Showing 61–80 of 586 results
/ Date/ Name
Nov 7, 2024Laser initiated p-11B fusion reactions in petawatt high-repetition-rates laser facilitiesOct 29, 2024A wiggling filamentary jet at the origin of the blazar multi-wavelength behaviourOct 14, 2024New Limits for Existence of Transverse Zero Sound in Fermi Liquid 3HeOct 14, 2024Measurement of the double-differential cross section of muon-neutrino charged-current interactions with low hadronic energy in the NOvA Near DetectorSep 29, 2024Search for proton decay via $p\rightarrow{e^+η}$ and $p\rightarrow{μ^+η}$ with a 0.37 Mton-year exposure of Super-KamiokandeSep 26, 2024The track-length extension fitting algorithm for energy measurement of interacting particles in liquid argon TPCs and its performance with ProtoDUNE-SP dataAug 22, 2024DUNE Phase II: Scientific Opportunities, Detector Concepts, Technological SolutionsAug 13, 2024Measurement of neutrino oscillation parameters with the first six detection units of KM3NeT/ORCAAug 1, 2024First Measurement of the Total Inelastic Cross-Section of Positively-Charged Kaons on Argon at Energies Between 5.0 and 7.5 GeVJul 31, 2024A study in scarlet -- II. Spectroscopic properties of a sample of Intermediate Luminosity Red TransientsJul 14, 2024Supernova Pointing Capabilities of DUNEJun 12, 2024Jet modification via $π^0$-hadron correlations in Au$+$Au collisions at $\sqrt{s_{_{NN}}}=200$ GeVMay 21, 2024First joint oscillation analysis of Super-Kamiokande atmospheric and T2K accelerator neutrino dataMay 13, 2024JWST's PEARLS: resolved study of the stellar and dust components in starburst galaxies at cosmic noonApr 30, 2024Optical Spectroscopy of Type Ia Supernovae by the Carnegie Supernova Projects I and IIApr 16, 2024Maser Flares Driven by Isothermal Shock WavesApr 12, 2024Development of a data overflow protection system for Super-Kamiokande to maximize data from nearby supernovaeMar 26, 2024Optical variability of the blazar 3C 371: from minute to year timescalesMar 13, 2024Measurements of the charge ratio and polarization of cosmic-ray muons with the Super-Kamiokande detectorMar 12, 2024Second gadolinium loading to Super-Kamiokande