activity
20112016
most citedIndication of Electron Neutrino Appearance from an Accelerator-produced Off-axis Muon Neutrino Beam

1.4k citations · 2.5k across the 7 of their papers we have counts for

collaborators

7 papers

hep-ex2016★ 302 cited

Solar Neutrino Measurements in Super-Kamiokande-IV

Kamiokande Collaboration, K. Abe, Y. Haga +167

Upgraded electronics, improved water system dynamics, better calibration and analysis techniques allowed Super-Kamiokande-IV to clearly observe very low-energy 8B solar neutrino in…

astro-ph.HE2016★ 91 cited

Real-Time Supernova Neutrino Burst Monitor at Super-Kamiokande

K. Abe, Y. Haga, Y. Hayato +124

We present a real-time supernova neutrino burst monitor at Super-Kamiokande (SK). Detecting supernova explosions by neutrinos in real time is crucial for giving a clear picture of…

hep-ex2014

Precise Measurement of the Neutrino Mixing Parameter θ_{23} from Muon Neutrino Disappearance in an Off-axis Beam

T2K Collaboration, K. Abe, J. Adam +338

New data from the T2K neutrino oscillation experiment produce the most precise measurement of the neutrino mixing parameter theta_{23}. Using an off-axis neutrino beam with a peak…

hep-ex2013★ 521 cited

Observation of Electron Neutrino Appearance in a Muon Neutrino Beam

K. Abe, J. Adam, H. Aihara +336

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…

hep-ex2013★ 98 cited

Measurement of Neutrino Oscillation Parameters from Muon Neutrino Disappearance with an Off-axis Beam

T2K collaboration, K. Abe, N. Abgrall +335

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 us…

hep-ex2013★ 170 cited

Evidence of Electron Neutrino Appearance in a Muon Neutrino Beam

T2K Collaboration, K. Abe, N. Abgrall +356

The T2K collaboration: reports evidence for electron neutrino appearance at the atmospheric mass splitting, |Δm_{32}^2|=2.4x10^{-3} eV^2. An excess of electron neutrino interaction…