Showing 1–20 of 35 results
/ Date/ Name
Dec 25, 2024Quality Assurance and Quality Control of the $26~\text{m}^2$ SiPM production for the DarkSide-20k dark matter experimentSep 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 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 DUNEMar 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 ReportMar 29, 2023Impact of cross-section uncertainties on supernova neutrino spectral parameter fitting in the Deep Underground Neutrino ExperimentDec 19, 2022Highly-parallelized simulation of a pixelated LArTPC on a GPUNov 9, 2022Updated constraints on sterile neutrino mixing in the OPERA experiment using a new $ν_e$ identification methodNov 2, 2022Identification and reconstruction of low-energy electrons in the ProtoDUNE-SP detectorJun 29, 2022Reconstruction of interactions in the ProtoDUNE-SP detector with PandoraMar 31, 2022Separation of track- and shower-like energy deposits in ProtoDUNE-SP using a convolutional neural networkMar 30, 2022Scintillation light detection in the 6-m drift-length ProtoDUNE Dual Phase liquid argon TPCMar 11, 2022A Gaseous Argon-Based Near Detector to Enhance the Physics Capabilities of DUNEMar 11, 2022Snowmass Neutrino Frontier: DUNE Physics SummaryJul 19, 2021Searching for solar KDAR with DUNEJan 22, 2020Design and construction of a new detector to measure ultra-low radioactive-isotope contamination of argonDec 23, 2019First observation of a tau neutrino charged current interaction with charm production in the Opera experiment