Publications of Kate Scholberg    :chronological  alphabetical  combined listing:

%% Books   
@book{fds221119,
   Author = {K. Scholberg},
   Title = {Large Underground Detectors for Proton Decay and Neutrino
             Physics},
   Booktitle = {100 Years of Subatomic Physics},
   Publisher = {World Scientific},
   Editor = {Ernest M. Henley and Stephen D. Ellis},
   Year = {2013},
   Month = {August},
   Key = {fds221119}
}

@book{fds199353,
   Author = {Various authors and edited by I. Irastorza and K. Scholberg and P.
             Colas and I. Giomataris},
   Title = {Proceedings, 5th Symposium on Large TPCs for low energy rare
             event detection and Workshop on Neutrinos from
             Supernovae},
   Year = {2011},
   Key = {fds199353}
}

@book{fds30142,
   Author = {Various authors},
   Title = {Proceedings of SpacePart 2003},
   Editor = {R. Battiston and E. Katsavounidis and M. Salamon and K.
             Scholberg},
   Year = {2004},
   Key = {fds30142}
}


%% Papers Published   
@article{fds330359,
   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 neutrino and antineutrino oscillations by the
             T2K experiment including a new additional sample of
             veinteractions at the far detector},
   Journal = {Physical Review D},
   Volume = {96},
   Number = {9},
   Year = {2017},
   Month = {November},
   url = {http://dx.doi.org/10.1103/PhysRevD.96.092006},
   Abstract = {The T2K experiment reports an updated analysis of neutrino
             and antineutrino oscillations in appearance and
             disappearance channels. Asample of electron neutrino
             candidates at Super-Kamiokande in which a pion decay has
             been tagged is added to the four single-ring samples used in
             previous T2K oscillation analyses. Through combined analyses
             of these five samples, simultaneous measurements of four
             oscillation parameters, j?m2 32j, sin2 ?23, sin2 ?13, and
             dCP and of the mass ordering are made. A set of studies of
             simulated data indicates that the sensitivity to the
             oscillation parameters is not limited by neutrino
             interaction model uncertainty. Multiple oscillation analyses
             are performed, and frequentist and Bayesian intervals are
             presented for combinations of the oscillation parameters
             with and without the inclusion of reactor constraints on
             sin2 ?13.When combined with reactor measurements, the
             hypothesis of CP conservation (dCP 0 or p) is excluded at
             90% confidence level. The 90% confidence region for dCP is
             -2.95;-0.44(-1.47;-1.27) for normal (inverted) ordering. The
             central values and 68% confidence intervals for the other
             oscillation parameters for normal (inverted) ordering are
             ?m2 32 2.540.082.510.08 10-3 eV2=c4 and sin2?23 0.55+0.05
             -0.09 (0.55+0.05 -0.08 ), compatible with maximal mixing. In
             the Bayesian analysis, the data weakly prefer normal
             ordering (Bayes factor 3.7) and the upper octant for sin2
             ?23 (Bayes factor 2.4).},
   Doi = {10.1103/PhysRevD.96.092006},
   Key = {fds330359}
}

@article{fds329303,
   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 = {fds329303}
}

@article{fds328274,
   Author = {Akimov, D and Albert, JB and An, P and Awe, C and Barbeau, PS and Becker,
             B and Belov, V and Brown, A and Bolozdynya, A and Cabrera-Palmer, B and Cervantes, M and Collar, JI and Cooper, RJ and Cooper, RL and Cuesta, C and Dean, DJ and Detwiler, JA and Eberhardt, A and Efremenko, Y and Elliott,
             SR and Erkela, EM and Fabris, L and Febbraro, M and Fields, NE and Fox, W and Fu, Z and Galindo-Uribarri, A and Green, MP and Hai, M and Heath, MR and Hedges, S and Hornback, D and Hossbach, TW and Iverson, EB and Kaufman,
             LJ and Ki, S and Klein, SR and Khromov, A and Konovalov, A and Kremer, M and Kumpan, A and Leadbetter, C et al.},
   Title = {Observation of coherent elastic neutrino-nucleus
             scattering.},
   Journal = {Science},
   Volume = {357},
   Number = {6356},
   Pages = {1123-1126},
   Year = {2017},
   Month = {September},
   url = {http://dx.doi.org/10.1126/science.aao0990},
   Abstract = {The coherent elastic scattering of neutrinos off nuclei has
             eluded detection for four decades, even though its predicted
             cross section is by far the largest of all low-energy
             neutrino couplings. This mode of interaction offers new
             opportunities to study neutrino properties and leads to a
             miniaturization of detector size, with potential
             technological applications. We observed this process at a
             6.7σ confidence level, using a low-background,
             14.6-kilogram CsI[Na] scintillator exposed to the neutrino
             emissions from the Spallation Neutron Source at Oak Ridge
             National Laboratory. Characteristic signatures in energy and
             time, predicted by the standard model for this process, were
             observed in high signal-to-background conditions. Improved
             constraints on nonstandard neutrino interactions with quarks
             are derived from this initial data set.},
   Doi = {10.1126/science.aao0990},
   Key = {fds328274}
}

@article{fds328440,
   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 = {fds328440}
}

@article{fds328441,
   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 = {fds328441}
}

@article{fds327378,
   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 = {fds327378}
}

@article{fds326201,
   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 = {fds326201}
}

@article{fds327637,
   Author = {Wright, WP and Kneller, JP and Ohlmann, ST and Röpke, FK and Scholberg,
             K and Seitenzahl, IR},
   Title = {Neutrinos from type Ia supernovae: The gravitationally
             confined detonation scenario},
   Journal = {Physical Review D},
   Volume = {95},
   Number = {4},
   Year = {2017},
   Month = {February},
   url = {http://dx.doi.org/10.1103/PhysRevD.95.043006},
   Doi = {10.1103/PhysRevD.95.043006},
   Key = {fds327637}
}

@article{fds325022,
   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 = {fds325022}
}

@article{fds327012,
   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 = {fds327012}
}

@article{fds325970,
   Author = {Akimov, D and Albert, JB and Awe, C and Barbeau, PS and Becker, B and Belov, V and Bolozdynya, A and Burenkov, A and Cabrera-Palmer, B and Cervantes, M and Collar, JI and Cooper, RJ and Cooper, RL and Cuesta, C and Dean, D and del Valle Coello and M and Detwiler, J and Dolgolenko, AG and D’Onofrio, M and Eberhardt, A and Efremenko, Y and Elliott, SR and Etenko, A and Fabris, L and Fields, N and Fox, W and Galindo-Uribarri,
             A and Green, M and Heath, M and Hedges, S and Iverson, EB and Kaufman, LJ and Klein, SR and Khromov, A and Konovalov, A and Kovalenko, A and Kumpan,
             A and Li, L and Lu, W and Mann, K et al.},
   Title = {COHERENT Experiment: current status},
   Journal = {Journal of Physics},
   Volume = {798},
   Pages = {012213-012213},
   Year = {2017},
   Month = {January},
   url = {http://dx.doi.org/10.1088/1742-6596/798/1/012213},
   Doi = {10.1088/1742-6596/798/1/012213},
   Key = {fds325970}
}

@article{fds320671,
   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 = {fds320671}
}

@article{fds318462,
   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 = {fds318462}
}

@article{fds326485,
   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 = {fds326485}
}

@article{fds318463,
   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 = {fds318463}
}

@article{fds318464,
   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 = {fds318464}
}

@article{fds324045,
   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 = {fds324045}
}

@article{fds318465,
   Author = {Wright, WP and Nagaraj, G and Kneller, JP and Scholberg, K and Seitenzahl, IR},
   Title = {Neutrinos from type Ia supernovae: The deflagration-to-detonation
             transition scenario},
   Journal = {Physical Review D},
   Volume = {94},
   Number = {2},
   Year = {2016},
   Month = {July},
   url = {http://dx.doi.org/10.1103/PhysRevD.94.025026},
   Doi = {10.1103/PhysRevD.94.025026},
   Key = {fds318465}
}

@article{fds318466,
   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 = {fds318466}
}

@article{fds316012,
   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},
   ISSN = {0031-9007},
   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 = {fds316012}
}

@article{fds315558,
   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},
   ISSN = {2470-0010},
   url = {http://dx.doi.org/10.1103/PhysRevD.93.072002},
   Doi = {10.1103/PhysRevD.93.072002},
   Key = {fds315558}
}

@article{fds318467,
   Author = {Himmel, A and Scholberg, K},
   Title = {Supernova Neutrino Detection},
   Journal = {Nuclear and Particle Physics Proceedings},
   Volume = {273-275},
   Pages = {1897-1901},
   Year = {2016},
   Month = {April},
   url = {http://dx.doi.org/10.1016/j.nuclphysbps.2015.09.306},
   Doi = {10.1016/j.nuclphysbps.2015.09.306},
   Key = {fds318467}
}

@article{fds315555,
   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},
   ISSN = {2470-0010},
   url = {http://dx.doi.org/10.1103/PhysRevD.93.012004},
   Doi = {10.1103/PhysRevD.93.012004},
   Key = {fds315555}
}

@article{fds315556,
   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},
   ISSN = {2470-0010},
   url = {http://dx.doi.org/10.1103/PhysRevD.93.012006},
   Doi = {10.1103/PhysRevD.93.012006},
   Key = {fds315556}
}

@article{fds315557,
   Author = {Mirizzi, A and Tamborra, I and Janka, HT and Saviano, N and Scholberg,
             K and Bollig, R and Hüdepohl, L and Chakraborty,
             S},
   Title = {Supernova neutrinos: Production, oscillations and
             detection},
   Journal = {Rivista del Nuovo Cimento della Societa Italiana di
             Fisica},
   Volume = {39},
   Number = {1-2},
   Pages = {1-112},
   Year = {2016},
   Month = {January},
   ISSN = {0393-697X},
   url = {http://dx.doi.org/10.1393/ncr/i2016-10120-8},
   Abstract = {© 2015 Società Italiana di Fisica. Neutrinos play a
             crucial role in the collapse and explosion of massive stars,
             governing the infall dynamics of the stellar core,
             triggering and fueling the explosion and driving the cooling
             and deleptonization of the newly formed neutron star. Due to
             their role neutrinos carry information from the heart of the
             explosion and, due to their weakly interacting nature, offer
             the only direct probe of the dynamics and thermodynamics at
             the center of a supernova. In this paper, we review the
             present status of modelling the neutrino physics and signal
             formation in collapsing and exploding stars. We assess the
             capability of current and planned large underground neutrino
             detectors to yield faithful information of the time and
             flavor-dependent neutrino signal from a future Galactic
             supernova. We show how the observable neutrino burst would
             provide a benchmark for fundamental supernova physics with
             unprecedented richness of detail. Exploiting the treasure of
             the measured neutrino events requires a careful
             discrimination of source-generated properties from signal
             features that originate on the way to the detector. As for
             the latter, we discuss self-induced flavor conversions
             associated with neutrino-neutrino interactions that occur in
             the deepest stellar regions; matter effects that modify the
             pattern of flavor conversions in the dynamical stellar
             envelope; neutrino-oscillation signatures that result from
             structural features associated with the shock-wave
             propagation as well as turbulent mass motions in post-shock
             layers. Finally, we highlight our current understanding of
             the formation of the diffuse supernova neutrino background
             and we analyse the perspectives for a detection of this
             relic signal that integrates the contributions from all past
             core-collapse supernovae in the Universe.},
   Doi = {10.1393/ncr/i2016-10120-8},
   Key = {fds315557}
}

