and L and Dekhissi, H and De
             Marzo, C and De Mitri and I and Derkaoui, J et al.},
   Title = {The MACRO detector at Gran Sasso},
   Journal = {Nuclear Instruments and Methods in Physics Research Section
             A: Accelerators, Spectrometers, Detectors and Associated
             Equipment},
   Volume = {486},
   Number = {3},
   Pages = {663-707},
   Year = {2002},
   Month = {July},
   ISSN = {0168-9002},
   url = {http://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcApp=PARTNER_APP&SrcAuth=LinksAMR&KeyUT=WOS:000176945400010&DestLinkType=FullRecord&DestApp=ALL_WOS&UsrCustomerID=47d3190e77e5a3a53558812f597b0b92},
   Doi = {10.1016/S0168-9002(01)02169-6},
   Key = {Ambrosio:2002mb}
}

@article{fds326729,
   Author = {De Mitri and I},
   Title = {Search for massive rare particles with MACRO},
   Journal = {Nuclear Physics, Section B: Proceedings Supplements},
   Volume = {110},
   Pages = {186-188},
   Year = {2002},
   Month = {July},
   url = {http://dx.doi.org/10.1016/S0920-5632(02)01479-2},
   Doi = {10.1016/S0920-5632(02)01479-2},
   Key = {fds326729}
}

@article{Fukuda:2002nf,
   Author = {Fukuda, S and Fukuda, Y and Ishitsuka, M and Itow, Y and Kajita, T and Kameda, J and Kaneyuki, K and Kobayashi, K and Koshio, Y and Miura, M and Moriyama, S and Nakahata, M and Nakayama, S and Okada, A and Sakurai, N and Shiozawa, M and Suzuki, Y and Takeuchi, H and Takeuchi, Y and Toshito,
             T and Totsuka, Y and Yamada, S and Desai, S and Kearns, E and Messier, MD and Stone, JL and Sulak, LR and Walter, CW and Wang, W and Goldhaber, M and Casper, D and Gajewski, W and Kropp, WR and Mine, S and Liu, DW and Smy,
             MB and Sobel, HW and Vagins, MR and Ganezer, KS and Keig, WE and Ellsworth,
             RW and Tasaka, S and Kibayashi, A et al.},
   Title = {Search for neutrinos from gamma-ray bursts using
             Super-Kamiokande},
   Journal = {The Astrophysical Journal},
   Volume = {578},
   Number = {1 I},
   Pages = {317-324},
   Year = {2002},
   ISSN = {0004-637X},
   url = {http://arxiv.org/pdf/astro-ph/0205304},
   Abstract = {Using the Super-Kamiokande neutrino observatory, a search
             was conducted for neutrinos produced in coincidence with
             gamma-ray bursts observed by the Burst and Transient Source
             Experiment detector. Super-Kamiokande data in the neutrino
             energy range of 7 MeV ∼ 100 TeV were analyzed. For
             gamma-ray bursts that occurred between 1996 April and 2000
             May, no statistically significant signal in excess of the
             background levels was detected. Implied upper limits on
             associated gamma-ray burst neutrino production are
             presented.},
   Doi = {10.1086/342405},
   Key = {Fukuda:2002nf}
}

@article{Ambrosio:2001ai,
   Author = {Ambrosio, M and Antolini, R and Auriemma, G and Bakari, D and Baldini,
             A and Barbarino, GC and Barish, BC and Battistoni, G and Becherini, Y and Bellotti, R and Bemporad, C and Bernardini, P and Bilokon, H and Bloise,
             C and Bower, C and Brigida, M and Bussino, S and Cafagna, F and Calicchio,
             M and Campana, D and Carboni, M and Caruso, R and Cecchini, S and Cei, F and Chiarella, V and Choudhary, BC and Coutu, S and Cataldo, GD and Dekhissi, H and Marzo, CD and Mitri, ID and Derkaoui, J and Vincenzi,
             MD and Credico, AD and Erriquez, O and Favuzzi, C and Forti, C and Fusco,
             P and Giacomelli, G and Giannini, G et al.},
   Title = {A combined analysis technique for the search for fast
             magnetic monopoles with the MACRO detector},
   Journal = {Astroparticle Physics},
   Volume = {18},
   Number = {1},
   Pages = {27-41},
   Year = {2002},
   ISSN = {0927-6505},
   url = {http://arxiv.org/pdf/hep-ex/0110083},
   Abstract = {We describe a search method for fast moving (β = v/c &gt; 5
             × 10-3) magnetic monopoles using simultaneously the
             scintillator, streamer tube and track-etch subdetectors of
             the MACRO apparatus. The first two subdetectors are used
             primarily for the identification of candidates while the
             track-etch one is used as the final tool for their rejection
             or confirmation. Using this technique, a first sample of
             more than two years of data has been analyzed without any
             evidence of a magnetic monopole. We set a 90% CL upper limit
             to the local monopole flux of 1.5 × 10-15 cm-2 s-1 sr-1 in
             the velocity range 5 × 10-3 ≤ β ≤ 0.99 and for nucleon
             decay catalysis cross-section smaller than ∼1 mb © 2002
             Elsevier Science B.V. All rights reserved.},
   Doi = {10.1016/S0927-6505(01)00183-9},
   Key = {Ambrosio:2001ai}
}

@article{Walter:2002sa,
   Author = {Walter, CW},
   Title = {Quasi-elastic events and nuclear effects with the K2K Sci-Fi
             detector},
   Journal = {Nuclear Physics B - Proceedings Supplements},
   Volume = {111},
   Pages = {140-145},
   Year = {2002},
   Abstract = {The near detector complex of the K2K long-baseline neutrino
             experiment contains a scintillating fiber tracking detector.
             It is capable of detecting not only the muon but also the
             outgoing proton in neutrino-nucleon scattering. This allows
             for the enhancement of quasi-elastic interactions in the
             data sample. However, a proper modeling of the nuclear
             re-interactions of the proton is necessary to achieve
             reliable results.},
   Key = {Walter:2002sa}
}

@article{Ambrosio:2002du,
   Author = {Ambrosio, M and Antolini, R and Auriemma, G and Bakari, D and Baldini,
             A and Barbarino, GC and Barish, BC and Battistoni, G and Becherini, Y and Bellotti, R and Bemporad, C and Bernardini, P and Bilokon, H and Bloise,
             C and Bower, C and Brigida, M and Bussino, S and Cafagna, F and Calicchio,
             M and Campana, D and Candela, A and Carboni, M and Caruso, R and Cassese,
             F and Cecchini, S and Cei, F and Chiarella, V and Choudhary, BC and Coutu,
             S and Cozzi, M and Cataldo, GD and Deo, MD and Dekhissi, H and Marzo, CD and Mitri, ID and Derkaoui, J and Vincenzi, MD and Credico, AD and Dincecco,
             M and Erriquez, O et al.},
   Title = {Muon energy estimate through multiple scattering with the
             MACRO detector},
   Journal = {Nuclear Instruments and Methods in Physics Research Section
             A: Accelerators, Spectrometers, Detectors and Associated
             Equipment},
   Volume = {492},
   Number = {3},
   Pages = {376-386},
   Year = {2002},
   ISSN = {0168-9002},
   url = {http://arxiv.org/pdf/physics/0203018},
   Abstract = {Muon energy measurement represents an important issue for
             any experiment addressing neutrino-induced up-going muon
             studies. Since the neutrino oscillation probability depends
             on the neutrino energy, a measurement of the muon energy
             adds an important piece of information concerning the
             neutrino system. We show in this paper how the MACRO limited
             streamer tube system can be operated in drift mode by using
             the TDCs included in the QTPs, an electronics designed for
             magnetic monopole search. An improvement of the space
             resolution is obtained, through an analysis of the multiple
             scattering of muon tracks as they pass through our detector.
             This information can be used further to obtain an estimate
             of the energy of muons crossing the detector. Here we
             present the results of two dedicated tests, performed at
             CERN PS-T9 and SPS-X7 beam lines, to provide a full check of
             the electronics and to exploit the feasibility of such a
             multiple scattering analysis. We show that by using a neural
             network approach, we are able to reconstruct the muon energy
             for Eμ&lt;40 GeV. The test beam data provide an absolute
             energy calibration, which allows us to apply this method to
             MACRO data. © 2002 Elsevier Science B.V. All rights
             reserved.},
   Doi = {10.1016/S0168-9002(02)01413-4},
   Key = {Ambrosio:2002du}
}

@article{Ambrosio:2002qu,
   Author = {Ambrosio, M and Antolini, R and Auriemma, G and Bakari, D and Baldini,
             A and Barbarino, GC and Barish, BC and Battistoni, G and Becherini, Y and Bellotti, R and Bemporad, C and Bernardini, P and Bilokon, H and Bloise,
             C and Bower, C and Brigida, M and Bussino, S and Cafagna, F and Calicchio,
             M and Campana, D and Carboni, M and Caruso, R and Cecchini, S and Cei, F and Chiarella, V and Choudhary, BC and Coutu, S and Cozzi, M and Cataldo,
             GD and Dekhissi, H and Marzo, CD and Mitri, ID and Derkaoui, J and Vincenzi, MD and Credico, AD and Erriquez, O and Favuzzi, C and Forti,
             C and Fusco, P and Giacomelli, G et al.},
   Title = {Search for nucleon decays induced by GUT magnetic monopoles
             with the MACRO experiment},
   Journal = {The European Physical Journal C - Particles and
             Fields},
   Volume = {26},
   Number = {2},
   Pages = {163-172},
   Year = {2002},
   ISSN = {1434-6044},
   url = {http://arxiv.org/pdf/hep-ex/0207024},
   Abstract = {The interaction of a Grand Unification Magnetic Monopole
             with a nucleon can lead to a barion-number violating process
             in which the nucleon decays into a lepton and one or more
             mesons (catalysis of nucleon decay). In this paper we report
             an experimental study of the effects of a catalysis process
             in the MACRO detector. Using a dedicated analysis we obtain
             new magnetic monopole (MM) flux upper limits at the level of
             ∼ 3 · 10-16 cm-2 s-1 sr-1 for 1.1 · 10-4 ≤ |β| ≤ 5
             · 10-3, based on the search for catalysis events in the
             MACRO data. We also analyze the dependence of the MM flux
             limit on the catalysis cross section.},
   Doi = {10.1140/epjc/s2002-01045-x},
   Key = {Ambrosio:2002qu}
}

