activity
19992026
most citedIndication of Electron Neutrino Appearance from an Accelerator-produced Off-axis Muon Neutrino Beam

1.4k citations · 9.9k across the 99 of their papers we have counts for

collaborators

100 papers

hep-ex2026

Measurement of reconstructed final-state kinematics in charged-current interactions on water using the J-PARC beam and NINJA emulsion detector

NINJA Collaboration, A. Kasumi, S. Han +50

We present a study of charged-particle multiplicities and the kinematic distributions of muons, protons, and charged pions in a flux-integrated sample of charged-current inclusive…

astro-ph.HE2022★ 4 cited

A search for correlated low-energy electron antineutrinos in KamLAND with gamma-ray bursts

S. Abe, S. Asami, A. Gando +64

We present the results of a time-coincident event search for low-energy electron antineutrinos in the KamLAND detector with gamma-ray bursts from the Gamma-ray Coordinates Network…

physics.ins-det2021★ 5 cited

Wide angle acceptance and high-speed track recognition in nuclear emulsion

Y. Suzuki, T. Fukuda, H. Kawahara +5

A nuclear emulsion film is a three-dimensional tracking device that is widely used in cosmic-ray and high energy physics experiments. Scanning with a wide angle acceptance is cruci…

hep-ex2021★ 6 cited

New Methods and Simulations for Cosmogenic Induced Spallation Removal in Super-Kamiokande-IV

Kamiokande Collaboration, S. Locke, A. Coffani +215

Radioactivity induced by cosmic muon spallation is a dominant source of backgrounds for MeV neutrino interactions in water Cherenkov detectors. In particular, it…

physics.ins-det2021★ 1 cited

First Gadolinium Loading to Super-Kamiokande

K. Abe, C. Bronner, Y. Hayato +212

In order to improve Super-Kamiokande's neutron detection efficiency and to thereby increase its sensitivity to the diffuse supernova neutrino background flux, 13 tons of $\rm Gd_2(…

astro-ph.HE2021★ 44 cited

Limits on astrophysical antineutrinos with the KamLAND experiment

S. Abe, S. Asami, A. Gando +66

We report on a search for electron antineutrinos () from astrophysical sources in the neutrino energy range 8.3 to 30.8 MeV with the KamLAND detector. In an exposure of 6.…