@article{fds315554,
   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},
   ISSN = {1550-7998},
   url = {http://dx.doi.org/10.1103/PhysRevD.92.112003},
   Doi = {10.1103/PhysRevD.92.112003},
   Key = {fds315554}
}

@article{fds315552,
   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},
   ISSN = {0031-9007},
   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 = {fds315552}
}

@article{fds248097,
   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},
   ISSN = {1550-7998},
   url = {http://dx.doi.org/10.1103/PhysRevD.91.112010},
   Doi = {10.1103/PhysRevD.91.112010},
   Key = {fds248097}
}

@article{fds248098,
   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},
   ISSN = {1550-7998},
   url = {http://dx.doi.org/10.1103/PhysRevD.91.112002},
   Doi = {10.1103/PhysRevD.91.112002},
   Key = {fds248098}
}

@article{fds315553,
   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 = {fds315553}
}

@article{fds315559,
   Author = {Scholberg, K},
   Title = {Coherent elastic neutrino-nucleus scattering},
   Journal = {Journal of Physics},
   Volume = {606},
   Pages = {012010-012010},
   Year = {2015},
   Month = {May},
   ISSN = {1742-6588},
   url = {http://dx.doi.org/10.1088/1742-6596/606/1/012010},
   Doi = {10.1088/1742-6596/606/1/012010},
   Key = {fds315559}
}

@article{fds315551,
   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},
   ISSN = {0031-9007},
   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 = {fds315551}
}

@article{fds248096,
   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 = {fds248096}
}

@article{fds248099,
   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 = {fds248099}
}

@article{fds303749,
   Author = {collaboration, S-K 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 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 et al.},
   Title = {Search for n-nbar oscillation in Super-Kamiokande},
   Journal = {Phys. Rev. D},
   Volume = {91},
   Number = {7},
   Pages = {072006},
   Year = {2015},
   Month = {April},
   url = {http://arxiv.org/abs/1109.4227v2},
   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 = {fds303749}
}

@article{fds248110,
   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://dx.doi.org/10.1016/j.astropartphys.2014.05.004},
   Doi = {10.1016/j.astropartphys.2014.05.004},
   Key = {fds248110}
}

@article{Barbeau:2014mla,
   Author = {Barbeau, PS and Collar, JI and Efremenko, Y and Scholberg,
             K},
   Title = {Comment on "Fitting the Annual Modulation in DAMA with
             Neutrons from Muons and Neutrinos"},
   Journal = {Physical Review Letters},
   Volume = {113},
   Number = {22},
   Pages = {229001},
   Year = {2014},
   Month = {November},
   ISSN = {0031-9007},
   url = {http://arxiv.org/pdf/1409.3185},
   Abstract = {A Comment on the Letter by J. H. Davis, Phys. Rev. Lett.
             113, 081302 (2014)PRLTAO0031-900710.1103/PhysRevLett.113.081302.},
   Doi = {10.1103/physrevlett.113.229001},
   Key = {Barbeau:2014mla}
}

@article{fds248107,
   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 = {fds248107}
}

@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{fds248105,
   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 = {fds248105}
}

@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{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},
   ISSN = {1674-1137},
   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{Litos:2014fxa,
   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 = {Litos:2014fxa}
}

@article{Brice:2013fwa,
   Author = {Brice, SJ and Cooper, RL and DeJongh, F and Empl, A and Garrison, LM and Hime, A and Hungerford, E and Kobilarcik, T and Loer, B and Mariani, C and Mocko, M and Muhrer, G and Pattie, R and Pavlovic, Z and Ramberg, E and Scholberg, K and Tayloe, R and Thornton, RT and Yoo, J and Young,
             A},
   Title = {A method for measuring coherent elastic neutrino-nucleus
             scattering at a far off-axis high-energy neutrino beam
             target},
   Journal = {Physical Review D - Particles, Fields, Gravitation, and
             Cosmology},
   Volume = {89},
   Number = {7},
   Pages = {072004},
   Year = {2014},
   Month = {April},
   ISSN = {1550-7998},
   url = {http://arxiv.org/pdf/1311.5958},
   Abstract = {http://arxiv.org/abs/1311.5958},
   Doi = {10.1103/PhysRevD.89.072004},
   Key = {Brice:2013fwa}
}

@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 = {Phys. Rev. Lett.},
   Volume = {112},
   Number = {9},
   Pages = {091805},
   Year = {2014},
   Month = {March},
   url = {http://arxiv.org/abs/1312.5176v3},
   Abstract = {We report an indication that the elastic scattering rate of
             solar $^8$B neutrinos with electrons in the Super-Kamiokande
             detector is larger when the neutrinos pass through the 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 $(-3.2\pm1.1(\text{stat})\pm0.5(\text{syst}))\%$,
             which deviates from zero by 2.7 $\sigma$. Since the elastic
             scattering process is mostly sensitive to electron-flavored
             solar neutrinos, a non-zero 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 $4\times10^{-5}$eV$^2\leq\Delta
             m^2_{21}\leq7\times10^{-5}$eV$^2$ and large mixing values of
             $\theta_{12}$, 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 Rodríguez, JC 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 = {Observation of Electron Neutrino Appearance in a Muon
             Neutrino Beam},
   Journal = {Phys. Rev. Lett.},
   Volume = {112},
   Number = {6},
   Pages = {061802},
   Year = {2014},
   Month = {February},
   url = {http://arxiv.org/abs/1311.4750v2},
   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 7.3$\sigma$ when compared
             to 4.92 $\pm$ 0.55 expected background events. In the PMNS
             mixing model, the electron neutrino appearance signal
             depends on several parameters including three mixing angles
             $\theta_{12}$, $\theta_{23}$, $\theta_{13}$, a mass
             difference $\Delta m^2_{32}$ and a CP violating phase
             $\delta_{\mathrm{CP}}$. In this neutrino oscillation
             scenario, assuming $|\Delta m^2_{32}| = 2.4 \times 10^{-3}$
             $\rm eV^2$, $\sin^2 \theta_{23} = 0.5$, and $\Delta m^2_{32}
             >0$ ($\Delta m^2_{32} <0$), a best-fit value of $\sin^2 2
             \theta_{13}$ = $0.140^{+0.038}_{-0.032}$
             ($0.170^{+0.045}_{-0.037}$) is obtained at
             $\delta_{\mathrm{CP}}=0$. When combining the result with the
             current best knowledge of oscillation parameters including
             the world average value of $\theta_{13}$ from reactor
             experiments, some values of $\delta_{\mathrm{CP}}$ are
             disfavored at the 90% CL.},
   Doi = {10.1103/PhysRevLett.112.061802},
   Key = {Abe:2013hdq}
}

@article{fds248111,
   Author = {Izatt, E and Scholberg, K and Kopper, R},
   Title = {Neutrino-KAVE: An immersive visualization and fitting tool
             for neutrino physics education},
   Journal = {Proceedings - IEEE Virtual Reality},
   Pages = {83-84},
   Year = {2014},
   Month = {January},
   url = {http://dx.doi.org/10.1109/VR.2014.6802062},
   Abstract = {Water Cherenkov neutrino detectors, like the existing
             Super-Kamiokande ('Super-K') and the planned
             Hyper-Kamiokande ('Hyper-K') detectors, are used to study
             neutrino particle physics. These detectors consist of large
             vessels holding many thousands of tons of water, as well as
             tens of thousands of photomultiplier tubes. Such detectors
             produce large and multi-layered datasets well-suited to
             immersive visualization and interaction. We have developed a
             novel virtual reality (VR) application called Neutrino-KAVE
             which functions as an visualization and data interaction
             application. Neutrino-KAVE displays the collocation of
             photon sensors and their color-coded data within a to-scale
             representation of the Super-K or Hyper-K detector, and
             provides a new visualization technique for neutrino
             interaction patterns. Neutrino-KAVE also provides both a
             mechanism for modifying aspects of the presented data set,
             and a user interface for system control of this multifaceted
             application. In this paper, we describe in detail our
             implementation and design choices. We also report on its use
             cases, initial reception, and future development. © 2014
             IEEE.},
   Doi = {10.1109/VR.2014.6802062},
   Key = {fds248111}
}

@article{fds248117,
   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 = {fds248117}
}

@article{Gilchriese:2014oka,
   Author = {Gilchriese, M.G. and Cushman, P. and Heeger, K. and Klein,
             J. and Scholberg, K. and others},
   Title = {Planning the Future of U.S. Particle Physics (Snowmass
             2013): Chapter 7: Underground Laboratory
             Capabilities},
   Year = {2014},
   url = {http://arxiv.org/pdf/1401.6115},
   Abstract = {http://arxiv.org/abs/1401.6115},
   Key = {Gilchriese:2014oka}
}

@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{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{Hewett:2014qja,
   Author = {Hewett, J.L. and Weerts, H. and Babu, K.S. and Butler, J. and Casey, B. and others},
   Title = {Planning the Future of U.S. Particle Physics (Snowmass
             2013): Chapter 2: Intensity Frontier},
   Year = {2014},
   url = {http://arxiv.org/pdf/1401.6077},
   Abstract = {http://arxiv.org/abs/1401.6077},
   Key = {Hewett:2014qja}
}

