Showing 21–40 of 44 results
/ Date/ Name
Aug 13, 2024Measurement of neutrino oscillation parameters with the first six detection units of KM3NeT/ORCAApr 12, 2024Development of a data overflow protection system for Super-Kamiokande to maximize data from nearby supernovaeMar 13, 2024Measurements of the charge ratio and polarization of cosmic-ray muons with the Super-Kamiokande detectorJan 22, 2024Citizen Science for IceCube: Name that NeutrinoNov 7, 2023Searches for neutrino counterparts of gravitational waves from the LIGO/Virgo third observing run with KM3NeTOct 26, 2023Ready for O4 II: GRANDMA Observations of Swift GRBs during eight-weeks of Spring 2022Sep 21, 2023Search for Continuous and Transient Neutrino Emission Associated with IceCube's Highest-Energy Tracks: An 11-Year AnalysisAug 31, 2023Measurements of the $ν_μ$ and $\barν_μ$-induced Coherent Charged Pion Production Cross Sections on $^{12}C$ by the T2K experimentMar 23, 2023Search for neutrino lines from dark matter annihilation and decay with IceCubeMar 6, 2023Measurements of neutrino oscillation parameters from the T2K experiment using $3.6\times10^{21}$ protons on targetFeb 15, 2023Search for neutrino counterparts to the gravitational wave sources from LIGO/Virgo O3 run with the ANTARES detectorDec 22, 2022Hint for a TeV neutrino emission from the Galactic Ridge with ANTARESDec 13, 2022A Search for Coincident Neutrino Emission from Fast Radio Bursts with Seven Years of IceCube Cascade EventsJul 20, 2022The GRANDMA network in preparation for the fourth gravitational-wave observing runJul 1, 2021Sensitivity to light sterile neutrino mixing parameters with KM3NeT/ORCAMar 17, 2021Determining the Neutrino Mass Ordering and Oscillation Parameters with KM3NeT/ORCAFeb 11, 2021The KM3NeT potential for the next core-collapse supernova observation with neutrinosDec 4, 2020Neutron-Antineutron Oscillation Search using a 0.37 Megaton$\cdot$Year Exposure of Super-KamiokandeSep 2, 2020The Hyper-Kamiokande Experiment -- Snowmass LOIMay 11, 2020Indirect Search for Dark Matter from the Galactic Center and Halo with the Super-Kamiokande Detector