@article{Fukuda:2002pe,
   Author = {Fukuda, S and Fukuda, Y and Ishitsuka, M and Itow, Y and Kajita, T and Kameda, J and Kaneyuki, K and Kobayashi, K and Koshio, Y and Miura, M and Moriyama, S and Nakahata, M and Nakayama, S and Namba, T and Okada, A and Sakurai, N and Shiozawa, M and Suzuki, Y and Takeuchi, H and Takeuchi,
             Y and Totsuka, Y and Yamada, S and Desai, S and Earl, M and Kearns, E and Messier, MD and Stone, JL and Sulak, LR and Walter, CW and Goldhaber, M and Barszczak, T and Casper, D and Gajewski, W and Kropp, WR and Mine, S and Liu, DW and Smy, MB and Sobel, HW and Vagins, MR and Gago, A and Ganezer,
             KS and Keig, WE and Ellsworth, RW et al.},
   Title = {Determination of solar neutrino oscillation parameters using
             1496 days of Super-Kamiokande-I data},
   Journal = {Physics Letters B},
   Volume = {539},
   Number = {3-4},
   Pages = {179-187},
   Year = {2002},
   ISSN = {0370-2693},
   url = {http://arxiv.org/pdf/hep-ex/0205075},
   Abstract = {A number of different fits to solar neutrino mixing and mass
             square difference were performed using 1496 days of
             Super-Kamiokande-I's solar neutrino data. These data select
             two allowed areas at large neutrino mixing when combined
             with either the solar 8B flux prediction of the standard
             solar model or the SNO interaction rate measurements. A
             global fit combining SK data with the solar neutrino
             interaction rates measured by Homestake, SNO, Gallex/GNO and
             SAGE prefers a single allowed area, the Large Mixing Angle
             solution, at the 98.9% confidence level. The mass square
             difference Δm2 between the two mass eigenstates ranges from
             about 3 to 19 × 10-5 eV2, while the mixing angle θ is in
             the range of tan2θ ≈ 0.25-0.65. © 2002 Elsevier Science
             B.V. All rights reserved.},
   Doi = {10.1016/S0370-2693(02)02090-7},
   Key = {Fukuda:2002pe}
}

@article{fds318499,
   Author = {Ambrosio, M and Antolini, R and Auriemma, G and Bakari, D and Baldini,
             A and Barbarino, GC and Barish, BC and Battistoni, G and Becherini, Y and Bellotti, R and Bemporad, C and Bernardini, P and Bilokon, H and Bloise,
             C and Bower, C and Brigida, M and Bussino, S and Cafagna, F and Calicchio,
             M and Campana, D and Carboni, M and Caruso, R and Cecchini, S and Cei, F and Chiarella, V and Chiarusi, T and Choudhary, BC and Coutu, S and Cozzi,
             M and Cataldo, GD and Dekhissi, H and Marzo, CD and Mitri, ID and Derkaoui,
             J and Vincenzi, MD and Credico, AD and Erriquez, O and Favuzzi, C and Forti, C and Fusco, P et al.},
   Title = {Final results of magnetic monopole searches with the MACRO
             experiment: The MACRO collaboration},
   Journal = {The European Physical Journal C - Particles and
             Fields},
   Volume = {25},
   Number = {4},
   Pages = {511-522},
   Year = {2002},
   url = {http://dx.doi.org/10.1140/epjc/s2002-01046-9},
   Abstract = {We present the final results obtained by the MACRO
             experiment in the search for GUT magnetic monopoles in the
             penetrating cosmic radiation, for the range 4 × 10-5 &lt;
             β &lt; 1. Several searches with all the MACRO sub-detectors
             (i.e. scintillation counters, limited streamer tubes and
             nuclear track detectors) were performed, both in stand alone
             and combined ways. No candidates were detected and a 90%
             Confidence Level (C.L.) upper limit to the local magnetic
             monopole flux was set at the level of 1.4 × 10-16 cm-2 s-1
             sr-1. This result is the first experimental limit obtained
             in direct searches which is well below the Parker bound in
             the whole β range in which GUT magnetic monopoles are
             expected.},
   Doi = {10.1140/epjc/s2002-01046-9},
   Key = {fds318499}
}

@article{Ahn:2001cq,
   Author = {Ahn, SH and An, S and Aoki, A and Berns, HG and Bhang, HC and Boyd, S and Casper, D and Chikamatsu, T and Choi, JH and Echigo, S and Etoh, M and Fujii, K and Fukuda, S and Fukuda, Y and Gajewski, W and Golebiewska, U and Hara, T and Hasegawa, T and Hayato, Y and Hill, J and Hong, SJ and Ieiri,
             M and Inada, T and Inagaki, T and Ishida, T and Ishii, H and Ishii, T and Ishino, H and Ishitsuka, M and Itow, Y and Iwashita, T and Jang, HI and Jang, JS and Jeon, EJ and Jeong, EM and Jung, CK and Kadowaki, T and Kajita, T and Kameda, J and Kaneyuki, K and Kato, I and Kato, Y and Kearns,
             E and Kenmochi, S and Khang, BH and Kibayashi, A et
             al.},
   Title = {Detection of accelerator-produced neutrinos at a distance of
             250 km},
   Journal = {Physics Letters B},
   Volume = {511},
   Number = {2-4},
   Pages = {178-184},
   Year = {2001},
   Month = {July},
   ISSN = {0370-2693},
   url = {http://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcApp=PARTNER_APP&SrcAuth=LinksAMR&KeyUT=WOS:000169770800007&DestLinkType=FullRecord&DestApp=ALL_WOS&UsrCustomerID=47d3190e77e5a3a53558812f597b0b92},
   Abstract = {http://arxiv.org/abs/hep-ex/0103001},
   Doi = {10.1016/S0370-2693(01)00647-5},
   Key = {Ahn:2001cq}
}

@article{Fukuda:2001nk,
   Author = {Fukuda, S and Fukuda, Y and Ishitsuka, M and Itow, Y and Kajita, T and Kameda, J and Kaneyuki, K and Kobayashi, K and Koshio, Y and Miura, M and Moriyama, S and Nakahata, M and Nakayama, S and Okada, A and Sakurai, N and Shiozawa, M and Suzuki, Y and Takeuchi, H and Takeuchi, Y and Toshito,
             T and Totsuka, Y and Yamada, S and Desai, S and Earl, M and Kearns, E and Messier, MD and Scholberg, K and Stone, JL and Sulak, LR and Walter, CW and Goldhaber, M and Barszczak, T and Casper, D and Gajewski, W and Kropp,
             WR and Mine, S and Liu, DW and Price, LR and Smy, MB and Sobel, HW and Vagins,
             MR and Ganezer, KS and Keig, WE et al.},
   Title = {Constraints on neutrino oscillations using 1258 days of
             Super-Kamiokande solar neutrino data.},
   Journal = {Physical Review Letters},
   Volume = {86},
   Number = {25},
   Pages = {5656-5660},
   Year = {2001},
   Month = {June},
   ISSN = {0031-9007},
   url = {http://www.ncbi.nlm.nih.gov/pubmed/11415326},
   Abstract = {We report the result of a search for neutrino oscillations
             using precise measurements of the recoil electron energy
             spectrum and zenith angle variations of the solar neutrino
             flux from 1258 days of neutrino-electron scattering data in
             Super-Kamiokande. The absence of significant zenith angle
             variation and spectrum distortion places strong constraints
             on neutrino mixing and mass difference in a flux-independent
             way. Using the Super-Kamiokande flux measurement in
             addition, two allowed regions at large mixing are
             found.},
   Doi = {10.1103/PhysRevLett.86.5656},
   Key = {Fukuda:2001nk}
}

@article{Fukuda:2001nj,
   Author = {Fukuda, S and Fukuda, Y and Ishitsuka, M and Itow, Y and Kajita, T and Kameda, J and Kaneyuki, K and Kobayashi, K and Koshio, Y and Miura, M and Moriyama, S and Nakahata, M and Nakayama, S and Okada, A and Sakurai, N and Shiozawa, M and Suzuki, Y and Takeuchi, H and Takeuchi, Y and Toshito,
             T and Totsuka, Y and Yamada, S and Desai, S and Earl, M and Kearns, E and Messier, MD and Scholberg, K and Stone, JL and Sulak, LR and Walter, CW and Goldhaber, M and Barszczak, T and Casper, D and Gajewski, W and Kropp,
             WR and Mine, S and Liu, DW and Price, LR and Smy, MB and Sobel, HW and Vagins,
             MR and Ganezer, KS and Keig, WE et al.},
   Title = {Solar 8B and hep neutrino measurements from 1258 days of
             Super-Kamiokande data.},
   Journal = {Physical Review Letters},
   Volume = {86},
   Number = {25},
   Pages = {5651-5655},
   Year = {2001},
   Month = {June},
   ISSN = {0031-9007},
   url = {http://www.ncbi.nlm.nih.gov/pubmed/11415325},
   Abstract = {Solar neutrino measurements from 1258 days of data from the
             Super-Kamiokande detector are presented. The measurements
             are based on recoil electrons in the energy range 5.0-20.0
             MeV. The measured solar neutrino flux is
             2.32+/-0.03(stat)+0.08-0.07(syst)x10(6) cm(-2) x s(-1),
             which is 45.1+/-0.5(stat)+1.6-1.4(syst)% of that predicted
             by the BP2000 SSM. The day vs night flux asymmetry
             (Phi(n)-Phi(d))/Phi(average) is 0.033+/-0.022(stat)+0.013-0.012(syst).
             The recoil electron energy spectrum is consistent with no
             spectral distortion. For the hep neutrino flux, we set a 90%
             C.L. upper limit of 40x10(3) cm(-2) x s(-1), which is 4.3
             times the BP2000 SSM prediction.},
   Doi = {10.1103/PhysRevLett.86.5651},
   Key = {Fukuda:2001nj}
}

@article{fds318500,
   Author = {Bhatnagar, P and Glasheen, BM and Bains, SK and Long, SL and Minocha, R and Walter, C and Minocha, SC},
   Title = {Transgenic manipulation of the metabolism of polyamines in
             poplar cells.},
   Journal = {Plant physiology},
   Volume = {125},
   Number = {4},
   Pages = {2139-2153},
   Year = {2001},
   Month = {April},
   Abstract = {The metabolism of polyamines (putrescine, spermidine, and
             spermine) has become the target of genetic manipulation
             because of their significance in plant development and
             possibly stress tolerance. We studied the polyamine
             metabolism in non-transgenic (NT) and transgenic cells of
             poplar (Populus nigra x maximowiczii) expressing a mouse Orn
             decarboxylase (odc) cDNA. The transgenic cells showed
             elevated levels of mouse ODC enzyme activity, severalfold
             higher amounts of putrescine, a small increase in
             spermidine, and a small reduction in spermine as compared
             with NT cells. The conversion of labeled ornithine (Orn)
             into putrescine was significantly higher in the transgenic
             than the NT cells. Whereas exogenously supplied Orn caused
             an increase in cellular putrescine in both cell lines,
             arginine at high concentrations was inhibitory to putrescine
             accumulation. The addition of urea and glutamine had no
             effect on polyamines in either of the cell lines. Inhibition
             of glutamine synthetase by methionine sulfoximine led to a
             substantial reduction in putrescine and spermidine in both
             cell lines. The results show that: (a) Transgenic expression
             of a heterologous odc gene can be used to modulate
             putrescine metabolism in plant cells, (b) accumulation of
             putrescine in high amounts does not affect the native
             arginine decarboxylase activity, (c) Orn biosynthesis occurs
             primarily from glutamine/glutamate and not from catabolic
             breakdown of arginine, (d) Orn biosynthesis may become a
             limiting factor for putrescine production in the odc
             transgenic cells, and (e) assimilation of nitrogen into
             glutamine keeps pace with an increased demand for its use
             for putrescine production.},
   Key = {fds318500}
}