@article{fds248118,
   Author = {Scholberg, K},
   Title = {Daeδalus},
   Journal = {AIP Conference Proceedings},
   Volume = {1560},
   Pages = {179-183},
   Year = {2013},
   Month = {December},
   ISSN = {0094-243X},
   url = {http://dx.doi.org/10.1063/1.4826747},
   Abstract = {DAEδALUS (Decay At rest Experiment for δ studies At the
             Laboratory for Underground Science) is a new approach to
             measuring CP violation in the neutrino sector using
             few-tens-of-MeV neutrinos from decay at rest of pions
             created by multiple cyclotrons, in conjunction with a large
             inverse-beta-decay-sensitive detector. The DAEδALUS
             high-intensity stopped-pion neutrino sources would also
             enable exploration of low-energy neutrino physics at short
             baseline. © 2013 AIP Publishing LLC.},
   Doi = {10.1063/1.4826747},
   Key = {fds248118}
}

@article{fds325023,
   Author = {Izatt, B and Scholberq, K and McMahan, RP},
   Title = {Super-KAVE: An immersive visualization tool for neutrino
             physics},
   Journal = {Proceedings - IEEE Virtual Reality},
   Pages = {75-76},
   Year = {2013},
   Month = {October},
   ISBN = {9781467347952},
   url = {http://dx.doi.org/10.1109/VR.2013.6549370},
   Abstract = {Located under Japan's Mount Ikenoyama, the Super-Kamiokande
             (or 'Super-K') neutrino detector is used to study neutrino
             particle physics. The Super-K detector consists of a
             cylindrical stainless steel tank (41.4m tall and 39.3m in
             diameter) holding 50,000 tons of water and 13,031
             photomultiplier tubes (PMTs). To view the data captured by
             these sensors, many physicists use 2D visualization tools
             which present the data color-coded on a deconstructed
             representation of the cylinder. Unfortunately, this
             deconstructed visualization makes it difficult for
             physicists to fully visualize patterns of neutrino
             interactions. To address this, we have developed a novel
             virtual reality (VR) application called 'Super-KAVE', which
             uses a CAVE to immerse users in a lifesize representation of
             the Super-K detector. Super-KAVE displays the collocation of
             photon sensors and their color-coded data, provides a new
             visualization technique for neutrino-interaction patterns,
             and supports transitioning between data events. In this
             paper, we describe the Super-K detector and its data,
             discuss the design and implementation of our Super-KAVE
             application, and report on its expected uses. © 2013
             IEEE.},
   Doi = {10.1109/VR.2013.6549370},
   Key = {fds325023}
}

@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 = {737C},
   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{fds248126,
   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 = {fds248126}
}

@article{fds318468,
   Author = {Scholberg, K},
   Title = {Large underground detectors for proton decay and neutrino
             physics},
   Pages = {311-342},
   Booktitle = {100 Years of Subatomic Physics},
   Year = {2013},
   Month = {January},
   ISBN = {9789814425810},
   url = {http://dx.doi.org/10.1142/9789814425810_0012},
   Abstract = {© 2013 by World Scientific Publishing Co. Pte. Ltd. All
             rights reserved. This chapter tells the story of several
             decades of experimental physics done deep underground with
             huge detectors. Not for the first time in the history of
             science, the most exciting signals were not the ones
             originally sought. Large underground detectors were
             originally designed and built to search for the decay of the
             proton, which was predicted by Grand Unified Theories
             (GUTs). Later, these same detectors studied solar,
             supernova, and atmospheric neutrinos. The unambiguous
             discovery of neutrino mass and oscillations was a highlight
             of the end of last century; the solution to the solar
             neutrino problem was a highlight of the beginning of this
             century. Current-generation detectors acting as targets for
             reactor and beam neutrinos have been steadily improving our
             understanding of neutrinos. And the story is not over | the
             original quest for proton decay has not yet been fulfilled,
             neutrinos have not yet yielded all their secrets, and more
             surprises may be in store.},
   Doi = {10.1142/9789814425810_0012},
   Key = {fds318468}
}

@article{Akimov:2013yow,
   Author = {Akimov, D. and others},
   Title = {Coherent Scattering Investigations at the Spallation Neutron
             Source: a Snowmass White Paper},
   Year = {2013},
   url = {http://arxiv.org/pdf/1310.0125},
   Abstract = {http://arxiv.org/abs/1310.0125},
   Key = {Akimov:2013yow}
}

@article{Aberle:2013ssa,
   Author = {Aberle, C. and Adelmann, A. and Alonso, J. and Barletta,
             W.A. and Barlow, R. and others},
   Title = {Whitepaper on the DAEdALUS Program},
   Year = {2013},
   url = {http://arxiv.org/pdf/1307.2949},
   Abstract = {http://arxiv.org/abs/1307.2949},
   Key = {Aberle:2013ssa}
}

@article{Kearns:2013lea,
   Author = {Kearns, E. and others},
   Title = {Hyper-Kamiokande Physics Opportunities},
   Year = {2013},
   url = {http://arxiv.org/pdf/1309.0184},
   Abstract = {http://arxiv.org/abs/1309.0184},
   Key = {Kearns:2013lea}
}

@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{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{Lipton:2013hta,
   Author = {Lipton, R. and Mokhov, N.V. and Para, A. and Striganov, S.I. and Terentiev, N.K. and others},
   Title = {Compendium of Instrumentation Whitepapers on Frontier
             Physics Needs for Snowmass 2013},
   Year = {2013},
   Key = {Lipton:2013hta}
}

@article{Zhang:2013tua,
   Author = {Zhang, H. and others},
   Title = {Supernova Relic Neutrino Search with Neutron Tagging at
             Super-Kamiokande-IV},
   Year = {2013},
   url = {http://arxiv.org/pdf/1311.3738},
   Abstract = {http://arxiv.org/abs/1311.3738},
   Key = {Zhang:2013tua}
}

@article{Scholberg:2013pxa,
   Author = {Scholberg, K},
   Title = {The long-baseline neutrino experiment},
   Journal = {Nuclear Physics, Section B: Proceedings Supplements},
   Volume = {237-238},
   Pages = {184-186},
   Year = {2013},
   ISSN = {0920-5632},
   url = {http://dx.doi.org/10.1016/j.nuclphysbps.2013.04.085},
   Abstract = {This document briefly describes the physics goals of the
             Long-Baseline Neutrino Experiment planned for the United
             States, and a snapshot of its status in fall 2012. © 2013
             Elsevier B.V.},
   Doi = {10.1016/j.nuclphysbps.2013.04.085},
   Key = {Scholberg:2013pxa}
}

@article{Scholberg:2013hba,
   Author = {Scholberg, K and Villante, FL},
   Title = {Oscillations at low energies},
   Journal = {Nuclear Physics, Section B: Proceedings Supplements},
   Volume = {237-238},
   Pages = {352-357},
   Year = {2013},
   ISSN = {0920-5632},
   url = {http://dx.doi.org/10.1016/j.nuclphysbps.2013.04.125},
   Abstract = {We summarize here, briefly, the experimental and theoretical
             results presented at the NOW2012 workshop during the
             parallel session "Oscillation at low energies". The talks
             covered a wide range of topics, including reactor neutrinos,
             solar neutrinos, supernovae neutrinos and sterile neutrino
             searches. The session featured new results, reviews and
             ideas for the future. © 2013 Elsevier B.V.},
   Doi = {10.1016/j.nuclphysbps.2013.04.125},
   Key = {Scholberg:2013hba}
}

@article{Patton:2013nwa,
   Author = {Patton, KM and McLaughlin, GC and Scholberg, K},
   Title = {Prospects for using coherent elastic neutrino-nucleus
             scattering to measure the nuclear neutron form
             factor},
   Journal = {International Journal of Modern Physics E},
   Volume = {22},
   Number = {6},
   Pages = {1330013},
   Year = {2013},
   ISSN = {0218-3013},
   url = {http://dx.doi.org/10.1142/S0218301313300130},
   Abstract = {We review the prospects of using coherent elastic
             neutrino-nucleus scattering (CENNS) to measure the nuclear
             neutron form factor. The merits and limitations of several
             potential neutrino sources are discussed. The effects of
             detector shape uncertainty and detector size on a
             measurement of the neutron RMS radius are also considered.
             We find that the detector spectral shape uncertainty is the
             important limiting factor on a measurement of the neutron
             RMS radius. In order to measure the neutron RMS radius to
             5%, the spectral shape uncertainty of the detector needs to
             be known to 1% or better. © 2013 World Scientific
             Publishing Company.},
   Doi = {10.1142/S0218301313300130},
   Key = {Patton:2013nwa}
}

@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{fds248204,
   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},
   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 = {fds248204}
}

@article{Scholberg:2012zz,
   Author = {Scholberg, K.},
   Title = {DAEdALUS},
   Journal = {AIP Conf.Proc.},
   Volume = {1441},
   Pages = {435-437},
   Year = {2012},
   url = {http://dx.doi.org/10.1063/1.3700577},
   Doi = {10.1063/1.3700577},
   Key = {Scholberg:2012zz}
}

@article{Hewett:2012ns,
   Author = {Hewett, J.L. and Weerts, H. and Brock, R. and Butler, J.N. and Casey, B.C.K. and others},
   Title = {Fundamental Physics at the Intensity Frontier},
   Year = {2012},
   url = {http://arxiv.org/pdf/1205.2671},
   Abstract = {http://arxiv.org/abs/1205.2671},
   Key = {Hewett:2012ns}
}

@article{Regis:2012sn,
   Author = {Regis, C. and others},
   Title = {Search for Proton Decay via $p -> \mu^+ K^0$ in
             Super-Kamiokande I, II, and III},
   Journal = {Phys.Rev.},
   Volume = {D86},
   Pages = {012006},
   Year = {2012},
   url = {http://arxiv.org/pdf/1205.6538},
   Abstract = {http://arxiv.org/abs/1205.6538},
   Doi = {10.1103/PhysRevD.86.012006},
   Key = {Regis:2012sn}
}

@article{Abazajian:2012ys,
   Author = {Abazajian, K.N. and Acero, M.A. and Agarwalla, S.K. and Aguilar-Arevalo, A.A. and Albright, C.H. and others},
   Title = {Light Sterile Neutrinos: A White Paper},
   Year = {2012},
   url = {http://arxiv.org/pdf/1204.5379},
   Abstract = {http://arxiv.org/abs/1204.5379},
   Key = {Abazajian:2012ys}
}

