Showing 1–20 of 84 results
/ Date/ Name
Apr 23, 2026Precision measurement of positron decay modes of Xe-125 in the LUX-ZEPLIN experimentApr 21, 2026On Fourier decay and the distance set problemMar 27, 2026Pushing the Limits of Pulse Shape Discrimination in a Large Liquid Xenon DetectorFeb 24, 2026Low-Energy Radon Backgrounds from Electrode Grids in Dual-Phase Xenon TPCsFeb 18, 2026Measurement of the Muon Flux at the Sanford Underground Research Facility with the LUX-ZEPLIN Dark Matter DetectorDec 10, 2025SN 2022ngb: A faint, slowly evolving Type IIb supernova with a low-mass envelopeDec 8, 2025Searches for Light Dark Matter and Evidence of Coherent Elastic Neutrino-Nucleus Scattering of Solar Neutrinos with the LUX-ZEPLIN (LZ) ExperimentNov 21, 2025Search for New Physics via Low-Energy Electron Recoils with a 4.2 Tonne\times Year Exposure from the LZ ExperimentNov 6, 2025Massive stars exploding in a He-rich circumstellar medium XII. SN 2024acyl: A fast, linearly declining Type Ibn supernova with early flash-ionisation featuresOct 23, 2025Detection of ultra-high-energy cosmic rays in the southern hemisphere with FAST: data acquisition and preliminary resultsOct 7, 2025Study of few-electron backgrounds in the LUX-ZEPLIN detectorOct 1, 2025Progress towards stereo observation of ultra-high-energy cosmic rays with Fluorescence detector Array of Single-pixel TelescopesSep 18, 2025Low-energy nuclear recoil calibration of the LUX-ZEPLIN experiment with a photoneutron sourceAug 26, 2025Flow-dependent tagging of $^{214}$Pb decays in the LZ dark matter detectorJul 17, 2025NSF-DOE Vera C. Rubin Observatory Observations of Interstellar Comet 3I/ATLAS (C/2025 N1)Jul 2, 2025Dangerous Questions in Astronomy EducationMay 11, 2025The competing effects of recent and long-term star formation histories on oxygen, nitrogen, and stellar metallicitiesMay 2, 2025Summary Report of the Physics Beyond Colliders Study at CERNMar 23, 2025New constraints on cosmic ray-boosted dark matter from the LUX-ZEPLIN experimentMar 7, 2025Measurements and models of enhanced recombination following inner-shell vacancies in liquid xenon