@article{Blaufuss:2000tp,
   Author = {Blaufuss, E and Guillian, G and Fukuda, Y and Fukuda, S and Ishitsuka,
             M and Itow, Y and Kajita, T and Kameda, J and Kaneyuki, K and Kobayashi, K and Kobayashi, Y and Koshio, Y and Miura, M and Moriyama, S and Nakahata, M and Nakayama, S and Obayashi, Y and Okada, A and Okumura, K and Sakurai, N and Shiozawa, M and Suzuki, Y and Takeuchi, B and Takeuchi, Y and Toshito,
             T and Totsuka, Y and Yamada, S and Earl, M and Habig, A and Kearns, E and Messier, MD and Scholberg, K and Stone, JL and Sulak, LR and Walter, CW and Goldhaber, M and Barszczak, T and Casper, D and Gajewski, W and Kropp,
             WR and Mine, S and Price, LR et al.},
   Title = {N-16 as a calibration source for Super-Kamiokande},
   Journal = {Nuclear Instruments and Methods in Physics Research Section
             A: Accelerators, Spectrometers, Detectors and Associated
             Equipment},
   Volume = {458},
   Number = {3},
   Pages = {638-649},
   Year = {2001},
   Month = {February},
   ISSN = {0168-9002},
   url = {http://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcApp=PARTNER_APP&SrcAuth=LinksAMR&KeyUT=WOS:000167040900004&DestLinkType=FullRecord&DestApp=ALL_WOS&UsrCustomerID=47d3190e77e5a3a53558812f597b0b92},
   Abstract = {http://arxiv.org/abs/hep-ex/0005014},
   Key = {Blaufuss:2000tp}
}

@article{fds248733,
   Author = {Blaufuss, E and Guillian, G and Fukuda, Y and Fukuda, S and Ishitsuka,
             M and Itow, Y and Kajita, T and Kameda, J and Kaneyuki, K and Kobayashi, K and Kobayashi, Y and Koshio, Y and Miura, M and Moriyama, S and Nakahata, M and Nakayama, S and Obayashi, Y and Okada, A and Okumura, K and Sakurai, N and Shiozawa, M and Suzuki, Y and Takeuchi, H and Takeuchi, Y and Toshito,
             T and Totsuka, Y and Yamada, S and Earl, M and Habig, A and Kearns, E and Messier, MD and Scholberg, K and Stone, JL and Sulak, LR and Walter, CW and Goldhaber, M and Barszczak, T and Casper, D and Gajewski, W and Kropp,
             WR and Mine, S and Price, LR et al.},
   Title = {16N as a calibration source for
             Super-Kamiokande},
   Journal = {Nuclear Instruments and Methods in Physics Research Section
             A: Accelerators, Spectrometers, Detectors and Associated
             Equipment},
   Volume = {458},
   Number = {3},
   Pages = {638-649},
   Year = {2001},
   ISSN = {0168-9002},
   url = {http://dx.doi.org/10.1016/S0168-9002(00)00900-1},
   Abstract = {The decay of 16N is used to cross check the absolute energy
             scale calibration for solar neutrinos established by the
             electron linear accelerator (LINAC). A deuterium-tritium
             neutron generator was employed to create 16N via the (n,p)
             reaction on 16O in the water of the detector. This technique
             is isotropic and has different systematic uncertainties than
             the LINAC. The results from this high-statistics data sample
             agree with the absolute energy scale of the LINAC to better
             than 1%. A natural source of 16N from the capture of μ- on
             16O, which is collected as a background to the solar
             neutrino analysis, is also discussed.},
   Doi = {10.1016/S0168-9002(00)00900-1},
   Key = {fds248733}
}

@article{Ambrosio:2001je,
   Author = {Ambrosio, M and Antolini, R and Auriemma, G and Bakari, D and Baldini,
             A and Barbarino, GC and Barish, BC and Battistoni, G and Becherini, Y and Bellotti, R and Bemporad, C and Bernardini, P and Bilokon, H and Bisi,
             V and Bloise, C and Bower, C and Brigida, M and Bussino, S and Cafagna, F and Calicchio, M and Campana, D and Carboni, M and Caruso, R and Cecchini,
             S and Cei, F and Chiarella, V and Choudhary, BC and Coutu, S and Cataldo,
             GD and Dekhissi, H and Marzo, CD and Mitri, ID and Derkaoui, J and Vincenzi, MD and Credico, AD and Erriquez, O and Favuzzi, C and Forti,
             C and Fusco, P and Giacomelli, G et al.},
   Title = {Matter effects in upward-going muons and sterile neutrino
             oscillations},
   Journal = {Physics Letters B},
   Volume = {517},
   Number = {1-2},
   Pages = {59-66},
   Year = {2001},
   ISSN = {0370-2693},
   url = {http://arxiv.org/pdf/hep-ex/0106049},
   Abstract = {The angular distribution of upward-going muons produced by
             atmospheric neutrinos in the rock below the MACRO detector
             shows anomalies in good agreement with two flavor vμ →
             vτ oscillations with maximum mixing and Δm2 around 0.0024
             eV2. Exploiting the dependence of magnitude of the matter
             effect on oscillation channel, and using a set of 809
             upward-going muons observed in MACRO, we show that the two
             flavor vμ → vs oscillation is disfavored with 99% C.L.
             with respect to vμ → vτ. © 2001 Elsevier Science B.V.
             All rights reserved.},
   Doi = {10.1016/S0370-2693(01)00992-3},
   Key = {Ambrosio:2001je}
}

@article{Ambrosio:2000yx,
   Author = {Ambrosio, M and Antolini, R and Auriemma, G and Bakari, D and Baldini,
             A and Barbarino, GC and Barish, BC and Battistoni, G and Bellotti, R and Bemporad, C and Bernardini, P and Bilokon, H and Bisi, V and Bloise, C and Bower, C and Brigida, M and Bussino, S and Cafagna, F and Calicchio, M and Campana, D and Carboni, M and Cecchini, S and Cei, F and Chiarella, V and Choudhary, BC and Coutu, S and Cataldo, GD and Dekhissi, H and Marzo,
             CD and Mitri, ID and Derkaoui, J and Vincenzi, MD and Credico, AD and Erriquez, O and Favuzzi, C and Forti, C and Fusco, P and Giacomelli, G and Giannini, G and Giglietto, N et al.},
   Title = {Neutrino astronomy with the macro detector},
   Journal = {The Astrophysical Journal},
   Volume = {546},
   Number = {2 PART 1},
   Pages = {1038-1054},
   Year = {2001},
   ISSN = {0004-637X},
   url = {http://arxiv.org/pdf/astro-ph/0002492},
   Abstract = {High-energy gamma-ray astronomy is now a well-established
             field, and several sources have been discovered in the
             region from a few giga-electron volts up to several
             tera-electron volts. If sources involving hadronic processes
             exist, the production of photons would be accompanied by
             neutrinos too. Other possible neutrino sources could be
             related to the annihilation of weakly interacting, massive
             particles (WIMPs) at the center of galaxies with black
             holes. We present the results of a search for pointlike
             sources using 1100 upward-going muons produced by neutrino
             interactions in the rock below and inside the Monopole
             Astrophysics and Cosmic Ray Observatory (MACRO) detector in
             the underground Gran Sasso Laboratory. These data show no
             evidence of a possible neutrino pointlike source or of
             possible correlations between gamma-ray bursts and
             neutrinos. They have been used to set flux upper limits for
             candidate pointlike sources which are in the range
             10-14-10-15 cm-2 s-1.},
   Doi = {10.1086/318281},
   Key = {Ambrosio:2000yx}
}

@article{Fukuda:2000np,
   Author = {Fukuda, S and Fukuda, Y and Ishitsuka, M and Kajita, T and Kameda, J and Kaneyuki, K and Kobayashi, K and Koshio, Y and Miura, M and Moriyama, S and Nakahata, M and Nakayama, S and Obayashi, Y and Okada, A and Okumura, K and Sakurai, N and Shiozawa, M and Suzuki, Y and Takeuchi, H and Takeuchi,
             Y and Toshito, T and Totsuka, Y and Yamada, S and Earl, M and Habig, A and Kearns, E and Messier, MD and Scholberg, K and Stone, JL and Sulak, LR and Walter, CW and Goldhaber, M and Barszczak, T and Casper, D and Gajewski,
             W and Kropp, WR and Mine, S and Price, LR and Smy, M and Sobel, HW and Vagins,
             MR and Ganezer, KS et al.},
   Title = {Tau neutrinos favored over sterile neutrinos in atmospheric
             muon neutrino oscillations.},
   Journal = {Physical Review Letters},
   Volume = {85},
   Number = {19},
   Pages = {3999-4003},
   Year = {2000},
   Month = {November},
   ISSN = {0031-9007},
   url = {http://www.ncbi.nlm.nih.gov/pubmed/11056609},
   Abstract = {The previously published atmospheric neutrino data did not
             distinguish whether muon neutrinos were oscillating into tau
             neutrinos or sterile neutrinos, as both hypotheses fit the
             data. Using data recorded in 1100 live days of the
             Super-Kamiokande detector, we use three complementary data
             samples to study the difference in zenith angle distribution
             due to neutral currents and matter effects. We find no
             evidence favoring sterile neutrinos, and reject the
             hypothesis at the 99% confidence level. On the other hand,
             we find that oscillation between muon and tau neutrinos
             suffices to explain all the results in hand.},
   Doi = {10.1103/PhysRevLett.85.3999},
   Key = {Fukuda:2000np}
}

@article{Ambrosio:2000kh,
   Author = {Ambrosio, M and Antolini, R and Auriemma, G and Bakari, D and Baldini,
             A and Barbarino, GC and Barish, BC and Battistoni, G and Bellotti, R and Bemporad, C and Bernardini, P and Bilokon, H and Bisi, V and Bloise, C and Bower, C and Brigida, M and Bussino, S and Cafagna, F and Calicchio, M and Campana, D and Carboni, M and Cecchini, S and Cei, F and Chiarella, V and Choudhary, BC and Coutu, S and De Cataldo and G and Dekhissi, H and De
             Marzo, C and De Mitri and I and Derkaoui, J and De Vincenzi and M and Di
             Credico, A and Erriquez, O and Favuzzi, C and Forti, C and Fusco, P and Giacomelli, G and Giannini, G et al.},
   Title = {Search for lightly ionizing particles with the MACRO
             detector},
   Journal = {Physical Review D: Particles, Fields, Gravitation and
             Cosmology},
   Volume = {62},
   Number = {5},
   Pages = {052003},
   Year = {2000},
   Month = {September},
   ISSN = {0556-2821},
   url = {http://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcApp=PARTNER_APP&SrcAuth=LinksAMR&KeyUT=WOS:000089022500007&DestLinkType=FullRecord&DestApp=ALL_WOS&UsrCustomerID=47d3190e77e5a3a53558812f597b0b92},
   Abstract = {http://arxiv.org/abs/hep-ex/0002029},
   Doi = {10.1103/PhysRevD.62.052003},
   Key = {Ambrosio:2000kh}
}

