Showing 21–40 of 116 results
/ Date/ Name
Apr 22, 2024Squeezing the quantum noise of a gravitational-wave detector below the standard quantum limitMar 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 27, 2023MedAlign: A Clinician-Generated Dataset for Instruction Following with Electronic Medical RecordsAug 7, 2023Search for Eccentric Black Hole Coalescences during the Third Observing Run of LIGO and VirgoMay 9, 2023Coronal Heating as Determined by the Solar Flare Frequency Distribution Obtained by Aggregating Case StudiesMar 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 detectorOct 26, 2022Accelerating Progress Towards Practical Quantum Advantage: The Quantum Technology Demonstration Project RoadmapOct 11, 2022The Future of High Energy Physics Software and ComputingJun 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 SummaryJan 3, 2022All-sky search for continuous gravitational waves from isolated neutron stars using Advanced LIGO and Advanced Virgo O3 dataNov 30, 2021All-sky search for gravitational wave emission from scalar boson clouds around spinning black holes in LIGO O3 dataNov 5, 2021GWTC-3: Compact Binary Coalescences Observed by LIGO and Virgo During the Second Part of the Third Observing Run