@article{Bolozdynya:2012xv,
   Author = {Bolozdynya, A. and Cavanna, F. and Efremenko, Y. and Garvey,
             G.T. and Gudkov, V. and others},
   Title = {Opportunities for Neutrino Physics at the Spallation Neutron
             Source: A White Paper},
   Year = {2012},
   url = {http://arxiv.org/pdf/1211.5199},
   Abstract = {http://arxiv.org/abs/1211.5199},
   Key = {Bolozdynya:2012xv}
}

@article{Cianciolo:2012ex,
   Author = {Cianciolo, V. and Balantekin, A.B. and Bernstein, A. and Cirigliano, V. and Cooper, M.D. and others},
   Title = {Discovering the New Standard Model: Fundamental Symmetries
             and Neutrinos},
   Year = {2012},
   url = {http://arxiv.org/pdf/1212.5190},
   Abstract = {http://arxiv.org/abs/1212.5190},
   Key = {Cianciolo:2012ex}
}

@article{Scholberg:2011kt,
   Author = {Scholberg, K},
   Title = {Supernova neutrino detection},
   Journal = {Journal of Physics},
   Volume = {375},
   Number = {PART 4},
   Pages = {042036},
   Year = {2012},
   ISSN = {1742-6588},
   url = {http://dx.doi.org/10.1088/1742-6596/375/1/042036},
   Abstract = {When a massive star collapses at the end of its life, nearly
             all of the gravitational binding energy of the resulting
             remnant is released in the form of neutrinos. The burst of
             neutrinos from a Galactic core collapse supernova will be
             detected in neutrino detectors worldwide. This talk will
             cover supernova neutrino detection techniques in general,
             current supernova neutrino detectors, and prospects for
             specific future experiments.},
   Doi = {10.1088/1742-6596/375/1/042036},
   Key = {Scholberg:2011kt}
}

@article{fds248196,
   Author = {Scholberg, K},
   Title = {DAEδALUS},
   Journal = {AIP Conference Proceedings},
   Volume = {1441},
   Pages = {435-437},
   Year = {2012},
   ISSN = {0094-243X},
   url = {http://dx.doi.org/10.1063/1.3700577},
   Abstract = {DAEδALUS (Decay At rest Experiment for δ studies At the
             Laboratory for Underground Science) is a new approach to
             measuring CP violation in the neutrino sector using
             few-tens-of-MeV neutrinos from decay at rest of pions
             created by multiple cyclotrons, in conjunction with a large
             water Cherenkov detector. The DAEδALUS high-intensity
             stopped-pion neutrino sources would also enable exploration
             of low-energy neutrino physics at short baseline. © 2012
             American Institute of Physics.},
   Doi = {10.1063/1.3700577},
   Key = {fds248196}
}

@article{Scholberg:2012jg,
   Author = {Scholberg, K},
   Title = {Future underground large detectors: prospects and physics
             case},
   Journal = {Journal of Physics},
   Volume = {375},
   Number = {PART 4},
   Pages = {042048},
   Year = {2012},
   ISSN = {1742-6588},
   url = {http://dx.doi.org/10.1088/1742-6596/375/4/042048},
   Abstract = {A new generation of large underground detectors is being
             planned to further investigate neutrino mass and mixing and
             to search for possible CP violation that may provide a hint
             to the origin of our asymmetric universe. Such detectors
             would also investigate neutrinos in nature - from the
             earth's crust to supernovae. The physics case for such a
             program is presented and plans for detectors worldwide are
             summarized.},
   Doi = {10.1088/1742-6596/375/4/042048},
   Key = {Scholberg:2012jg}
}

@article{Scholberg:2012xfa,
   Author = {Scholberg, K},
   Title = {Prospects for measuring neutrino-nucleus coherent scattering
             with a stopped-pion neutrino source},
   Journal = {Nuclear Physics, Section B: Proceedings Supplements},
   Volume = {229-232},
   Pages = {505-},
   Year = {2012},
   ISSN = {0920-5632},
   url = {http://dx.doi.org/10.1016/j.nuclphysbps.2012.09.142},
   Abstract = {This poster describes prospects for measurement of coherent
             elastic neutrino-nucleus scattering using various
             potentially available stopped-pion neutrino sources, noting
             the possibility of detection in dark matter detectors at
             DUSEL in conjunction with the proposed DAEδALUS neutrino
             source. © 2012.},
   Doi = {10.1016/j.nuclphysbps.2012.09.142},
   Key = {Scholberg:2012xfa}
}

@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 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},
   Pages = {010001},
   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 = {Beringer:1900zz}
}

@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{Scholberg:2012id,
   Author = {Scholberg, K},
   Title = {Supernova neutrino detection},
   Journal = {Annual Review of Nuclear and Particle Science},
   Volume = {62},
   Number = {81},
   Pages = {81-103},
   Year = {2012},
   ISSN = {0163-8998},
   url = {http://arxiv.org/pdf/1205.6003},
   Abstract = {A core-collapse supernova will produce an enormous burst of
             neutrinos of all flavors in the few-tens-of-MeV range.
             Measurement of the flavor, time, and energy structure of a
             nearby core-collapse neutrino burst will yield answers to
             many physics and astrophysics questions. The neutrinos left
             over from past cosmic supernovae are also observable, and
             their detection will improve knowledge of core-collapse
             rates and average neutrino emission. This review describes
             experimental techniques for detection of core-collapse
             neutrinos, as well as the sensitivities of current and
             future detectors. © 2012 by Annual Reviews.},
   Doi = {10.1146/annurev-nucl-102711-095006},
   Key = {Scholberg:2012id}
}

@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{Anderson:2012pn,
   Author = {Anderson, AJ and Conrad, JM and Figueroa-Feliciano, E and Ignarra, C and Karagiorgi, G and Scholberg, K and Shaevitz, MH and Spitz,
             J},
   Title = {Measuring active-to-sterile neutrino oscillations with
             neutral current coherent neutrino-nucleus
             scattering},
   Journal = {Physical Review D - Particles, Fields, Gravitation, and
             Cosmology},
   Volume = {86},
   Number = {1},
   Pages = {013004},
   Year = {2012},
   ISSN = {1550-7998},
   url = {http://arxiv.org/pdf/1201.3805},
   Abstract = {Light sterile neutrinos have been introduced as an
             explanation for a number of oscillation signals at
             Δm2∼1eV2. Neutrino oscillations at relatively short
             baselines provide a probe of these possible new states. This
             paper describes an accelerator-based experiment using
             neutral current coherent neutrino-nucleus scattering to
             strictly search for active-to-sterile neutrino oscillations.
             This experiment could, thus, definitively establish the
             existence of sterile neutrinos and provide constraints on
             their mixing parameters. A cyclotron-based proton beam can
             be directed to multiple targets, producing a low-energy pion
             and muon decay-at-rest neutrino source with variable
             distance to a single detector. Two types of detectors are
             considered: a germanium-based detector inspired by the
             SuperCDMS design and a liquid argon detector inspired by the
             proposed CLEAR experiment. © 2012 American Physical
             Society.},
   Doi = {10.1103/PhysRevD.86.013004},
   Key = {Anderson:2012pn}
}

@article{fds248206,
   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},
   Year = {2012},
   ISSN = {1550-7998},
   url = {http://dx.doi.org/10.1103/PhysRevD.86.012006},
   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 = {fds248206}
}

@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{Abe:2011xv,
   Author = {Abe, K and Abgrall, N and Ajima, Y and Aihara, H and Albert, JB and Andreopoulos, C and Andrieu, B and Anerella, MD and Aoki, S and Araoka,
             O and Argyriades, J and Ariga, A and Ariga, T and Assylbekov, S and Autiero, D and Badertscher, A and Barbi, M and Barker, GJ and Barr, G and Bass, M and Batkiewicz, M and Bay, F and Bentham, S and Berardi, V and Berger, BE and Bertram, I and Besnier, M and Beucher, J and Beznosko, D and Bhadra, S and Blaszczyk, FDM and Blocki, J and Blondel, A and Bojechko,
             C and Bouchez, J and Boyd, SB and Bravar, A and Bronner, C and Brook-Roberge, DG and Buchanan, N and Budd, H et
             al.},
   Title = {Measurements of the T2K neutrino beam properties using the
             INGRID on-axis near detector},
   Journal = {Nuclear Instruments and Methods in Physics Research Section
             A: Accelerators, Spectrometers, Detectors and Associated
             Equipment},
   Volume = {694},
   Pages = {211-223},
   Year = {2012},
   ISSN = {0168-9002},
   url = {http://arxiv.org/pdf/1111.3119},
   Abstract = {Precise measurement of neutrino beam direction and intensity
             was achieved based on a new concept with modularized
             neutrino detectors. INGRID (Interactive Neutrino GRID) is an
             on-axis near detector for the T2K long baseline neutrino
             oscillation experiment. INGRID consists of 16 identical
             modules arranged in horizontal and vertical arrays around
             the beam center. The module has a sandwich structure of iron
             target plates and scintillator trackers. INGRID directly
             monitors the muon neutrino beam profile center and intensity
             using the number of observed neutrino events in each module.
             The neutrino beam direction is measured with accuracy better
             than 0.4 mrad from the measured profile center. The
             normalized event rate is measured with 4% precision. © 2012
             Elsevier B.V. All rights reserved.},
   Doi = {10.1016/j.nima.2012.03.023},
   Key = {Abe:2011xv}
}

@article{Abe:2012gx,
   Author = {Abe, K and Abgrall, N and Ajima, Y and Aihara, H and Albert, JB and Andreopoulos, C and Andrieu, B and Anerella, MD and Aoki, S and Araoka,
             O and Argyriades, J and Ariga, A and Ariga, T and Assylbekov, S and Autiero, D and Badertscher, A and Barbi, M and Barker, GJ and Barr, G and Bass, M and Batkiewicz, M and Bay, F and Bentham, S and Berardi, V and Berger, BE and Bertram, I and Besnier, M and Beucher, J and Beznosko, D and Bhadra, S and Blaszczyk, FDMM and Blondel, A and Bojechko, C and Bouchez, J and Boyd, SB and Bravar, A and Bronner, C and Brook-Roberge,
             DG and Buchanan, N and Budd, H and Calland, RG et
             al.},
   Title = {First muon-neutrino disappearance study with an off-axis
             beam},
   Journal = {Physical Review D - Particles, Fields, Gravitation, and
             Cosmology},
   Volume = {85},
   Number = {3},
   Pages = {031103},
   Year = {2012},
   ISSN = {1550-7998},
   url = {http://arxiv.org/pdf/1201.1386},
   Abstract = {We report a measurement of muon-neutrino disappearance in
             the T2K experiment. The 295-km muon-neutrino beam from Tokai
             to Kamioka is the first implementation of the off-axis
             technique in a long-baseline neutrino oscillation
             experiment. With data corresponding to 1.43×1020 protons on
             target, we observe 31 fully-contained single μ-like ring
             events in Super-Kamiokande, compared with an expectation of
             104±14(syst) events without neutrino oscillations. The
             best-fit point for two-flavor ν μ→ν τ oscillations is
             sin2(2θ 23)=0.98 and |Δm322|=2.65×10 -3eV2. The boundary
             of the 90% confidence region includes the points ( sin2(2θ
             23), |Δm322|)=(1.0,3.1×10 -3eV2), (0.84, 2.65×10 -3eV2)
             and (1.0, 2.2×10 -3eV2). © 2012 American Physical
             Society.},
   Doi = {10.1103/PhysRevD.85.031103},
   Key = {Abe:2012gx}
}

