Showing 21–40 of 73 results
/ Date/ Name
Mar 12, 2024Search for $CP$-Violating Neutrino Nonstandard Interactions with the NOvA ExperimentMar 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 2, 2022Identification and reconstruction of low-energy electrons in the ProtoDUNE-SP detectorJul 13, 2022Improved measurement of the $0_2^+\rightarrow0_1^+$ E0 transition strength for $^{72}$Se using the SPICE spectrometerJun 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 SummaryAug 18, 2021An Improved Measurement of Neutrino Oscillation Parameters by the NOvA ExperimentJan 12, 2021Spectro-Timing Analysis of a highly variable narrow-line Seyfert 1 galaxy NGC 4748 with AstroSat and XMM-NewtonSep 10, 2020Search for Slow Magnetic Monopoles with the NOvA Detector on the SurfaceMay 28, 2020Measurement of jet-medium interactions via direct photon-hadron correlations in Au$+$Au and $d$$+$Au collisions at $\sqrt{s_{_{NN}}}=200$ GeVJun 12, 2019First measurement of neutrino oscillation parameters using neutrinos and antineutrinos by NOvAMay 10, 2018Beam-energy and centrality dependence of direct-photon emission from ultra-relativistic heavy-ion collisionsMar 5, 2018Measurement of two-particle correlations with respect to second- and third-order event planes in Au$+$Au collisions at $\sqrt{s_{_{NN}}}=200$ GeV