@article{fds326730,
   Author = {Akhmadaliev, S and Albiol, F and Amaral, P and Ambrosini, G and Amorim,
             A and Anderson, K and Andrieux, ML and Aubert, B and Augé, E and Badaud,
             F and Baisin, L and Barreiro, F and Battistoni, G and Bazan, A and Bazizi,
             K and Bee, C and Belorgey, J and Belymam, A and Benchekroun, D and Berglund, S and Berset, JC and Blanchot, G and Bogush, A and Bohm, C and Boldea, V and Bonivento, W and Borgeaud, P and Borisov, O and Bosman, M and Bouhemaid, N and Breton, D and Brette, P and Bromberg, C and Budagov, J and Burdin, S and Caloba, L and Camarena, F and Camin, DV and Canton, B and Caprini, M and Carvalho, J et al.},
   Title = {Results from a new combined test of an electromagnetic
             liquid argon calorimeter with a hadronic scintillating-tile
             calorimeter},
   Journal = {Nuclear Instruments and Methods in Physics Research Section
             A: Accelerators, Spectrometers, Detectors and Associated
             Equipment},
   Volume = {449},
   Number = {3},
   Pages = {461-477},
   Year = {2000},
   Month = {July},
   url = {http://dx.doi.org/10.1016/S0168-9002(00)00153-4},
   Doi = {10.1016/S0168-9002(00)00153-4},
   Key = {fds326730}
}

@article{Ambrosio:2000ja,
   Author = {Ambrosio, M and Antolini, R and Auriemma, G and Bakari, D and Baldini,
             A and Barbarino, GC and Barish, BC and Battistoni, G and Bellotti, R and Bemporad, C and Bernardini, P and Bilokon, H and Bisi, V and Bloise, C and Bower, C and Brigida, M and Bussino, S and Cafagna, F and Calicchio, M and Campana, D and Carboni, M and Cecchini, S and Cei, F and Chiarella, V and Choudhary, BC and Coutu, S and De Cataldo and G and Dekhissi, H and De
             Marzo, C and De Mitri and I and Derkaoui, J and De Vincenzi and M and Di
             Credico, A and Erriquez, O and Favuzzi, C and Forti, C and Fusco, P and Giacomelli, G and Giannini, G et al.},
   Title = {Low energy atmospheric muon neutrinos in
             MACRO},
   Journal = {Physics Letters B},
   Volume = {478},
   Number = {1-3},
   Pages = {5-13},
   Year = {2000},
   Month = {April},
   ISSN = {0370-2693},
   url = {http://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcApp=PARTNER_APP&SrcAuth=LinksAMR&KeyUT=WOS:000086540600002&DestLinkType=FullRecord&DestApp=ALL_WOS&UsrCustomerID=47d3190e77e5a3a53558812f597b0b92},
   Abstract = {http://arxiv.org/abs/hep-ex/0001044},
   Doi = {10.1016/S0370-2693(00)00267-7},
   Key = {Ambrosio:2000ja}
}

@article{fds248731,
   Author = {Patrizii, L and Ambrosio, M and Antolini, R and Aramo, C and Auriemma,
             G and Bakari, D and Baldini, A and Barbarino, GC and Barish, BC and Battistoni, G and Bellotti, R and Bemporad, C and Bernardini, P and Bilokon, H and Bisi, V and Bloise, C and Bower, C and Bussino, S and Cafagna, F and Calicchio, M and Campana, D and Carboni, M and Castellano, M and Cecchini, S and Cei, F and Chiarella, V and Choudhary,
             BC and Coutu, S and Benedicts, LD and Cataldo, GD and Dekhissi, H and Marzo, CD and Mitri, ID and Derkaoui, J and Vincenzi, MD and Credico,
             AD and Erriquez, O and Favuzzi, C and Forti, C and Fusco, P et
             al.},
   Title = {Search for massive rare particles with the MACRO detector at
             Gran Sasso},
   Journal = {Nuclear Physics, Section B: Proceedings Supplements},
   Volume = {85},
   Number = {1-3},
   Pages = {221-226},
   Year = {2000},
   ISSN = {0920-5632},
   Abstract = {Searches for massive penetrating particles in the cosmic
             radiation have been performed with the MACRO detector.
             Scintillators, streamer tubes (instrumented with specialized
             electronics) and nuclear track detectors have been used to
             search for signatures coming from magnetic monopoles (MMs);
             the scintillator and the nuclear track subdetectors were
             also used for searches for other rare particles
             (nuclearites, charged Q-balls). Based on no observation of
             such signals, we establish stringent flux limits, for MMs as
             slow as a few 10-5 c.},
   Key = {fds248731}
}

@article{fds248732,
   Author = {Ambrosio, M and Antolini, R and Auriemma, G and Bakari, D and Baldini,
             A and Barbarino, GC and Barish, BC and Battistoni, G and Bellotti, R and Bemporad, C and Bernardini, P and Bilokon, H and Bisi, V and Bloise, C and Bower, C and Brigida, M and Bussino, S and Cafagna, F and Calicchio, M and Campana, D and Carboni, M and Cecchini, S and Cei, F and Chiarella, V and Choudhary, BC and Coutu, S and Cataldo, GD and Dekhissi, H and Marzo,
             CD and Mitri, ID and Derkaoui, J and Vincenzi, MD and Credico, AD and Erriquez, O and Favuzzi, C and Forti, C and Fusco, P and Giacomelli, G and Giannini, G and Giglietto, N et al.},
   Title = {Search for lightly ionizing particles with the MACRO
             detector},
   Journal = {Physical Review D: Particles, Fields, Gravitation and
             Cosmology},
   Volume = {62},
   Number = {5},
   Pages = {1-9},
   Year = {2000},
   ISSN = {0556-2821},
   Abstract = {A search for lightly ionizing particles has been performed
             with the MACRO detector. This search was sensitive to
             particles with charges between 1/5 e and close to the charge
             of an electron, with β between approximately 0.25 and 1.0.
             Unlike previous searches both single track events and tracks
             buried within high multiplicity muon showers were examined.
             In a period of approximately one year no candidates were
             observed. Assuming an isotropic flux, for the single track
             sample this corresponds to a 90% C.L. upper flux limit Φ
             ≤9.2×10-15 cm-2 s-1 sr-1. ©2000 The American Physical
             Society.},
   Key = {fds248732}
}

@article{Suzuki:2000nj,
   Author = {Suzuki, A and Park, H and Aoki, S and Echigo, S and Fujii, K and Hara, T and Iwashita, T and Kitamura, M and Kohama, M and Kume, G and Onchi, M and Otaki, T and Sato, K and Takatsuki, M and Takenaka, K and Tanaka, Y and Tashiro, K and Inagaki, T and Kato, I and Mukai, S and Nakaya, T and Nishikawa, K and Sasao, N and Shima, A and Yokoyama, H and Chikamatsu,
             T and Hayato, Y and Ishida, T and Ishii, T and Ishino, H and Jeon, EJ and Kobayashi, T and Lee, SB and Nakamura, K and Oyama, Y and Sakai, A and Sakuda, M and Tumakov, V and Fukuda, S and Fukuda, Y and Ishizuka, M and Itow, Y and Kajita, T and Kameda, J and Kaneyuki, K et
             al.},
   Title = {Design, construction, and operation of SciFi tracking
             detector for K2K experiment},
   Journal = {Nuclear Instruments and Methods in Physics Research Section
             A: Accelerators, Spectrometers, Detectors and Associated
             Equipment},
   Volume = {453},
   Number = {1-2},
   Pages = {165-176},
   Year = {2000},
   ISSN = {0168-9002},
   url = {http://arxiv.org/pdf/hep-ex/0004024},
   Abstract = {We describe the construction and performance of a
             scintillating fiber detector used in the near detector for
             the K2K (KEK to Kamioka, KEK E362) long baseline neutrino
             oscillation experiment. The detector uses 3.7 m long and
             0.692 mm diameter scintillating fiber coupled to
             image-intensifier tubes (IIT), and a CCD camera readout
             system. Fiber sheet production and detector construction
             began in 1997, and the detector was commissioned in March
             1999. Results from the first K2K runs confirm good initial
             performance: position resolution is estimated to be about
             0.8 mm, and track finding efficiency is 98±2% for long
             tracks (i.e., those which intersect more than 5 fiber
             planes). The hit efficiency was estimated to be 92±2% using
             cosmic-ray muons, after noise reduction at the offline
             stage. The possibility of using the detector for particle
             identification is also discussed.},
   Doi = {10.1016/S0168-9002(00)00624-0},
   Key = {Suzuki:2000nj}
}

@article{Ambrosio:1999gj,
   Author = {Ambrosio et al., M},
   Title = {Nuclearite search with the MACRO detector at Gran
             Sasso},
   Journal = {The European Physical Journal C - Particles and
             Fields},
   Volume = {13},
   Number = {3},
   Pages = {453-453},
   Year = {2000},
   ISSN = {1434-6044},
   url = {http://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcApp=PARTNER_APP&SrcAuth=LinksAMR&KeyUT=WOS:000086888100006&DestLinkType=FullRecord&DestApp=ALL_WOS&UsrCustomerID=47d3190e77e5a3a53558812f597b0b92},
   Abstract = {http://arxiv.org/abs/hep-ex/9904031},
   Doi = {10.1007/s100520050708},
   Key = {Ambrosio:1999gj}
}

@booklet{Ambrosio99,
   Author = {Ambrosio, and M, and others},
   Title = {Limits on dark matter WIMPs using upward-going muons in the
             MACRO detector},
   Journal = {Physical Review D},
   Volume = {6008},
   Number = {8},
   Pages = {art. no.-082002},
   Year = {1999},
   Month = {October},
   Abstract = {We perform an indirect search for weakly interacting massive
             particles (WIMPs) using the MACRO detector to look for
             neutrino-induced upward-going muons resulting from the
             annihilation of WIMPs trapped in the Sun and Earth. The
             search is conducted in various angular cones centered on the
             Sun and Earth to accommodate a range of WIMP masses. No
             significant excess over the background from atmospheric
             neutrinos is seen. We set experimental flux limits on the
             upward-going muon fluxes from the Sun and the Earth. These
             limits are used to constrain neutralino particle parameters
             from supersymmetric theory, including those suggested by
             recent results from DAMA-NaI. ©1999 The American Physical
             Society.},
   Key = {Ambrosio99}
}

@booklet{Ambrosio99a,
   Author = {Ambrosio, and M, and others},
   Title = {High statistics measurement of the underground muon pair
             separation at Gran Sasso},
   Journal = {Physical Review D},
   Volume = {6003},
   Number = {3},
   Pages = {1-13},
   Year = {1999},
   Month = {August},
   Key = {Ambrosio99a}
}

@booklet{Ambrosio99c,
   Author = {Ambrosio, and M, and others},
   Title = {Observation of the shadowing of cosmic rays by the Moon
             using a deep underground detector},
   Journal = {Physical Review D},
   Volume = {5901},
   Number = {1},
   Pages = {art. no.-012003},
   Year = {1999},
   Month = {January},
   Abstract = {Using data collected by the MACRO experiment during the
             years 1989-1996, we show evidence for the shadow of the Moon
             in the underground cosmic ray flux with a significance of
             3.6σ. This detection of the shadowing effect is the first
             by an underground detector. A maximum-likelihood analysis is
             used to determine that the angular resolution of the
             apparatus is 0.9°±0.3°. These results demonstrate
             MACRO'S capabilities as a muon telescope by confirming its
             absolute pointing ability and quantifying its angular
             resolution. ©1998 The American Physical
             Society.},
   Key = {Ambrosio99c}
}

@article{fds326731,
   Author = {Battistoni, G},
   Title = {Experimental study of hadronic interaction models using
             coincident data from EAS-TOP and MACRO},
   Journal = {Nuclear Physics, Section B: Proceedings Supplements},
   Volume = {70},
   Number = {1-3},
   Pages = {483-485},
   Year = {1999},
   Month = {January},
   url = {http://dx.doi.org/10.1016/S0920-5632(98)00477-0},
   Doi = {10.1016/S0920-5632(98)00477-0},
   Key = {fds326731}
}