@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{Abe:2011sj,
   Author = {Abe, K and Abgrall, N and Ajima, Y and Aihara, H and Albert, JB and Andreopoulos, C and Andrieu, B and Aoki, S and Araoka, O and Argyriades,
             J and Ariga, A and Ariga, T and Assylbekov, S and Autiero, D and Badertscher, A and Barbi, M and Barker, GJ and Barr, G and Bass, M and Bay,
             F and Bentham, S and Berardi, V and Berger, BE and Bertram, I and Besnier,
             M and Beucher, J and Beznosko, D and Bhadra, S and Blaszczyk, FDMM and Blondel, A and Bojechko, C and Bouchez, J and Boyd, SB and Bravar, A and Bronner, C and Brook-Roberge, DG and Buchanan, N and Budd, H and Calvet,
             D and Cartwright, SL and Carver, A et al.},
   Title = {Indication of electron neutrino appearance from an
             accelerator-produced off-axis muon neutrino
             beam.},
   Journal = {Physical Review Letters},
   Volume = {107},
   Number = {4},
   Pages = {041801},
   Year = {2011},
   Month = {July},
   url = {http://www.ncbi.nlm.nih.gov/pubmed/21866992},
   Abstract = {The T2K experiment observes indications of ν(μ) → ν(e)
             appearance in data accumulated with 1.43×10(20) protons on
             target. Six events pass all selection criteria at the far
             detector. In a three-flavor neutrino oscillation scenario
             with |Δm(23)(2)| = 2.4×10(-3)  eV(2), sin(2)2θ(23) =
             1 and sin(2)2θ(13) = 0, the expected number of such events
             is 1.5±0.3(syst). Under this hypothesis, the probability to
             observe six or more candidate events is 7×10(-3),
             equivalent to 2.5σ significance. At 90% C.L., the data are
             consistent with 0.03(0.04) < sin(2)2θ(13) < 0.28(0.34) for
             δ(CP) = 0 and a normal (inverted) hierarchy.},
   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},
   Volume = {83},
   Number = {5},
   Pages = {052010},
   Year = {2011},
   Month = {March},
   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 = {http://arxiv.org/abs/1010.0118},
   Doi = {10.1103/PhysRevD.83.052010},
   Key = {Abe:2010hy}
}

@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{Akiri:2011dv,
   Author = {Akiri, T. and others},
   Title = {The 2010 Interim Report of the Long-Baseline Neutrino
             Experiment Collaboration Physics Working
             Groups},
   Year = {2011},
   url = {http://arxiv.org/pdf/1110.6249},
   Abstract = {http://arxiv.org/abs/1110.6249},
   Key = {Akiri:2011dv}
}

@article{Scholberg:2011zzb,
   Author = {Scholberg, K},
   Title = {Supernova neutrino detection in water Cherenkov
             detectors},
   Journal = {Journal of Physics},
   Volume = {309},
   Number = {1},
   Pages = {012028},
   Year = {2011},
   ISSN = {1742-6588},
   url = {http://dx.doi.org/10.1088/1742-6596/309/1/012028},
   Abstract = {This talk will describe sensitivity of past, current and
             future water Cherenkov detectors to a burst of supernova
             neutrinos.},
   Doi = {10.1088/1742-6596/309/1/012028},
   Key = {Scholberg:2011zzb}
}

@article{fds248189,
   Author = {Irastorza, IG and Scholberg, K and Colas, P and Giomataris,
             I},
   Title = {Preface},
   Journal = {Journal of Physics},
   Volume = {309},
   Number = {1},
   Pages = {iii},
   Year = {2011},
   ISSN = {1742-6588},
   url = {http://dx.doi.org/10.1088/1742-6596/309/1/011001},
   Doi = {10.1088/1742-6596/309/1/011001},
   Key = {fds248189}
}

@article{Scholberg:2011zza,
   Author = {Scholberg, K},
   Title = {The T2K experiment},
   Journal = {Journal of Physics},
   Volume = {309},
   Number = {1},
   Pages = {012018},
   Year = {2011},
   ISSN = {1742-6588},
   url = {http://dx.doi.org/10.1088/1742-6596/309/1/012018},
   Abstract = {This talk will describe briefly the physics goals of the
             Tokai to Kamioka (T2K) experiment, and its current status
             and prospects.},
   Doi = {10.1088/1742-6596/309/1/012018},
   Key = {Scholberg:2011zza}
}

@article{Burgmeier:2011zz,
   Author = {Burgmeier, A and Scholberg, K and Wendell, R},
   Title = {Supernova pointing by neutrino matter oscillation},
   Journal = {Journal of Physics},
   Volume = {312},
   Number = {SECTION 7},
   Pages = {072007},
   Year = {2011},
   ISSN = {1742-6588},
   url = {http://dx.doi.org/10.1088/1742-6596/312/7/072007},
   Abstract = {A core-collapse supernova will emit a neutrino burst that
             can be detected on Earth. If the neutrinos travel through
             the Earth before reaching the detector they oscillate via
             interaction with Earth's matter, yielding oscillations in
             the neutrino energy spectrum. The frequency of these
             oscillations in energy is correlated with the pathlength
             traveled in the Earth and therefore contains information on
             the supernova location. For this technique to be useful for
             pointing, good energy resolution, well-known oscillation
             parameters and high statistics are required. This method is
             inferior to pointing with elastic scattering in a water
             Cherenkov detector but could be applied for
             scintillator-type detectors which have better energy
             resolution but weak intrinsic pointing capabilities. By the
             time a nearby supernova happens the requirements might well
             be fulfilled, and if no water Cherenkov detector is running
             at that time it may provide the only possibility to gain
             directional information. The pointing quality can be further
             improved by the combination of measurements from multiple
             detectors and also by taking relative timing into
             account.},
   Doi = {10.1088/1742-6596/312/7/072007},
   Key = {Burgmeier:2011zz}
}

@article{Scholberg:2011zzd,
   Author = {Scholberg, K},
   Title = {Experimental measurement of low energy neutrino
             interactions},
   Journal = {AIP Conference Proceedings},
   Volume = {1405},
   Pages = {277-282},
   Year = {2011},
   ISSN = {0094-243X},
   url = {http://dx.doi.org/10.1063/1.3661600},
   Abstract = {Neutrino interactions in the few to few tens of MeV range
             are of importance for several physics topics, including
             solar, supernova and reactor neutrinos, as well as future
             proposed oscillation and Standard Model test experiments.
             Although interaction cross-sections for some simple targets
             are well understood, very little experimental data exist for
             interactions with nuclei. This talk will discuss the
             motivation for measuring low energy neutrino interactions,
             the state of knowledge, and possible future strategies. ©
             2011 American Institute of Physics.},
   Doi = {10.1063/1.3661600},
   Key = {Scholberg:2011zzd}
}

@article{fds248193,
   Author = {Scholberg, K},
   Title = {Neutrino mass and oscillations},
   Journal = {Journal of Physics},
   Volume = {312},
   Number = {SECTION 7},
   Year = {2011},
   ISSN = {1742-6588},
   url = {http://dx.doi.org/10.1088/1742-6596/312/7/072002},
   Abstract = {This talk will summarize the current experimental
             understanding of neutrino mass and oscillation parameters,
             and will discuss prospects for future experiments.},
   Doi = {10.1088/1742-6596/312/7/072002},
   Key = {fds248193}
}

@article{Scholberg:2011zz,
   Author = {Scholberg, K},
   Title = {Prospects for Measuring Neutrino-Nucleus Coherent Scattering
             at a Stopped-Pion Neutrino Source},
   Journal = {Nuclear Physics, Section B: Proceedings Supplements},
   Volume = {221},
   Pages = {395-},
   Year = {2011},
   ISSN = {0920-5632},
   url = {http://dx.doi.org/10.1016/j.nuclphysbps.2011.10.043},
   Doi = {10.1016/j.nuclphysbps.2011.10.043},
   Key = {Scholberg:2011zz}
}

@article{Scholberg:2007nu,
   Author = {Scholberg, K},
   Title = {Supernova neutrino detection},
   Journal = {Nuclear Physics, Section B: Proceedings Supplements},
   Volume = {221},
   Pages = {248-253},
   Year = {2011},
   ISSN = {0920-5632},
   url = {http://arxiv.org/pdf/astro-ph/0701081},
   Abstract = {The gravitational core collapse of a star produces a huge
             burst of neutrinos of all flavors. A number of detectors
             worldwide are sensitive to such a burst; its detection would
             yield information about both particle physics and
             astrophysics. Sensitivity to all flavors, and ability to tag
             different interactions will be key for extraction of
             information. Here I will survey the capabilities of current
             and future detectors for detection of supernova neutrinos
             from the Milky Way and beyond. © 2011 Elsevier
             B.V.},
   Doi = {10.1016/j.nuclphysbps.2011.09.012},
   Key = {Scholberg:2007nu}
}

