Showing 21–40 of 111 results
/ Date/ Name
Mar 30, 2025The DUNE Science ProgramFeb 23, 2025Constraining the Cosmic-ray Energy Based on Observations of Nearby Galaxy Clusters by LHAASOFeb 10, 2025Neutrino Interaction Vertex Reconstruction in DUNE with Pandora Deep LearningOct 17, 2024Measurement of attenuation length of the muon content in extensive air showers from 0.3 to 30 PeV with LHAASOSep 26, 2024The track-length extension fitting algorithm for energy measurement of interacting particles in liquid argon TPCs and its performance with ProtoDUNE-SP dataSep 14, 2024Deep view of Composite SNR CTA1 with LHAASO in $γ$-rays up to 300 TeVAug 22, 2024DUNE Phase II: Scientific Opportunities, Detector Concepts, Technological SolutionsAug 19, 2024Observation of the $γ$-ray Emission from W43 with LHAASOAug 1, 2024First Measurement of the Total Inelastic Cross-Section of Positively-Charged Kaons on Argon at Energies Between 5.0 and 7.5 GeVJul 14, 2024Supernova Pointing Capabilities of DUNEJun 12, 2024Jet modification via $π^0$-hadron correlations in Au$+$Au collisions at $\sqrt{s_{_{NN}}}=200$ GeVMay 24, 2024Searches for new physics below twice the electron mass with GERDAMar 5, 2024Performance of a modular ton-scale pixel-readout liquid argon time projection chamberFeb 2, 2024Doping Liquid Argon with Xenon in ProtoDUNE Single-Phase: Effects on Scintillation LightDec 5, 2023The DUNE Far Detector Vertical Drift Technology, Technical Design ReportAug 26, 2023Measurement of the Gamma-Ray Energy Spectrum beyond 100 TeV from the HESS J1843$-$033 RegionAug 7, 2023Search for Eccentric Black Hole Coalescences during the Third Observing Run of LIGO and VirgoMar 29, 2023Impact of cross-section uncertainties on supernova neutrino spectral parameter fitting in the Deep Underground Neutrino ExperimentFeb 28, 2023JWST-TST Proper Motions: I. High-Precision NIRISS Calibration and Large Magellanic Cloud KinematicsJan 31, 2023Combining the CLAUDS & HSC-SSP surveys: U+grizy(+YJHKs) photometry and photometric redshifts for 18M galaxies in the 20 deg2 of the HSC-SSP Deep and ultraDeep fields