Showing 1–19 of 19 results
/ Date/ Name
Mar 16, 2026Cosmic ray mass composition measurement in the energy range from $10^{16.5}$ eV to $10^{18.5}$ eV observed with the TALE hybrid detectorJan 20, 2026The JEM-EUSO Collaboration: Contributions to the 39th International Cosmic Ray Conference (ICRC2025)Dec 1, 2025Searching for EeV photons with Telescope Array Surface Detector and neural networksJun 27, 2024Isotropy of cosmic rays beyond $10^{20}$ eV favors their heavy mass compositionJun 27, 2024Mass composition of ultra-high energy cosmic rays from distribution of their arrival directions with the Telescope ArrayJun 12, 2024Observation of Declination Dependence in the Cosmic Ray Energy SpectrumJan 15, 2024Nonproportionality of NaI(Tl) Scintillation Detector for Dark Matter Search ExperimentsNov 8, 2023Alpha backgrounds in NaI(Tl) crystals of COSINE-100Feb 28, 2023Monitoring of the polarized $H_{2}O$ maser emission around the massive protostars W75N(B)-VLA1 and W75N(B)-VLA2May 10, 2022First High-speed Video Camera Observations of a Lightning Flash Associated with a Downward Terrestrial Gamma-ray FlashJan 18, 2022Search for Spatial Correlations of Neutrinos with Ultra-High-Energy Cosmic RaysNov 18, 2021Observation of Variations in Cosmic Ray Single Count Rates During Thunderstorms and Implications for Large-Scale Electric Field ChangesOct 28, 2021Indications of a Cosmic Ray Source in the Perseus-Pisces SuperclusterMar 1, 2021Surface detectors of the TAx4 experimentJun 30, 2020Search for Large-scale Anisotropy on Arrival Directions of Ultra-high-energy Cosmic Rays Observed with the Telescope Array ExperimentJun 9, 2020Measurement of the Proton-Air Cross Section with Telescope Array's Black Rock Mesa and Long Ridge Fluorescence Detectors, and Surface Array in Hybrid ModeMay 15, 2020Evidence for a Supergalactic Structure of Magnetic Deflection Multiplets of Ultra-High Energy Cosmic RaysJan 24, 2018Evidence for Declination Dependence of the Ultrahigh Energy Cosmic Ray Spectrum in the Northern HemisphereNov 18, 2016Physics Potentials with the Second Hyper-Kamiokande Detector in Korea