@booklet{Hayato99,
   Author = {Hayato, Y and Earl, M and Fukuda, Y and Hayakawa, T and Inoue, K and Ishihara, K and Ishino, H and Itow, Y and Kajita, T and Kameda, J and Kasuga, S and Kobayashi, K and Kobayashi, Y and Koshio, Y and Miura, M and Nakahata, M and Nakayama, S and Obayashi, Y and Okada, A and Okumura, K and Sakurai, N and Shiozawa, M and Suzuki, Y and Takeuchi, H and Takeuchi,
             Y and Totsuka, Y and Yamada, S and Habig, A and Kearns, E and Messier, MD and Scholberg, K and Stone, JL and Sulak, LR and Walter, CW and Goldhaber,
             M and Barszczak, T and Casper, D and Gajewski, W and Kropp, WR and Mine, S and Price, LR and Smy, M and Sobel, HW et al.},
   Title = {Search for proton decay through p → ν̄K+ in a
             large water cherenkov detector},
   Journal = {Physical Review Letters},
   Volume = {83},
   Number = {8},
   Pages = {1529-1533},
   Year = {1999},
   Abstract = {We present results of a search for proton decays, p →
             ν̄K+, using data from a 33 kt · yr exposure of the
             Super-Kamiokande detector. Two decay modes of the kaon, K+
             → μ+νμ and K+ → π+π0, were studied. The data were
             consistent with the background expected from atmospheric
             neutrinos; therefore a lower limit on the partial lifetime
             of the proton τ/B(p → ν̄K+) was found to be 6.7 × 1032
             years at 90% confidence level. © 1999 The American Physical
             Society.},
   Key = {Hayato99}
}

@booklet{Ambrosio99d,
   Author = {Ambrosio, M and Antolini, R and Aramo, C and Auriemma, G and Baldini, A and Barbarino, GC and Barish, BC and Battistoni, G and Bellotti, R and Bemporad, C and Bernardini, P and Bilokon, H and Bisi, V and Bloise, C and Bower, C and Bussino, S and Cafagna, F and Calicchio, M and Campana, D and Carboni, M and Castellano, M and Cecchini, S and Cei, F and Chiarella,
             V and Choudhary, BC and Coutu, S and Benedictis, LD and Cataldo, GD and Dekhissi, H and Marzo, CD and Mitri, ID and Derkaoui, J and Vincenzi,
             MD and Credico, AD and Erriquez, O and Favuzzi, C and Forti, C and Fusco,
             P and Giacomelli, G and Giannini, G et al.},
   Title = {Measurement of the energy spectrum of underground muons at
             Gran Sasso with a transition radiation detector},
   Journal = {Astroparticle Physics},
   Volume = {10},
   Number = {1},
   Pages = {11-20},
   Year = {1999},
   ISSN = {0927-6505},
   Abstract = {We have measured directly the residual energy of cosmic ray
             muons crossing the MACRO detector at the Gran Sasso
             Laboratory. For this measurement we have used a transition
             radiation detector consisting of three identical modules,
             each of about 12m2 area, operating in the energy region from
             100 GeV to 1 TeV. The results presented here were obtained
             with the first module collecting data for more than two
             years. The average single muon energy is found to be 320 ±
             4 (stat.) ± 11 (syst.) GeV in the rock depth range
             3000-6500 hg/cm2. The results are in agreement with
             calculations of the energy loss of muons in the rock above
             the detector. © 1999 Elsevier Science B.V.},
   Key = {Ambrosio99d}
}

@booklet{Fukuda99b,
   Author = {Fukuda, Y and Hayakawa, T and Ichihara, E and Inoue, K and Ishihara, K and Ishino, H and Itow, Y and Kajita, T and Kameda, J and Kasuga, S and Kobayashi, K and Kobayashi, Y and Koshio, Y and Miura, M and Nakahata,
             M and Nakayama, S and Okada, A and Okumura, K and Sakurai, N and Shiozawa,
             M and Suzuki, Y and Takeuchi, Y and Totsuka, Y and Yamada, S and Earl, M and Habig, A and Kearns, E and Messier, MD and Scholberg, K and Stone, JL and Sulak, LR and Walter, CW and Goldhaber, M and Barszczak, T and Casper,
             D and Gajewski, W and Kropp, WR and Price, LR and Reines, F and Smy, M and Sobel, HW and Vagins, MR et al.},
   Title = {Measurement of the flux and zenith-angle distribution of
             upward throughgoing muons by Super-Kamiokande},
   Journal = {Physical Review Letters},
   Volume = {82},
   Number = {13},
   Pages = {2644-2648},
   Year = {1999},
   Abstract = {A total of 614 upward throughgoing mouns of minimum energy
             1.6 GeV are observed by Super-Kamiokande during 537 detector
             live days. The measured muon flux is [1.74 ± 0.07(stat) ±
             0.02(sys)] × 10-13cm-2s-1sr-1 compared to an expected flux
             of [1.97 ± 0.44(theor)] × 10-13cm-2s-1sr-1. The absolute
             measured flux is in agreement with the prediction within the
             errors. However, the zenith-angle dependence of the observed
             upward throughgoing muon flux does not agree with
             no-oscillation predictions. The observed distortion in shape
             is consistent with the νμ ↔ ντ oscillation hypothesis
             with sin2 2θ &gt; 0.4 and 1 × 10-3 &lt; 1 × 10-1 &lt;
             δm2 &lt; 1 × 10-1 eV2 at 90% confidence level. © 1999 The
             American Physical Society.},
   Key = {Fukuda99b}
}

@booklet{Fukuda99c,
   Author = {Fukuda, Y and Hayakawa, T and Ichihara, E and Inoue, K and Ishihara, K and Ishino, H and Itow, Y and Kajita, T and Kameda, J and Kasuga, S and Kobayashi, K and Kobayashi, Y and Koshio, Y and Miura, M and Nakahata,
             M and Nakayama, S and Okada, A and Okumura, K and Sakurai, N and Shiozawa,
             M and Suzuki, Y and Takeuchi, Y and Totsuka, Y and Yamada, S and Earl, M and Habig, A and Kearns, E and Messier, MD and Scholberg, K and Stone, JL and Sulak, LR and Walter, CW and Goldhaber, M and Barszczak, T and Casper,
             D and Gajewski, W and Halverson, PG and Hsu, J and Kropp, WR and Price, LR and Reines, F and Smy, M and Sobel, HW et al.},
   Title = {Constraints on Neutrino Oscillation Parameters from the
             Measurement of Day-Night Solar Neutrino Fluxes at
             Super-Kamiokande},
   Journal = {Physical Review Letters},
   Volume = {82},
   Number = {9},
   Pages = {1810-1814},
   Year = {1999},
   ISSN = {0031-9007},
   Abstract = {A search for day-night variations in the solar neutrino flux
             resulting from neutrino oscillations has been carried out
             using the 504 day sample of solar neutrino data obtained at
             Super-Kamiokande. The absence of a significant day-night
             variation has set an absolute flux independent exclusion
             region in the two neutrino oscillation parameter
             space.},
   Key = {Fukuda99c}
}

@booklet{Takeuchi99,
   Author = {Takeuchi, Y and Okumura, K and Kajita, T and Tasaka, S and Nemoto, M and Fukuda, Y and Okazawa, H and Hayakawa, T and Ishihara, K and Ishino, H and Itow, Y and Kameda, J and Kasuga, S and Kobayashi, K and Kobayashi, Y and Koshio, Y and Miura, M and Nakahata, M and Nakayama, S and Obayashi, Y and Okada, A and Sakurai, N and Shiozawa, M and Suzuki, Y and Takeuchi, H and Totsuka, Y and Yamada, S and Earl, M and Habig, A and Kearns, E and Messier, MD and Scholberg, K and Stone, JL and Sulak, LR and Walter, CW and Goldhaber, M and Barszczak, T and Casper, D and Gajewski, W and Kropp,
             WR and Mine, S and Price, LR and Smy, M et al.},
   Title = {Measurement of radon concentrations at Super-Kamiokande},
   Journal = {Physics Letters B},
   Volume = {452},
   Number = {3-4},
   Pages = {418-424},
   Year = {1999},
   ISSN = {0370-2693},
   Abstract = {Radioactivity from radon is a major background for observing
             solar neutrinos at Super-Kamiokande. In this paper, we
             describe the measurement of radon concentrations at
             Super-Kamiokande, the method of radon reduction, and the
             radon monitoring system. The measurement shows that the
             current low-energy event rate between 5.0 MeV and 6.5 MeV
             implies a radon concentration in the Super-Kamiokande water
             of less than 1.4 mBq/m3. © 1999 Published by Elsevier
             Science B.V. All rights reserved.},
   Key = {Takeuchi99}
}

@booklet{Fukuda99a,
   Author = {Fukuda, Y and Hayakawa, T and Ichihara, E and Inoue, K and Ishihara, K and Ishino, H and Itow, Y and Kajita, T and Kameda, J and Kasuga, S and Kobayashi, K and Kobayashi, Y and Koshio, Y and Miura, M and Nakahata,
             M and Nakayama, S and Okada, A and Okumura, K and Sakurai, N and Shiozawa,
             M and Suzuki, Y and Takeuchi, Y and Totsuka, Y and Yamada, S and Earl, M and Habig, A and Kearns, E and Messier, MD and Scholberg, K and Stone, JL and Sulak, LR and Walter, CW and Goldhaber, M and Barszczak, T and Casper,
             D and Gajewski, W and Halverson, PG and Hsu, J and Kropp, WR and Price, LR and Reines, F and Smy, M and Sobel, HW et al.},
   Title = {Measurement of the solar neutrino energy spectrum using
             neutrino-electron scattering},
   Journal = {Physical Review Letters},
   Volume = {82},
   Number = {12},
   Pages = {2430-2434},
   Year = {1999},
   Abstract = {A measurement of the energy spectrum of recoil electrons
             from solar neutrino scattering in the Super-Kamiokande
             detector is presented. The results shown here were obtained
             from 504 days of data taken between 31 May 1996 and 25 March
             1998. The shape of the measured spectrum is compared with
             the expectation for solar 8B neutrinos. The comparison takes
             into account both kinematic and detector related effects in
             the measurement process. The spectral shape comparison
             between the observation and the expectation gives a χ2 of
             25.3 with 15 degrees of freedom, corresponding to a 4.6%
             confidence level. © 1999 The American Physical
             Society.},
   Key = {Fukuda99a}
}

