Showing 1–20 of 20 results
/ Date/ Name
Oct 22, 2025Joint neutrino oscillation analysis from the T2K and NOvA experimentsSep 9, 2025Measurement of muon neutrino induced charged current interactions without charged pions in the final state using a new T2K off-axis near detector WAGASCI-BabyMINDJul 2, 2025Testing T2K's Bayesian constraints with priors in alternate parameterisationsJun 6, 2025Results from the T2K experiment on neutrino mixing including a new far detector $μ$-like sampleMay 28, 2025First measurement of neutron capture multiplicity in neutrino-oxygen neutral-current quasi-elastic-like interactions using an accelerator neutrino beamMay 1, 2025First Measurement of the Electron Neutrino Charged-Current Pion Production Cross Section on Carbon with the T2K Near DetectorMar 10, 2025Signal selection and model-independent extraction of the neutrino neutral-current single $π^+$ cross section with the T2K experimentMay 21, 2024First joint oscillation analysis of Super-Kamiokande atmospheric and T2K accelerator neutrino dataAug 31, 2023Measurements of the $ν_μ$ and $\barν_μ$-induced Coherent Charged Pion Production Cross Sections on $^{12}C$ by the T2K experimentMar 6, 2023Measurements of neutrino oscillation parameters from the T2K experiment using $3.6\times10^{21}$ protons on targetSep 21, 2022Multiple Coulomb Scattering of muons in Lithium HydrideJun 10, 2021Performance of the MICE diagnostic systemSep 2, 2020The Hyper-Kamiokande Experiment -- Snowmass LOIApr 11, 2020Simultaneous measurement of the muon neutrino charged-current cross section on oxygen and carbon without pions in the final state at T2KJul 19, 2019First demonstration of ionization cooling by the Muon Ionization Cooling ExperimentAug 30, 2017NEOWISE Reactivation Mission Year Three: Asteroid Diameters and AlbedosJan 23, 2017Design and expected performance of the MICE demonstration of ionization coolingNov 2, 2015Pion contamination in the MICE muon beamOct 28, 2015Electron-Muon Ranger: performance in the MICE Muon BeamSep 25, 2012Preliminary Analysis of WISE/NEOWISE 3-Band Cryogenic and Post-Cryogenic Observations of Main Belt Asteroids