@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{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{Anderson:2011bi,
   Author = {Anderson, AJ and Conrad, JM and Figueroa-Feliciano, E and Scholberg,
             K and Spitz, J},
   Title = {Coherent neutrino scattering in dark matter
             detectors},
   Journal = {Physical Review D - Particles, Fields, Gravitation, and
             Cosmology},
   Volume = {84},
   Number = {1},
   Pages = {013008},
   Year = {2011},
   ISSN = {1550-7998},
   url = {http://arxiv.org/pdf/1103.4894},
   Abstract = {Coherent elastic neutrino-nucleus and weakly interacting
             massive particle-nucleus interaction signatures are expected
             to be quite similar. This paper discusses how a
             next-generation ton-scale dark matter detector could
             discover neutrino-nucleus coherent scattering, a
             precisely-predicted standard model process. A high-intensity
             pion- and muon- decay-at-rest neutrino source recently
             proposed for oscillation physics at underground laboratories
             would provide the neutrinos for these measurements. In this
             paper, we calculate raw rates for various target materials
             commonly used in dark matter detectors and show that
             discovery of this interaction is possible with a 2ton•year
             GEODM exposure in an optimistic energy threshold and
             efficiency scenario. We also study the effects of the
             neutrino source on weakly interacting massive particle
             sensitivity and discuss the modulated neutrino signal as a
             sensitivity/ consistency check between different dark matter
             experiments at the Deep Underground Science and Engineering
             Laboratory. Furthermore, we consider the possibility of
             coherent neutrino physics with a GEODM module placed within
             tens of meters of the neutrino source. © 2011 American
             Physical Society.},
   Doi = {10.1103/PhysRevD.84.013008},
   Key = {Anderson:2011bi}
}

@article{Tanaka:2011uf,
   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},
   Pages = {78},
   Year = {2011},
   ISSN = {0004-637X},
   url = {http://arxiv.org/pdf/1108.3384},
   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 = {Tanaka:2011uf}
}

@article{:2008zn,
   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 = {032002},
   Year = {2011},
   ISSN = {1550-7998},
   url = {http://arxiv.org/pdf/0803.4312},
   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 = {:2008zn}
}

@article{fds287697,
   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},
   Year = {2011},
   ISSN = {1550-7998},
   url = {http://dx.doi.org/10.1103/PhysRevD.83.054023},
   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 = {fds287697}
}

@article{fds318469,
   Author = {Ahluwalia, R and Chartrand, TL and Ratner, RK},
   Title = {Preface},
   Journal = {Advances in Consumer Research},
   Volume = {39},
   Pages = {iii},
   Year = {2011},
   Key = {fds318469}
}

@article{fds248119,
   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 = {fds248119}
}

@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{Alonso:2010fs,
   Author = {Alonso, J. and others},
   Title = {Expression of Interest for a Novel Search for CP Violation
             in the Neutrino Sector: DAEdALUS},
   Year = {2010},
   url = {http://arxiv.org/pdf/1006.0260},
   Abstract = {http://arxiv.org/abs/1006.0260},
   Key = {Alonso:2010fs}
}

@article{:2010fy,
   Author = {Alonso, J. and others},
   Title = {A Study of Detector Configurations for the DUSEL CP
             Violation Searches Combining LBNE and DAEdALUS},
   Year = {2010},
   url = {http://arxiv.org/pdf/1008.4967},
   Abstract = {http://arxiv.org/abs/1008.4967},
   Key = {:2010fy}
}

@article{Scholberg:2010zz,
   Author = {Scholberg, K},
   Title = {Future supernova neutrino detectors},
   Journal = {Journal of Physics},
   Volume = {203},
   Pages = {012079},
   Year = {2010},
   ISSN = {1742-6588},
   url = {http://dx.doi.org/10.1088/1742-6596/203/1/012079},
   Abstract = {This joint neutrino-gravitational wave session talk will
             describe current, near future and farther future supernova
             neutrino detectors. I will comment on the potential of
             future supernova neutrino-gravitational wave correlation
             searches. © 2010 IOP Publishing Ltd.},
   Doi = {10.1088/1742-6596/203/1/012079},
   Key = {Scholberg:2010zz}
}

@article{Schumaker:2010ata,
   Author = {Schumaker, MA and Boeltzig, A and Burritt, TH and Duba, CA and Duncan,
             FA and Farine, J and Habig, A and Hime, A and Howe, MA and Kielbik, A and Kraus, C and Nicholson, K and Robertson, RGH and Scholberg, K and Secrest, J and Shantz, TC and Virtue, CJ and Wilkerson, JF and Yen, S and Zuber, K},
   Title = {Data acquisition for the Helium and Lead
             Observatory},
   Journal = {IEEE Nuclear Science Symposium Conference
             Record},
   Volume = {2010},
   Pages = {1860-1865},
   Year = {2010},
   ISSN = {1095-7863},
   url = {http://dx.doi.org/10.1109/NSSMIC.2010.5874097},
   Abstract = {The Helium and Lead Observatory (HALO) is a dedicated
             supernova detector constructed in the underground facilities
             at SNOLAB in Sudbury, Canada. It is designed to detect
             neutrinos from a supernova within the Milky Way galaxy using
             lead blocks and 3He neutron detectors. Analysis of supernova
             neutrino events can produce new discoveries in astrophysics
             and fundamental particle physics. HALO will be a participant
             in the Supernova Early Warning System (SNEWS), which will
             rely on the time delay between neutrino emission and visible
             light emission to provide notification to astronomers of an
             imminent observable supernova. This article discusses the
             data acquisition system of HALO, including the software
             ORCA, electronics components, data flow, and the design of
             the high-voltage and signal connections for the 3He neutron
             detectors. © 2010 IEEE.},
   Doi = {10.1109/NSSMIC.2010.5874097},
   Key = {Schumaker:2010ata}
}

@article{Scholberg:2009jr,
   Author = {Scholberg, K and Burgmeier, A and Wendell, R},
   Title = {Obtaining supernova directional information using the
             neutrino matter oscillation pattern},
   Journal = {Physical Review D - Particles, Fields, Gravitation, and
             Cosmology},
   Volume = {81},
   Number = {4},
   Pages = {043007},
   Year = {2010},
   ISSN = {1550-7998},
   url = {http://hdl.handle.net/10161/4272 Duke open
             access},
   Abstract = {A nearby core collapse supernova will produce a burst of
             neutrinos in several detectors worldwide. With reasonably
             high probability, the Earth will shadow the neutrino flux in
             one or more detectors. In such a case, for allowed
             oscillation parameter scenarios, the observed neutrino
             energy spectrum will bear the signature of oscillations in
             Earth matter. Because the frequency of the oscillations in
             energy depends on the path length traveled by the neutrinos
             in the Earth, an observed spectrum also contains information
             about the direction to the supernova. We explore here the
             possibility of constraining the supernova location using
             matter oscillation patterns observed in a detector. Good
             energy resolution (typical of scintillator detectors),
             well-known oscillation parameters, and optimistically large
             (but conceivable) statistics are required. Pointing by this
             method can be significantly improved using multiple
             detectors located around the globe. Although it is not
             competitive with neutrino-electron elastic scattering-based
             pointing with water Cherenkov detectors, the technique could
             still be useful. © 2010 The American Physical
             Society.},
   Doi = {10.1103/PhysRevD.81.043007},
   Key = {Scholberg:2009jr}
}

@article{Leonor:2010yp,
   Author = {Leonor, I and Cadonati, L and Coccia, E and D'Antonio, S and Credico,
             AD and Fafone, V and Frey, R and Fulgione, W and Katsavounidis, E and Ott,
             CD and Pagliaroli, G and Scholberg, K and Thrane, E and Vissani,
             F},
   Title = {Searching for prompt signatures of nearby core-collapse
             supernovae by a joint analysis of neutrino and gravitational
             wave data},
   Journal = {Classical and Quantum Gravity},
   Volume = {27},
   Number = {8},
   Pages = {084019},
   Year = {2010},
   ISSN = {0264-9381},
   url = {http://arxiv.org/pdf/1002.1511},
   Abstract = {We discuss the science motivations and prospects for a joint
             analysis of gravitational wave (GW) and low-energy neutrino
             data to search for prompt signals from nearby supernovae
             (SNe). Both gravitational wave and low-energy neutrinos are
             expected to be produced in the innermost region of a
             core-collapse supernova, and a search for coincident signals
             would probe the processes which power a supernova explosion.
             It is estimated that the current generation of neutrino and
             gravitational wave detectors would be sensitive to galactic
             core-collapse supernovae, and would also be able to detect
             electromagnetically dark SNe. A joint GW-neutrino search
             would enable improvements to searches by way of lower
             detection thresholds, larger distance range, better
             live-time coverage by a network of GW and neutrino
             detectors, and increased significance of candidate
             detections. A close collaboration between the GW and
             neutrino communities for such a search will thus go far
             toward realizing a much sought-after astrophysics goal of
             detecting the next nearby supernova. © 2010 IOP Publishing
             Ltd.},
   Doi = {10.1088/0264-9381/27/8/084019},
   Key = {Leonor:2010yp}
}

@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{fds167254,
   Author = {Scholberg, K. and Wongjirad, T. and Hungerford, E. and Empl, A. and Markoff, D. and Efremenko, Y. and McKinsey, D. and Nikkel,
             J.},
   Title = {The CLEAR Experiment},
   Journal = {Proceedings of DPF 2009},
   Year = {2009},
   url = {http://arXiv.org/pdf/0910.1989v2},
   Abstract = {http://arXiv.org/abs/0910.1989},
   Key = {fds167254}
}

@article{Bernstein:2009ms,
   Author = {Bernstein, L. A. 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{Scholberg:2009zz,
   Author = {Scholberg, K},
   Title = {Neutrino Experiments at the SNS},
   Journal = {AIP Conference Proceedings},
   Volume = {1182},
   Pages = {76-79},
   Year = {2009},
   ISBN = {978-0-7354-0723-7},
   ISSN = {0094-243X},
   url = {http://dx.doi.org/10.1063/1.3293919},
   Abstract = {This talk describes planned neutrino physics experiments at
             the Spallation Neutron Source in Oak Ridge, Tennessee, with
             a focus on the proposed CLEAR (Coherent Low Energy
             Nuclear(A) Recoils) experiment. © 2009 American Institute
             of Physics.},
   Doi = {10.1063/1.3293919},
   Key = {Scholberg:2009zz}
}

@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{fds248225,
   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://dx.doi.org/10.1088/0004-637X/697/1/730},
   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 = {fds248225}
}

@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{: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{Duba:2008zz,
   Author = {Duba, C.A. and Duncan, F. and Farine, J. and Habig, A. and Hime, A. and others},
   Title = {HALO: The helium and lead observatory for supernova
             neutrinos},
   Journal = {J.Phys.Conf.Ser.},
   Volume = {136},
   Pages = {042077},
   Year = {2008},
   url = {http://dx.doi.org/10.1088/1742-6596/136/4/042077},
   Doi = {10.1088/1742-6596/136/4/042077},
   Key = {Duba:2008zz}
}