@booklet{Futagami99,
   Author = {Futagami, T and Fukuda, Y and Hayakawa, T and Inoue, K and Ishihara, K and Ishino, H and Itow, Y and Kajita, T and Kameda, J and Kasuga, S and Kobayashi, K and Kobayashi, Y and Koshio, Y and Miura, M and Nakahata,
             M and Nakayama, S and Obayashi, Y and Okada, A and Okumura, K and Sakurai,
             N and Shiozawa, M and Suzuki, Y and Takeuchi, H and Takeuchi, Y and Totsuka, Y and Yamada, S and Earl, M and Habig, A and Kearns, E and Messier, MD and Scholberg, K and Stone, JL and Sulak, LR and Walter, CW and Goldhaber, M and Barszczak, T and Casper, D and Gajewski, W and Kropp,
             WR and Mine, S and Price, LR and Smy, M and Sobel, HW et
             al.},
   Title = {Observation of the east-west anisotropy of the atmospheric
             neutrino flux},
   Journal = {Physical Review Letters},
   Volume = {82},
   Number = {26 I},
   Pages = {5194-5197},
   Year = {1999},
   ISSN = {0031-9007},
   url = {http://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcApp=PARTNER_APP&SrcAuth=LinksAMR&KeyUT=WOS:000081152700004&DestLinkType=FullRecord&DestApp=ALL_WOS&UsrCustomerID=47d3190e77e5a3a53558812f597b0b92},
   Abstract = {The east-west anisotropy, caused by the deflection of
             primary cosmic rays in the Earth's magnetic field, is
             observed for the first time in the flux of atmospheric
             neutrinos. Using a 45 kt yr exposure of the Super-Kamiokande
             detector, 552 e-like and 633 μ-like horizontally going
             events are selected in the momentum range between 400 and
             3000 MeV/c. The azimuthal distributions of e-like and
             μ-like events agree with the expectation from atmospheric
             neutrino flux calculations, verifying that the flux of
             atmospheric neutrinos in the GeV energy range is reasonably
             well modeled by calculations that account for the
             geomagnetic field. © 1999 The American Physical
             Society.},
   Doi = {10.1103/PhysRevLett.82.5194},
   Key = {Futagami99}
}

@booklet{Nakahata99,
   Author = {Nakahata, M and Fukuda, Y and Hayakawa, T and Ichihara, E and Inoue, K and Ishihara, K and Ishino, H and Itow, Y and Kajita, T and Kameda, J and Kasuga, S and Kobayashi, K and Kobayashi, Y and Koshio, Y and Martens,
             K and Miura, M and Nakayama, S and Okada, A and Okumura, K and Sakurai, N and Shiozawa, M and Suzuki, Y and Takeuchi, Y and Totsuka, Y and Yamada, S and Earl, M and Habig, A and Kearns, E and Messier, MD and Scholberg, K and Stone, JL and Sulak, LR and Walter, CW and Goldhaber, M and Barszczak,
             T and Casper, D and Gajewski, W and Halverson, PG and Hsu, J and Kropp, WR and Price, LR and Reines, F and Smy, M et al.},
   Title = {Calibration of Super-Kamiokande using an electron
             LINAC},
   Journal = {Nuclear Instruments and Methods in Physics Research Section
             A: Accelerators, Spectrometers, Detectors and Associated
             Equipment},
   Volume = {421},
   Number = {1-2},
   Pages = {113-129},
   Year = {1999},
   ISSN = {0168-9002},
   url = {http://dx.doi.org/10.1016/S0168-9002(98)01200-5},
   Abstract = {In order to calibrate the Super-Kamiokande experiment for
             solar neutrino measurements, a linear accelerator (LINAC)
             for electrons was installed at the detector. LINAC data were
             taken at various positions in the detector volume, tracking
             the detector response in the variables relevant to solar
             neutrino analysis. In particular, the absolute energy scale
             is now known with less than 1% uncertainty. © 1999 Elsevier
             Science B.V. All rights reserved.},
   Doi = {10.1016/S0168-9002(98)01200-5},
   Key = {Nakahata99}
}

@booklet{Ambrosio99b,
   Author = {Ambrosio, M and Antolini, R and Aramo, C and Auriemma, G and Baldini, A and Barbarino, GC and Barish, BC and Battistoni, G and Bellotti, R and Bemporad, C and Bernardini, P and Bilokon, H and Bisi, V and Bloise, C and Bower, C and Bussino, S and Cafagna, F and Calicchio, M and Campana, D and Carboni, M and Castellano, M and Cecchini, S and Cei, F and Chiarella,
             V and Coutu, S and Benedictis, LD and Cataldo, GD and Dekhissi, H and Marzo, CD and Mitri, ID and Vincenzi, MD and Credico, AD and Erriquez,
             O and Favuzzi, C and Forti, C and Fusco, R and Giacomelli, G and Giannini,
             G and Giglietto, N and Grassi, M et al.},
   Title = {Relevance of the hadronic interaction model in the
             interpretation of multiple muon data as detected with the
             MACRO experiment},
   Journal = {Nuclear Physics, Section B: Proceedings Supplements},
   Volume = {75},
   Number = {1-2},
   Pages = {265-278},
   Year = {1999},
   ISSN = {0920-5632},
   Abstract = {With the aim of discussing the effect of the possible
             sources of systematic uncertainties in simulation models,
             the analysis of multiple muon events from the MACRO
             experiment at Gran Sasso is reviewed. In particular, the
             predictions from different currently available hadronic
             interaction models are compared.},
   Key = {Ambrosio99b}
}

@booklet{Fukuda99,
   Author = {Fukuda, Y and Ishihara, K and Itow, Y and Kajita, T and Kameda, J and Kasuga, S and Kobayashi, K and Kobayashi, Y and Koshio, Y and Miura, M and Nakahata, M and Nakayama, S and Obayashi, Y and Okada, A and Okumura, K and Sakurai, N and Shiozawa, M and Suzuki, Y and Takeuchi, H and Takeuchi,
             Y and Totsuka, Y and Yamada, S and Earl, M and Habig, A and Kearns, E and Messier, MD and Scholberg, K and Stone, JL and Sulak, LR and Walter, CW and Goldhaber, M and Barszczak, T and Casper, D and Gajewski, W and Kropp,
             WR and Mine, S and Price, LR and Smy, M and Sobel, HW and Vagins, MR and Ganezer, KS and Keig, WE et al.},
   Title = {Neutrino-induced upward stopping muons in
             Super-Kamiokande},
   Journal = {Physics Letters B},
   Volume = {467},
   Number = {3-4},
   Pages = {185-193},
   Year = {1999},
   ISSN = {0370-2693},
   Abstract = {A total of 137 upward stopping muons of minimum energy 1.6
             GeV are observed by Super-Kamiokande during 516 detector
             live days. The measured muon flux is 0.39 ± 0.04(stat.) ±
             0.02(syst.) × 10-13 cm-2s-1sr-1 compared to an expected
             flux of 0.73 ± 0.16(theo.) × 10-13 cm-2s-1sr-1. Using our
             previously-published measurement of the upward through-going
             muon flux, we calculate the stopping/through-going flux
             ratio ℛ, which has less theoretical uncertainty. The
             measured value of ℛ = 0.22 ± 0.02(stat.) ± 0.01(syst.)
             is significantly smaller than the value 0.37-0.04+0.05(theo.)
             expected using the best theoretical information (the
             probability that the measured ℛ is a statistical
             fluctuation below the expected value is 0.39%). A
             simultaneous fitting to zenith angle distributions of upward
             stopping and through-going muons gives a result which is
             consistent with the hypothesis of neutrino oscillations with
             the parameters sin22θ &gt; 0.7 and 1.5 × 10-3 &lt; Δm2
             &lt; 1.5 × 10-2 eV2 at 90% confidence level, providing a
             confirmation of the observation of neutrino oscillations by
             Super-Kamiokande using the contained atmospheric neutrino
             events. © 1999 Published by Elsevier Science B.V. All
             rights reserved.},
   Key = {Fukuda99}
}

@article{fds304626,
   Author = {Ambrosio, M and Antolini, R and Aramo, C and Auriemma, G and Baldini, A and Barbarino, GC and Barish, BC and Battistoni, G and Bellotti, R and Bemporad, C and Bernardini, P and Bilokon, H and Bisi, V and Bloise, C and Bower, C and Bussino, S and Cafagna, F and Calicchio, M and Campana, D and Carboni, M and Castellano, M and Cecchini, S and Cei, F and Chiarella,
             V and Choudhary, BC and Coutu, S and Benedictis, LD and Cataldo, GD and Dekhissi, H and Marzo, CD and Mitri, ID and Derkaoui, J and Vincenzi,
             MD and Credico, AD and Erriquez, O and Favuzzi, C and Forti, C and Fusco,
             P and Giacomelli, G and Giannini, G et al.},
   Title = {Observation of the shadowing of cosmic rays by the Moon
             using a deep underground detector},
   Journal = {Physical Review D - Particles, Fields, Gravitation and
             Cosmology},
   Volume = {59},
   Number = {1},
   Pages = {1-7},
   Year = {1999},
   Abstract = {Using data collected by the MACRO experiment during the
             years 1989-1996, we show evidence for the shadow of the Moon
             in the underground cosmic ray flux with a significance of
             3.6σ. This detection of the shadowing effect is the first
             by an underground detector. A maximum-likelihood analysis is
             used to determine that the angular resolution of the
             apparatus is 0.9°±0.3°. These results demonstrate MACRO'S
             capabilities as a muon telescope by confirming its absolute
             pointing ability and quantifying its angular resolution.
             ©1998 The American Physical Society.},
   Key = {fds304626}
}

@article{fds304628,
   Author = {Ambrosio, M and Antolini, R and Aramo, C and Auriemma, G and Baldini, A and Barbarino, GC and Barish, BC and Battistoni, G and Bellotti, R and Bemporad, C and Bernardini, E and Bernardini, P and Bilokon, H and Bisi,
             V and Bloise, C and Bower, C and Bussino, S and Cafagna, F and Calicchio,
             M and Campana, D and Carboni, M and Castellano, M and Cecchini, S and Cei,
             F and Chiarella, V and Choudhary, BC and Coutu, S and Benedictis, LD and Cataldo, GD and Dekhissi, H and Marzo, CD and Mitri, ID and Derkaoui, J and Vincenzi, MD and Credico, AD and Diehl, E and Erriquez, O and Favuzzi,
             C and Forti, C and Fusco, P et al.},
   Title = {Limits on dark matter WIMPs using upward-going muons in the
             MACRO detector},
   Journal = {Physical Review D - Particles, Fields, Gravitation and
             Cosmology},
   Volume = {60},
   Number = {8},
   Pages = {1-10},
   Year = {1999},
   Abstract = {We perform an indirect search for weakly interacting massive
             particles (WIMPs) using the MACRO detector to look for
             neutrino-induced upward-going muons resulting from the
             annihilation of WIMPs trapped in the Sun and Earth. The
             search is conducted in various angular cones centered on the
             Sun and Earth to accommodate a range of WIMP masses. No
             significant excess over the background from atmospheric
             neutrinos is seen. We set experimental flux limits on the
             upward-going muon fluxes from the Sun and the Earth. These
             limits are used to constrain neutralino particle parameters
             from supersymmetric theory, including those suggested by
             recent results from DAMA-NaI. ©1999 The American Physical
             Society.},
   Key = {fds304628}
}

@article{fds304627,
   Author = {Ambrosio, M and Antolini, R and Aramo, C and Auriemma, G and Baldini, A and Barbarino, GC and Barish, BC and Battistoni, G and Bellotti, R and Bemporad, C and Bernardini, E and Bernardini, P and Bilokon, H and Bisi,
             V and Bloise, C and Bower, C and Bussino, S and Cafagna, F and Calicchio,
             M and Campana, D and Carboni, M and Castellano, M and Cecchini, S and Cei,
             F and Chiarella, V and Choudhary, BC and Coutu, S and Cataldo, GD and Dekhissi, H and Marzo, CD and Mitri, ID and Derkaoui, J and Vincenzi,
             MD and Credico, AD and Erriquez, O and Favuzzi, C and Forti, C and Fusco,
             P and Giacomelli, G and Giannini, G et al.},
   Title = {High statistics measurement of the underground muon pair
             separation at Gran Sasso},
   Journal = {Physical Review D - Particles, Fields, Gravitation and
             Cosmology},
   Volume = {60},
   Number = {3},
   Pages = {1-13},
   Year = {1999},
   Key = {fds304627}
}

