▪ Abstract High-energy (>100 MeV) neutrino astrophysics enters an era of opportunity and
discovery as the sensitivity of detectors approaches astrophysically relevant flux levels. We …

As part of the European LAGUNA design study on a next-generation neutrino detector, we
propose the liquid-scintillator detector LENA (Low Energy Neutrino Astronomy) as a …

The announcement by the IceCube Collaboration of the observation of 28 cosmic neutrino
candidates has been greeted with a great deal of justified excitement. The data reported so …

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 …

KamLAND has measured the flux of ν e’s from distant nuclear reactors. We find fewer ν e
events than expected from standard assumptions about ν e propagation at the 99.95% CL In a …

… h period in which the observed neutrino burst was found came after our learning of the
detection of a neutrino signal by Hirata et al. at UT 7". 35. with an uncertainty of ~ 1 min. … J …

We present measurements of ν μ disappearance in K2K, the KEK to Kamioka long-baseline
neutrino oscillation experiment. One-hundred and twelve beam-originated neutrino events …

We present results of a study of neutrino oscillation based on a 766 ton/year exposure of
KamLAND to reactor antineutrinos. We observe 258 ν e candidate events with energies above …

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–…

The K2K experiment observes indications of neutrino oscillation: a reduction of ν μ flux together
with a distortion of the energy spectrum. Fifty-six beam neutrino events are observed in …