@article{:2008ea,
   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://arxiv.org/pdf/0805.0186},
   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 = {:2008ea}
}

@article{Abe:2008zz,
   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://dx.doi.org/10.1103/PhysRevD.77.052001},
   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:2008zz}
}

@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{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{Scholberg:2008fa,
   Author = {Scholberg, K},
   Title = {The supernova early warning system},
   Journal = {Astronomische Nachrichten},
   Volume = {329},
   Number = {3},
   Pages = {337-339},
   Year = {2008},
   ISSN = {0004-6337},
   url = {http://arxiv.org/pdf/arXiv:0803.0531 [astro-ph]},
   Abstract = {A core collapse in the Milky Way will produce an enormous
             burst of neutrinos in detectors world-wide. Such a burst has
             the potential to provide an early warning of a supernova's
             appearance. I will describe the nature of the signal, the
             sensitivity of current detectors, and SNEWS, the SuperNova
             Early Warning System, a network designed to alert
             astronomers as soon as possible after the detected neutrino
             signal. © 2008 Wiley-VCH Verlag GmbH &amp; Co.
             KGaA.},
   Doi = {10.1002/asna.200710934},
   Key = {Scholberg:2008fa}
}

@article{fds248245,
   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 = {112001},
   Year = {2008},
   ISSN = {1550-7998},
   url = {http://arxiv.org/abs/hep-ex/0508053},
   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 = {fds248245}
}

@article{fds304613,
   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 = {fds304613}
}

@article{Scholberg:2008zza,
   Author = {Scholberg, K},
   Title = {CLEAR: Prospects for a Low Threshold Neutrino Experiment at
             the Spallation Neutron Source},
   Journal = {Journal of Physics},
   Volume = {136},
   Pages = {042044},
   Year = {2008},
   url = {http://dx.doi.org/10.1088/1742-6596/136/4/042044},
   Doi = {10.1088/1742-6596/136/4/042044},
   Key = {Scholberg:2008zza}
}

@article{Scholberg:2007zz,
   Author = {Scholberg, K},
   Title = {Neutrinos at the Spallation Neutron Source},
   Journal = {AIP Conference Proceedings},
   Volume = {967},
   Pages = {72-75},
   Year = {2007},
   ISSN = {0094-243X},
   url = {http://dx.doi.org/10.1063/1.2834514},
   Abstract = {The Spallation Neutron Source at Oak Ridge will provide an
             intense source of neutrinos in the tens of MeV range, which
             nicely overlaps with the supernova neutrino energy range. I
             will describe the Neutrinos at the SNS (vSNS) program
             planned to exploit this high power, high quality source for
             studies of neutrino cross-sections relevant for supernova
             neutrino physics. © 2007 American Institute of
             Physics.},
   Doi = {10.1063/1.2834514},
   Key = {Scholberg:2007zz}
}

@article{fds248234,
   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/abs/0706.2283},
   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 = {fds248234}
}

@article{fds248235,
   Author = {Guillian, and G, and others},
   Title = {Observation of the anisotropy of 10-TeV primary cosmic ray
             nuclei flux with the Super-Kamiokande-I detector},
   Journal = {Phys. Rev. D},
   Volume = {74},
   Number = {6},
   Pages = {062003},
   Year = {2007},
   ISSN = {1550-7998},
   url = {http://arxiv.org/abs/astro-ph/0508468},
   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 = {fds248235}
}

@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{fds304612,
   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 = {fds304612}
}

@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{fds304611,
   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 = {fds304611}
}

@article{fds248103,
   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 = {fds248103}
}

@article{fds248120,
   Author = {Scholberg, K},
   Title = {Supernova neutrino detection},
   Journal = {NEUTRINO 2006 - Proceedings of the 22nd International
             Conference on Neutrino Physics and Astrophysics},
   Pages = {285-290},
   Year = {2006},
   Abstract = {The gravitational core collapse of a star produces a huge
             burst of neutrinos of all flavors. A number of detectors
             worldwide are sensitive to such a burst; its detection would
             yield information about both particle physics and
             astrophysics. Sensitivity to all flavors, and ability to tag
             different interactions will be key for extraction of
             information. Here I will survey the capabilities of current
             and future detectors for detection of supernova neutrinos
             from the Milky Way and beyond.},
   Key = {fds248120}
}

@article{fds248121,
   Author = {Scholberg, K},
   Title = {Prospects for measuring neutrino-nucleus coherent scattering
             at a stopped-pion neutrino source},
   Journal = {NEUTRINO 2006 - Proceedings of the 22nd International
             Conference on Neutrino Physics and Astrophysics},
   Pages = {476-},
   Year = {2006},
   Key = {fds248121}
}

@article{fds248179,
   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 = {fds248179}
}

@article{fds248180,
   Author = {White, RR and Allan, A and Barthelmy, S and Bloom, J and Graham, M and Hessman, FV and Marka, S and Rots, A and Scholberg, K and Seaman, R and Stoughton, C and Vestrand, WT and Williams, R and Wozniak,
             PR},
   Title = {Astronomical network event and observation
             notification},
   Journal = {Astronomische Nachrichten},
   Volume = {327},
   Number = {8},
   Pages = {775-778},
   Year = {2006},
   ISSN = {0004-6337},
   url = {http://dx.doi.org/10.1002/asna.200610631},
   Abstract = {Networks are becoming a key element in most current and all
             future, telescope and observatory projects. The ability to
             easily and efficiently pass observation data, alert data and
             instrumentation requests between distributed systems could
             enable science as never before. However, any effective large
             scale or meta-network of astronomical resources will require
             a common communication format or development resources will
             have to be continuously dedicated to creating interpreters.
             The necessary elements of any astronomy communication can be
             easily identified, efficiently described and rigidly
             formatted so that both robotic and human operations can use
             the same data. In this paper we will explore the current
             state of notification, what notification requirements are
             essential to create a successful standard and present a
             standard now under development by the International Virtual
             Observatory Alliance (IVOA), called the VOEvent. © 2006
             WILEY-VCH Verlag GmbH &amp; Co. KGaA.},
   Doi = {10.1002/asna.200610631},
   Key = {fds248180}
}

@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{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{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{fds248242,
   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},
   Key = {fds248242}
}

@article{fds248243,
   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 = {fds248243}
}

@article{Scholberg:2005qs,
   Author = {Scholberg, K},
   Title = {Prospects for measuring coherent neutrino-nucleus elastic
             scattering at a stopped-pion neutrino source},
   Journal = {Physical Review D - Particles, Fields, Gravitation, and
             Cosmology},
   Volume = {73},
   Number = {3},
   Pages = {033005},
   Year = {2006},
   ISSN = {1550-7998},
   url = {http://arxiv.org/pdf/hep-ex/0511042},
   Abstract = {Rates of coherent neutrino-nucleus elastic scattering at a
             high-intensity stopped-pion neutrino source in various
             detector materials (relevant for novel low-threshold
             detectors) are calculated. Sensitivity of a coherent
             neutrino-nucleus elastic scattering experiment to new
             physics is also explored. © 2006 The American Physical
             Society.},
   Doi = {10.1103/PhysRevD.73.033005},
   Key = {Scholberg:2005qs}
}

@article{fds287696,
   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},
   Year = {2006},
   ISSN = {1550-7998},
   url = {http://dx.doi.org/10.1103/PhysRevD.73.112001},
   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 = {fds287696}
}

@article{fds248244,
   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 = {fds248244}
}

@article{fds248248,
   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 = {fds248248}
}

@article{fds248176,
   Author = {Scholberg, K and Porco, C},
   Title = {Look up! [2] (multiple letters)},
   Journal = {Natural History},
   Volume = {114},
   Number = {1},
   Pages = {12-13},
   Year = {2005},
   Key = {fds248176}
}

@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.pdf},
   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{fds248249,
   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},
   Pages = {112005},
   Year = {2005},
   url = {http://arxiv.org/abs/hep-ex/0501064},
   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 = {fds248249}
}

@article{fds248250,
   Author = {Scholberg, K},
   Title = {Indirect dark matter searches with AMS-02},
   Journal = {Nuclear Physics B - Proceedings Supplements},
   Volume = {138},
   Number = {1-3},
   Pages = {35-37},
   Year = {2005},
   url = {http://dx.doi.org/10.1016/j.nuclphysbps.2004.11.007},
   Abstract = {AMS-02 is the main phase of the Alpha Magnetic Spectrometer
             experiment and is to be installed on the International Space
             Station for a three-year exposure. I will review the
             experiment, focusing on indirect dark matter detection
             capabilities. © 2004 Elsevier B.V. All rights
             reserved.},
   Doi = {10.1016/j.nuclphysbps.2004.11.007},
   Key = {fds248250}
}

@article{fds248251,
   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/abs/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 = {fds248251}
}

@article{fds30143,
   Author = {Back, H. and others},
   Title = {Report of the Solar and Atmospheric Working Group, APS
             Neutrino Study},
   Year = {2004},
   Month = {October},
   url = {http://www.hep.utexas.edu/sno/apsstudy/},
   Key = {fds30143}
}

@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, 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://arxiv.org/pdf/astro-ph/0305325},
   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 = {Aglietta:2003hq}
}

@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{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{fds248172,
   Author = {Battiston, R and Salamon, M and Katsavounidis, E and Scholberg,
             K},
   Title = {Editorial},
   Journal = {Nuclear Physics B - Proceedings Supplements},
   Volume = {134},
   Number = {1-3},
   Pages = {xxx},
   Year = {2004},
   url = {http://dx.doi.org/10.1016/S0920-5632(04)00332-9},
   Doi = {10.1016/S0920-5632(04)00332-9},
   Key = {fds248172}
}

