Showing 21–40 of 56 results
/ Date/ Name
Jun 27, 2024PathAlign: A vision-language model for whole slide images in histopathologyMar 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 ReportMay 9, 2023Coronal Heating as Determined by the Solar Flare Frequency Distribution Obtained by Aggregating Case StudiesMay 5, 2023A Race Track Trapped-Ion Quantum ProcessorMar 29, 2023Impact of cross-section uncertainties on supernova neutrino spectral parameter fitting in the Deep Underground Neutrino ExperimentOct 10, 2022Kinetic Simulations Verifying Reconnection Rates Measured in the Laboratory, Spanning the Ion-Coupled to Near Electron-Only RegimesJun 26, 2022Sensitivity of the GAPS Experiment to Low-energy Cosmic-ray AntiprotonsJan 19, 2022Cold Atoms in Space: Community Workshop Summary and Proposed Road-MapAug 18, 2021An Improved Measurement of Neutrino Oscillation Parameters by the NOvA ExperimentJun 13, 2021Laboratory verification of electron-scale reconnection regions modulated by a three-dimensional instabilityApr 5, 2021Regulation of the Normalized Rate of Driven Magnetic Reconnection through Shocked Flux PileupJan 18, 2021Probing the capability of future direct imaging missions to spectrally constrain the frequency of Earth-like planetsSep 10, 2020Search for Slow Magnetic Monopoles with the NOvA Detector on the SurfaceAug 10, 2020Non-detection of O$_2$/O$_3$ informs frequency of Earth-like planets with LUVOIR but not HabExJun 12, 2019First measurement of neutrino oscillation parameters using neutrinos and antineutrinos by NOvADec 19, 2018Multivariate one-sided testing in matched observational studies as an adversarial gameFeb 24, 2017Dark Matter Search Results from the PICO-60 C$_3$F$_8$ Bubble Chamber