Showing 41–60 of 105 results
/ Date/ Name
Oct 13, 2023Open X-Embodiment: Robotic Learning Datasets and RT-X ModelsJul 28, 2023A search for new physics in low-energy electron recoils from the first LZ exposureJun 19, 2023Concept Extrapolation: A Conceptual PrimerJun 13, 2023Strong Interaction Physics at the Luminosity Frontier with 22 GeV Electrons at Jefferson LabMar 27, 2023Three Saturn-mass planets transiting F-type stars revealed with TESS and HARPSNov 30, 2022Background Determination for the LUX-ZEPLIN (LZ) Dark Matter ExperimentNov 22, 2022SPIn-NeRF: Multiview Segmentation and Perceptual Inpainting with Neural Radiance FieldsJul 8, 2022First Dark Matter Search Results from the LUX-ZEPLIN (LZ) ExperimentJul 2, 2022Relative permeability as a stationary process: energy fluctuations in immiscible displacementMay 23, 2022Precision Determination of the Neutral Weak Form Factor of $^{48}$CaMar 20, 2022Recognising the importance of preference change: A call for a coordinated multidisciplinary research effort in the age of AIMar 4, 2022A Next-Generation Liquid Xenon Observatory for Dark Matter and Neutrino PhysicsJan 8, 2022Cosmogenic production of $^{37}$Ar in the context of the LUX-ZEPLIN experimentDec 31, 2021First Determination of the 27Al Neutron Distribution Radius from a Parity-Violating Electron Scattering MeasurementNov 8, 2021New Measurements of the Beam-Normal Single Spin Asymmetry in Elastic Electron Scattering Over a Range of Spin-0 NucleiOct 25, 2021The young HD 73583 (TOI-560) planetary system: Two 10-M$_\oplus$ mini-Neptunes transiting a 500-Myr-old, bright, and active K dwarfJul 13, 2021TESS Data for Asteroseismology (T'DA) Stellar Variability Classification Pipeline: Set-Up and Application to the Kepler Q9 DataJun 1, 2021Search for dark matter annihilation signals from unidentified Fermi-LAT objects with H.E.S.SMay 5, 2021TESS and HARPS reveal two sub-Neptunes around TOI 1062Apr 26, 2021Projected sensitivity of the LUX-ZEPLIN (LZ) experiment to the two-neutrino and neutrinoless double beta decays of $^{134}$Xe