@article{fds248173,
   Author = {Hauler, F and Bartoloni, A and Becker, U and Berges, P and Borgia, B and Bosi, C and Burger, J and Capell, M and Chung, CH and Boer, WD and Dömmecke, F and Fisher, P and Fopp, S and Gargiulo, C and Gentile, S and Henning, R and Jungermann, L and Karpinski, W and Kim, GN and Kirn, T and Kounine, A and Koutsenko, V and Lebedev, A and Lübelsmeyer, K and Monreal, B and Park, WH and Rapagnani, P and Schael, S and Schmanau, M and Scholberg, K and Schwering, G and Siedenburg, T and Wallraff, W and Son,
             D and Wlochal, M},
   Title = {The AMS-02 TRD for the international space
             station},
   Journal = {IEEE Transactions on Nuclear Science},
   Volume = {51},
   Number = {4 I},
   Pages = {1365-1372},
   Year = {2004},
   ISSN = {0018-9499},
   url = {http://dx.doi.org/10.1109/TNS.2004.832901},
   Abstract = {The Alpha Magnetic Spectrometer (AMS-02) is an experiment
             which will be mounted on the international space station
             (ISS) to measure primary cosmic ray spectra in space. A key
             element is the transition radiation detector (TRD) to
             extract an e+ or p- signal reducing the p+ or e- background
             by a rejection factor 102-103 in an energy range from 10 to
             300 GeV. This will be used in combination with an
             electromagnetic calorimeter to provide overall p+ rejection
             of 106 at 90% e+ efficiency. The detector consists of 20
             layers of 6 mm diameter straw tubes alternating with 20 mm
             layers of polyethylene/polypropylene fleece radiator. The
             tubes are filled with a 4:1 mixture of Xe:CO2 at 1 bar
             absolute pressure from a recirculating gas system designed
             to operate &gt;3 years in space. There are in total 5248
             straw tubes which are read out by a custom-made DAQ system
             in less than 80 μs. The electronics must be low in power
             consumption and sustain the stringent requirements of
             operation in space. The construction of the detector and its
             electronics is presented in this paper.},
   Doi = {10.1109/TNS.2004.832901},
   Key = {fds248173}
}

@article{Antonioli:2004zb,
   Author = {Antonioli, P and Fienberg, RT and Fleurot, F and Fukuda, Y and Fulgione,
             W and Habig, A and Heise, J and McDonald, AB and Mills, C and Namba, T and Robinson, LJ and Scholberg, K and Schwendener, M and Sinnott, RW and Stacey, B and Suzuki, Y and Tafirout, R and Vigorito, C and Viren, B and Virtue, C and Zichichi, A},
   Title = {SNEWS: The SuperNova Early Warning System},
   Journal = {New Journal of Physics},
   Volume = {6},
   Pages = {1-23},
   Year = {2004},
   url = {http://arxiv.org/abs/astro-ph/9911359v1},
   Abstract = {This paper provides a technical description of the SuperNova
             Early Warning System (SNEWS), an international network of
             experiments with the goal of providing an early warning of a
             galactic supernova.},
   Doi = {10.1088/1367-2630/6/1/114},
   Key = {Antonioli:2004zb}
}

@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{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{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}
}

@inproceedings{Scholberg:2003he,
   Author = {Scholberg, K.},
   Title = {Neutrino physics: Status and prospects},
   Year = {2003},
   url = {http://arxiv.org/pdf/hep-ex/0308011},
   Abstract = {http://arxiv.org/abs/hep-ex/0308011},
   Key = {Scholberg:2003he}
}

@article{fds248154,
   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},
   Year = {2003},
   ISSN = {0556-2821},
   url = {http://dx.doi.org/10.1103/PhysRevD.68.092002},
   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 = {fds248154}
}

@article{fds248156,
   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},
   Year = {2003},
   ISSN = {0556-2821},
   url = {http://dx.doi.org/10.1103/PhysRevD.67.042002},
   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 = {fds248156}
}

@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: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: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: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{fds248164,
   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 = {fds248164}
}

@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{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{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{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{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{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{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{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{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: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 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},
   ISSN = {1434-6044},
   url = {http://arxiv.org/pdf/hep-ex/0207020},
   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}
}

@inproceedings{Siedenburg:2002dn,
   Author = {Siedenburg, T and Chung, CH and Fopp, S and García, MF and Karpinski,
             W and Kirn, T and Lübelsmeyer, K and Orboeck, J and Schael, S and Dratzig,
             ASV and Schwering, G and Siedling, R and Wallraff, W and Becker, U and Berges, P and Burger, J and Fischer, P and Henning, R and Kounine, A and Koutsenko, V and Scholberg, K and Boer, WD and Hauler, F and Jungermann,
             L},
   Title = {A Transition Radiation Detector for AMS},
   Journal = {Nuclear Physics B - Proceedings Supplements},
   Volume = {113},
   Pages = {154-158},
   Year = {2002},
   url = {http://dx.doi.org/10.1016/S0920-5632(02)01835-2},
   Abstract = {For cosmic particle spectroscopy on the International Space
             Station the AMS experiment will be equipped with a
             Transition Radiation Detector to improve proton background
             supression up to 300 GeV. The TRD has 20 layers of fleece
             radiator with Xe/CO2 proportional-mode straw-tube chambers.
             They are supported in a conically shaped octagon structure
             made of CFC-Al-honeycomb. For low power consumption VA
             analog multiplexers are used as front-end readout. A 20
             layer prototype has achieved proton rejections above 100 at
             90% electron efficiency for beam energies up to 250 GeV. The
             detector is under construction at RWTH Aachen, the gas
             system will be built at MIT, slow-control and DAQ at TH
             Karlsruhe.},
   Doi = {10.1016/S0920-5632(02)01835-2},
   Key = {Siedenburg:2002dn}
}

@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{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{fds248142,
   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://dx.doi.org/10.1086/318281},
   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 = {fds248142}
}

@article{fds248143,
   Author = {Scholberg, K},
   Title = {Neutrino physics: An experimental overview},
   Journal = {International Journal of Modern Physics A},
   Volume = {16},
   Number = {SUPPL. 1A},
   Pages = {104-115},
   Year = {2001},
   ISSN = {0217-751X},
   url = {http://dx.doi.org/10.1142/S0217751X01006346},
   Abstract = {The field of neutrino physics is currently very exciting,
             with several recent results pointing to new physics. I will
             give an overview of the current experimental situation,
             focusing primarily on neutrino oscillation results. The data
             are not entirely consistent however, and puzzles remain. I
             will then review the new experiments which are poised to
             solve the outstanding puzzles.},
   Doi = {10.1142/S0217751X01006346},
   Key = {fds248143}
}

@article{fds248145,
   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 = {fds248145}
}

@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}
}

@inproceedings{Scholberg:2001bn,
   Author = {Scholberg Kate},
   Title = {Supernova neutrino detection at a future underground
             facility},
   Journal = {eConf},
   Volume = {C010630},
   Pages = {E605},
   Year = {2001},
   Key = {Scholberg:2001bn}
}

@booklet{Fukuda00,
   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 = {Fukuda00}
}

@booklet{Ambrosio00,
   Author = {Ambrosio, and M, and others},
   Title = {Search for lightly ionizing particles with the MACRO
             detector},
   Journal = {Phys. Rev. D},
   Volume = {6205},
   Number = {5},
   Pages = {art. no.-052003},
   Year = {2000},
   Month = {September},
   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 = {Ambrosio00}
}

@booklet{Ambrosio00b,
   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},
   Doi = {10.1016/S0370-2693(00)00267-7},
   Key = {Ambrosio00b}
}

@booklet{Ambrosio00a,
   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 De Benedictis and L and De Cataldo and G and Dekhissi, H and De Marzo and E and De Mitri and I and Derkaoui, J and De
             Vincenzi, M and Di Credico and A and Erriquez, O and Favuzzi, C and Forti,
             C and Fusco, P and Giacomelli, G et al.},
   Title = {Nuclearite search with the MACRO detector at Gran
             Sasso},
   Journal = {The European Physical Journal C - Particles and
             Fields},
   Volume = {13},
   Number = {3},
   Pages = {453-458},
   Year = {2000},
   Month = {April},
   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},
   Doi = {10.1007/s100520000142},
   Key = {Ambrosio00a}
}

@article{fds248138,
   Author = {Scholberg, K},
   Title = {Supernova neutrino detection},
   Journal = {Nuclear Physics B - Proceedings Supplements},
   Volume = {91},
   Number = {1-3},
   Pages = {331-337},
   Year = {2000},
   Abstract = {World-wide, several detectors currently running or neaxing
             completion are sensitive to a core collapse supernova
             neutrino signal in the Galaxy. I will briefly describe the
             nature of the neutrino signal and then survey current and
             future detection techniques. I will also explore what
             physics and astrophysics we can learn from the next Galactic
             core collapse.},
   Key = {fds248138}
}

@article{fds248140,
   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 = {fds248140}
}

@booklet{Suzuki00,
   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://dx.doi.org/10.1016/S0168-9002(00)00624-0},
   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 = {Suzuki00}
}

@article{fds304610,
   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},
   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 = {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.},
   Doi = {10.1103/PhysRevD.62.052003},
   Key = {fds304610}
}

@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}
}

@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},
   Series = {Section A- Accelerators, Spectrometers, Detectors and
             Associated Equipment},
   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},
   Series = {Proceedings Supplements},
   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{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{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{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{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{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{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}
}

@booklet{Kaneyuki99,
   Author = {Kaneyuki, K and Scholberg, K},
   Title = {Neutrino oscillations},
   Journal = {American scientist},
   Volume = {87},
   Number = {3},
   Pages = {222-231},
   Year = {1999},
   ISSN = {0003-0996},
   url = {http://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcApp=PARTNER_APP&SrcAuth=LinksAMR&KeyUT=WOS:000079671000014&DestLinkType=FullRecord&DestApp=ALL_WOS&UsrCustomerID=47d3190e77e5a3a53558812f597b0b92},
   Abstract = {Always elusive, Fermi's 'little neutral one' turns out to be
             a quick-change artist as well, offering answers and new
             questions for physics and cosmocology.},
   Key = {Kaneyuki99}
}

@article{fds304608,
   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 = {fds304608}
}

@article{fds304607,
   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 = {fds304607}
}

@article{fds304609,
   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 = {fds304609}
}

@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{fds248131,
   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 = {fds248131}
}

@article{fds248132,
   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 = {fds248132}
}

@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{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{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{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{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{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{Ambrosio97d,
   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, 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 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 = {High energy cosmic ray physics with the MACRO experiment at
             gran sasso},
   Journal = {Nuclear Physics B},
   Pages = {172-175},
   Year = {1997},
   Month = {February},
   ISSN = {0550-3213},
   url = {http://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcApp=PARTNER_APP&SrcAuth=LinksAMR&KeyUT=WOS:A1997WW40500032&DestLinkType=FullRecord&DestApp=ALL_WOS&UsrCustomerID=47d3190e77e5a3a53558812f597b0b92},
   Doi = {10.1016/S0920-5632(96)00869-9},
   Key = {Ambrosio97d}
}

@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)