@booklet{Fukuda98,
   Author = {Fukuda, Y and Hayakawa, T and Ichihara, E and Inoue, K and Ishihara, K and Ishino, H and Itow, Y and Kajita, T and Kameda, J and Kasuga, S and Kobayashi, K and Kobayashi, Y and Koshio, Y and Martens, K and Miura, M and Nakahata, M and Nakayama, S and Okada, A and Oketa, M and Okumura, K and Ota, M and Sakurai, N and Shiozawa, M and Suzuki, Y and Takeuchi, Y and Totsuka, Y and Yamada, S and Earl, M and Habig, A and Hong, JT and Kearns,
             E and Kim, SB and Masuzawa, M and Messier, MD and Scholberg, K and Stone,
             JL and Sulak, LR and Walter, CW and Goldhaber, M and Barszczak, T and Gajewski, W and Halverson, PG and Hsu, J et al.},
   Title = {Measurements of the solar neutrino flux from
             super-Kamiokande's first 300 days (vol 81, pg 1158,
             1998)},
   Journal = {Physical Review Letters},
   Volume = {81},
   Number = {19},
   Pages = {4279-4279},
   Year = {1998},
   Month = {November},
   ISSN = {0031-9007},
   url = {http://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcApp=PARTNER_APP&SrcAuth=LinksAMR&KeyUT=WOS:000077011000068&DestLinkType=FullRecord&DestApp=ALL_WOS&UsrCustomerID=47d3190e77e5a3a53558812f597b0b92},
   Doi = {10.1103/PhysRevLett.81.4279},
   Key = {Fukuda98}
}

@booklet{Fukuda98d,
   Author = {Fukuda, Y and Hayakawa, T and Ichihara, E and Inoue, K and Ishihara, K and Ishino, H and Itow, Y and Kajita, T and Kameda, J and Kasuga, S and Kobayashi, K and Kobayashi, Y and Koshio, Y and Martens, K and Miura, M and Nakahata, M and Nakayama, S and Okada, A and Oketa, M and Okumura, K and Ota, M and Sakurai, N and Shiozawa, M and Suzuki, Y and Takeuchi, Y and Totsuka, Y and Yamada, S and Earl, M and Habig, A and Hong, JT and Kearns,
             E and Kim, SB and Masuzawa, M and Messier, MD and Scholberg, K and Stone,
             JL and Sulak, LR and Walter, CW and Goldhaber, M and Barszczak, T and Gajewski, W and Halverson, PG and Hsu, J et al.},
   Title = {Measurement of a small atmospheric nu(mu)/nu(e)
             ratio},
   Journal = {Physics Letters B},
   Volume = {433},
   Number = {1-2},
   Pages = {9-18},
   Year = {1998},
   Month = {August},
   ISSN = {0370-2693},
   url = {http://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcApp=PARTNER_APP&SrcAuth=LinksAMR&KeyUT=WOS:000075193300002&DestLinkType=FullRecord&DestApp=ALL_WOS&UsrCustomerID=47d3190e77e5a3a53558812f597b0b92},
   Doi = {10.1016/S0370-2693(98)00476-6},
   Key = {Fukuda98d}
}

@article{fds326732,
   Author = {Astbury, A and Aubert, B and Augé, E and Baisin, L and Barreiro, F and Battistoni, G and Bazan, A and Baze, JM and Beaudoin, G and Beaugiraud,
             B and Berset, JC and Boniface, J and Boos, E and Breton, D and Camin, DV and Canton, B and Cavalli, D and Chase, R and Chekhtman, A and Chevalley,
             JL and Chmeissani, M and Chollet, JC and Citterio, M and Colas, J and Collot, J and Costa, G and Cousinou, MC and Cozzi, L and Dargent, P and David, J and Davis, RA and Delagnes, E and de LaTaille, C and Del Peso,
             J and Depommier, P and de Saintignon, P and Dinkespiller, B and Eek, LO and Etienne, F and Eynard, G et al.},
   Title = {Test beam results of a stereo preshower integrated in the
             liquid argon accordion calorimeter},
   Journal = {Nuclear Instruments and Methods in Physics Research Section
             A: Accelerators, Spectrometers, Detectors and Associated
             Equipment},
   Volume = {411},
   Number = {2-3},
   Pages = {313-329},
   Year = {1998},
   Month = {July},
   url = {http://dx.doi.org/10.1016/S0168-9002(98)00342-8},
   Doi = {10.1016/S0168-9002(98)00342-8},
   Key = {fds326732}
}

@article{fds248725,
   Author = {Giglietto, N and Ambrosio, M and Antolini, R and Auriemma, G and Baker,
             R and Baldini, A and Barbarino, GC and Barish, BC and Battistoni, G and Bellotti, R and Bemporad, C and Bernardini, P and Bilokon, H and Bisi,
             V and Bloise, C and Bosio, T and Bower, C and Bussino, S and Cafagna, F and Calicchio, M and Campana, D and Carboni, M and Castellano, M and Cecchini, S and Cei, F and Chiarella, V and Corona, A and Coutu, S and Benedictis, LD and Cataldo, GD and Dekhissi, H and Marzo, CD and Mitri,
             ID and Vincenzi, MD and Credico, AD and Erriquez, O and Fantini, R and Favuzzi, C and Forti, C and Fusco, P et al.},
   Title = {Performance of the MACRO detector at Gran Sasso: Moon shadow
             and seasonal variations},
   Journal = {Nuclear Physics, Section B: Proceedings Supplements},
   Volume = {61},
   Number = {3 SUPPL.},
   Pages = {180-184},
   Year = {1998},
   ISSN = {0920-5632},
   Abstract = {The MACRO underground detector at Gran Sasso has recorded
             about 30 million muon events in the period 1989-1995. We
             have analyzed these data to look for time variations and to
             study the pointing capabilities of the apparatus in the
             search for astrophysical point sources. We have observed a
             3% seasonal variation of the high energy muon rate, due to
             atmospheric temperature variations, in agreement with
             theoretical predictions. We report also the detection of the
             moon shadowing effect with a statistical significance of 3.7
             σ. The results obtained straighten the possibility that a
             "muon astronomy" using underground experiments is
             possible.},
   Key = {fds248725}
}

@article{fds248726,
   Author = {Fukuda, Y and Hayakawa, T and Ichihara, E and Inoue, K and Ishihara, K and Ishino, H and Itow, Y and Kajita, T and Kameda, J and Kasuga, S and Kobayashi, K and Kobayashi, Y and Koshio, Y and Martens, K and Miura, M and Nakahata, M and Nakayama, S and Okada, A and Oketa, M and Okumura, K and Ota, M and Sakurai, N and Shiozawa, M and Suzuki, Y and Takeuchi, Y and Totsuka, Y and Yamada, S and Earl, M and Habig, A and Hong, JT and Kearns,
             E and Kim, SB and Masuzawa, M and Messier, MD and Scholberg, K and Stone,
             JL and Sulak, LR and Walter, CW and Goldhaber, M and Barszczak, T and Gajewski, W and Halverson, PG and Hsu, J et al.},
   Title = {Measurement of a small atmospheric νμe
             ratio},
   Journal = {Physics Letters B},
   Volume = {433},
   Number = {1-2},
   Pages = {9-18},
   Year = {1998},
   ISSN = {0370-2693},
   Abstract = {From an exposure of 25.5 kiloton-years of the
             Super-Kamiokande detector, 900 muon-like and 983
             electron-like single-ring atmospheric neutrino interactions
             were detected with momentum pe &gt; 100 MeV/c, pμ &gt; 200
             MeV/c, and with visible energy less than 1.33 GeV. Using a
             detailed Monte Carlo simulation, the ratio
             (μ/e)DATA/(μ/e)MC was measured to be 0.61 ± 0.03(stat.)
             ± 0.05(sys.), consistent with previous results from the
             Kamiokande, IMB and Soudan-2 experiments, and smaller than
             expected from theoretical models of atmospheric neutrino
             production. © 1998 Published by Elsevier Science B.V. All
             rights reserved.},
   Key = {fds248726}
}

@booklet{Ambrosio98b,
   Author = {Ambrosio, M and Antolini, R and Auriemma, G and Baker, R and Baldini, A and Barbarino, GC and Barish, BC and Battistoni, G and Bellotti, R and Bemporad, C and Bernardini, P and Bilokon, H and Bisi, V and Bloise, C and Bower, C and Bussino, S and Cafagna, F and Calicchio, M and Campana, D and Carboni, M and Castellano, M and Cecchini, S and Cei, F and Celio, P and Chiarella, V and Corona, A and Coutu, S and Benedictis, LD and Cataldo,
             GD and Dekhissi, H and Marzo, CD and Mitri, ID and Vincenzi, MD and Credico, AD and Erriquez, O and Favuzzi, C and Forti, C and Fusco, P and Giacomelli, G and Giannini, G et al.},
   Title = {Real time supernova neutrino burst detection with
             MACRO},
   Journal = {Astroparticle Physics},
   Volume = {8},
   Number = {3},
   Pages = {123-133},
   Year = {1998},
   ISSN = {0927-6505},
   Abstract = {The MACRO experiment has been running as a supernova
             neutrino detector since 1989 and is sensitive to the whole
             galaxy since the beginning of 1992. A galactic supernova
             would produce some hundreds of v̄e events in the detector.
             We describe our stellar gravitational collapse online
             monitors and alarm system, and present the results of a
             search for neutrino bursts from supernovae during a period
             of 1.5 yr. © 1998 Elsevier Science B.V.},
   Key = {Ambrosio98b}
}

@booklet{Fukuda98b,
   Author = {Fukuda, Y and Hayakawa, T and Ichihara, E and Inoue, K and Ishihara, K and Ishino, H and Itow, Y and Kajita, T and Kameda, J and Kasuga, S and Kobayashi, K and Kobayashi, Y and Koshio, Y and Miura, M and Nakahata,
             M and Nakayama, S and Okada, A and Okumura, K and Sakurai, N and Shiozawa,
             M and Suzuki, Y and Takeuchi, Y and Totsuka, Y and Yamada, S and Earl, M and Habig, A and Kearns, E and Messier, MD and Scholberg, K and Stone, JL and Sulak, LR and Walter, CW and Goldhaber, M and Barszczxak, T and Casper,
             D and Gajewski, W and Halverson, PG and Hsu, J and Kropp, WR and Price, LR and Reines, F and Smy, M and Sobel, HW et al.},
   Title = {Evidence for oscillation of atmospheric neutrinos},
   Journal = {Physical Review Letters},
   Volume = {81},
   Number = {8},
   Pages = {1562-1567},
   Year = {1998},
   ISSN = {0031-9007},
   Abstract = {We present an analysis of atmospheric neutrino data from a
             33.0 kton yr (535-day) exposure of the Super-Kamiokande
             detector. The data exhibit a zenith angle dependent deficit
             of muon neutrinos which is inconsistent with expectations
             based on calculations of the atmospheric neutrino flux.
             Experimental biases and uncertainties in the prediction of
             neutrino fluxes and cross sections are unable to explain our
             observation. The data are consistent, however, with
             two-flavor νμ ↔ ντ oscillations with sin2 2θ &gt;
             0.82 and 5 × 10-4 &lt; Δm2 &lt; 6 × 10-3 eV2 at 90%
             confidence level.},
   Key = {Fukuda98b}
}

@booklet{Shiozawa98,
   Author = {Shiozawa, M and Viren, B and Fukuda, Y and Hayakawa, T and Ichihara, E and Inoue, K and Ishihara, K and Ishino, H and Itow, Y and Kajita, T and Kameda, J and Kasuga, S and Kobayashi, K and Kobayashi, Y and Koshio, Y and Miura, M and Nakahata, M and Nakayama, S and Okada, A and Oketa, M and Okumura, K and Ota, M and Sakurai, N and Suzuki, Y and Takeuchi, Y and Totsuka, Y and Yamada, S and Earl, M and Habig, A and Kearns, E and Messier, MD and Scholberg, K and Stone, JL and Sulak, LR and Walter, CW and Goldhaber, M and Barszczak, T and Gajewski, W and Halverson, PG and Hsu,
             J and Kropp, WR and Price, LR and Reines, F et al.},
   Title = {Search for proton decay via p → e+
             π0 in a large water cherenkov
             detector},
   Journal = {Physical Review Letters},
   Volume = {81},
   Number = {16},
   Pages = {3319-3323},
   Year = {1998},
   ISSN = {0031-9007},
   Abstract = {We have searched for proton decay via p → e+ π0 using
             data from a 25.5 kton · yr exposure of the Super-Kamiokande
             detector. We find no candidate events with an expected
             background induced by atmospheric neutrinos of 0.1 events.
             From these data, we set a lower limit on the partial
             lifetime of the proton τ/Bp→e+π0 to be 1.6 × 1033 years
             at a 90% confidence level.},
   Key = {Shiozawa98}
}

@booklet{Fukuda98a,
   Author = {Fukuda, Y and Hayakawa, T and Ichihara, E and Inoue, K and Ishihara, K and Ishino, H and Itow, Y and Kajita, T and Kameda, J and Kasuga, S and Kobayashi, K and Kobayashi, Y and Koshio, Y and Martens, K and Miura, M and Nakahata, M and Nakayama, S and Okada, A and Oketa, M and Okumura, K and Ota, M and Sakurai, N and Shiozawa, M and Suzuki, Y and Takeuchi, Y and Totsuka, Y and Yamada, S and Earl, M and Habig, A and Kearns, E and Kim,
             SB and Messier, MD and Scholberg, K and Stone, JL and Sulak, LR and Walter,
             CW and Goldhaber, M and Barszczak, T and Gajewski, W and Halverson, PG and Hsu, J and Kropp, WR and Price, LR et al.},
   Title = {Study of the atmospheric neutrino flux in the multi-GeV
             energy range},
   Journal = {Physics Letters B},
   Volume = {436},
   Number = {1-2},
   Pages = {33-41},
   Year = {1998},
   ISSN = {0370-2693},
   Abstract = {The flavor ratio of the atmospheric neutrino flux and its
             zenith angle dependence have been studied in the multi-GeV
             energy range using an exposure of 25.5 kiloton-years of the
             Super-Kamiokande detector. By comparing the data to a
             detailed Monte Carlo simulation, the ratio
             (μ/e)DATA/(μ/e)MC was measured to be 0.66 ± 0.06(stat.)
             ± 0.08(sys.). In addition, a strong distortion in the shape
             of the μ-like event zenith angle distribution was observed.
             The ratio of the number of upward to downward μ-like events
             was found to be 0.52+0.070.06(stat.) ± 0.01(sys.), with an
             expected value of 0.98 ± 0.03(stat.) ± 0.02(sys.), while
             the same ratio for the e-like events was consistent with
             unity. © 1998 Elsevier Science B.V. All rights
             reserved.},
   Key = {Fukuda98a}
}

@booklet{Ambrosio98a,
   Author = {Ambrosio, M and Antolini, R and Aramo, C and Auriemma, G and Baldini, A and Barbarino, GC and Barish, BC and Battistoni, G and Bellotti, R and Bemporad, C and Bernardini, P and Bilokon, H and Bisi, V and Bloise, C and Bower, C and Bussino, S and Cafagna, F and Calicchio, M and Campana, D and Carboni, M and Castellano, M and Cecchini, S and Cei, F and Chiarella,
             V and Coutu, S and Cunti, G and Benedictis, LD and Cataldo, GD and Dekhissi, H and Marzo, CD and Mitri, ID and Vincenzi, MD and Credico,
             AD and Erriquez, O and Favuzzi, C and Forti, C and Fusco, P and Giacomelli,
             G and Giannini, G and Giglietto, N et al.},
   Title = {The observation of up-going charged particles produced by
             high energy muons in underground detectors},
   Journal = {Astroparticle Physics},
   Volume = {9},
   Number = {2},
   Pages = {105-117},
   Year = {1998},
   ISSN = {0927-6505},
   Abstract = {An experimental study of the production of up-going charged
             particles in inelastic interactions of down-going
             underground muons is reported, using data obtained from the
             MACRO detector at the Gran Sasso Laboratory. In a sample of
             12.2 x 106 single muons, corresponding to a detector
             lifetime of 1.55y, 243 events are observed having an
             up-going particle associated with a down-going muon. These
             events are analysed to determine the range and emission
             angle distributions of the up-going particle, corrected for
             detection and reconstruction efficiency. Measurements of the
             muon neutrino flux by underground detectors are often based
             on the observation of through-going and stopping muons
             produced in νμ interactions in the rock below the
             detector. Up-going particles produced by an undetected
             down-going muon are a potential background source in these
             measurements. The implications of this background for
             neutrino studies using MACRO are discussed. © 1998 Elsevier
             Science B.V.},
   Key = {Ambrosio98a}
}

@booklet{Ambrosio98,
   Author = {Ambrosio, M and Antolini, R and Aramo, C and Auriemma, G and Baldini, A and Barbarino, GC and Barish, BC and Battistoni, G and Bellotti, R and Bemporad, C and Bernardini, P and Bilokon, H and Bisi, V and Bloise, C and Bower, C and Bussino, S and Cafagna, F and Calicchio, M and Campana, D and Carboni, M and Castellano, M and Cecchini, S and Cei, F and Chiarella,
             V and Choudhary, BC and Coutu, S and Benedictis, LD and Cataldo, GD and Dekhissi, H and Marzo, CD and Mitri, ID and Derkaoui, J and Vincenzi,
             MD and Credico, AD and Erriquez, O and Favuzzi, C and Forti, C and Fusco,
             P and Giacomelli, G and Giannini, G et al.},
   Title = {Measurement of the atmospheric neutrino-induced upgoing muon
             flux using MACRO},
   Journal = {Physics Letters B},
   Volume = {434},
   Number = {3-4},
   Pages = {451-457},
   Year = {1998},
   ISSN = {0370-2693},
   Abstract = {We present a measurement of the flux of neutrino-induced
             upgoing muons (&lt; Eν &gt; ∼ 100 GeV) using the MACRO
             detector. The ratio of the number of observed to expected
             events integrated over all zenith angles is 0.74 ± 0.036
             (stat) ± 0.046 (systematic) ± 0.13 (theoretical). The
             observed zenith distribution for -1.0 ≤ cosθ ≤ -0.1
             does not fit well with the no oscillation expectation,
             giving a maximum probability for χ2 of 0.1%. The acceptance
             of the detector has been extensively studied using downgoing
             muons, independent analyses and Monte Carlo simulations. The
             other systematic uncertainties cannot be the source of the
             discrepancies between the data and expectations. We have
             investigated whether the observed number of events and the
             shape of the zenith distribution can be explained by a
             neutrino oscillation hypothesis. Fitting either the flux or
             zenith distribution independently yields mixing parameters
             of sin22θ = 1.0 and Δm2 of a few times 10-3 eV2. However,
             the observed zenith distribution does not fit well with any
             expectations, giving a maximum probability for χ2 of 5% for
             the best oscillation hypothesis, and the combined
             probability for the shape and number of events is 17%. We
             conclude that these data favor a neutrino oscillation
             hypothesis, but with unexplained structure in the zenith
             distribution not easily explained by either the statistics
             or systematics of the experiment. © 1998 Published by
             Elsevier Science B.V. All rights reserved.},
   Key = {Ambrosio98}
}

@booklet{Fukuda98c,
   Author = {Fukuda, Y and Hayakawa, T and Ichihara, E and Inoue, K and Ishihara, K and Ishino, H and Itow, Y and Kajita, T and Kameda, J and Kasuga, S and Kobayashi, K and Kobayashi, Y and Koshio, Y and Martens, K and Miura, M and Nakahata, M and Nakayama, S and Okada, A and Oketa, M and Okumura, K and Ota, M and Sakurai, N and Shiozawa, M and Suzuki, Y and Takeuchi, Y and Totsuka, Y and Yamada, S and Earl, M and Habig, A and Hong, JT and Kearns,
             E and Kim, SB and Masuzawa, M and Messier, MD and Scholberg, K and Stone,
             JL and Sulak, LR and Walter, CW and Goldhaber, M and Barszczak, T and Gajewski, W and Halverson, PG and Hsu, J et al.},
   Title = {Measurements of the solar neutrino flux from
             Super-Kamiokande's first 300 days},
   Journal = {Physical Review Letters},
   Volume = {81},
   Number = {6},
   Pages = {1158-1162},
   Year = {1998},
   ISSN = {0031-9007},
   Abstract = {The first results of the solar neutrino flux measurement
             from Super-Kamiokande are presented. The results shown here
             are obtained from data taken between 31 May 1996, and 23
             June 1997. Using our measurement of recoil electrons with
             energies above 6.5 MeV, we infer the total flux of 8B solar
             neutrinos to be 2.42 ± 0.06(stat)-0.07+0.10(syst) ×
             106cm-2 s-1. This result is consistent with the Kamiokande
             measurement and is 36% of the flux predicted by the BP95
             solar model. The flux is also measured in 1.5 month subsets
             and shown to be consistent with a constant
             rate.},
   Key = {Fukuda98c}
}

@booklet{Ambrosio97e,
   Author = {Ambrosio, M and Antolini, R and Auriemma, G and Baker, R and Baldini, A and Barbarino, GC and Barish, BC and Battistoni, G and Bellotti, R and Bemporad, C and Bernardini, P and Bilokon, H and Bisi, V and Bloise, C and Bosio, T and Bower, C and Bussino, S and Cafagna, R and Calicchio, M and Campana, D and Carboni, M and Castellano, M and Cecchini, S and Cei, F and Chiarella, V and Corona, A and Coutu, S and DeCataldo, G and Dekhissi,
             H and DeMarzo, C and De Mitri and I and DeVincenzi, M and DiCredico, A and Erriquez, O and Fantini, R and Favuzzi, C and Forti, C and Fusco, P and Giacomelli, G and Giannini, G et al.},
   Title = {The performance of MACRO liquid scintillator in the search
             for magnetic monopoles with 10(-3)