Showing 1–19 of 19 results
/ Date/ Name
Oct 20, 2014The origin of the atomic and molecular gas contents of early-type galaxies. II. Misaligned gas accretionNov 21, 2025Search for New Physics via Low-Energy Electron Recoils with a 4.2 Tonne\times Year Exposure from the LZ ExperimentJan 17, 2020Do model emission line galaxies live in filaments at z~1?Jan 9, 20203\%-accurate predictions for the clustering of dark matter, haloes and subhaloes, over a wide range of cosmologies and scalesAug 25, 2017The host dark matter halos of [OII] emitters at 0.5< z< 1.5Jul 20, 2016The evolution of the galaxy content of dark matter haloesApr 23, 2026Precision measurement of positron decay modes of Xe-125 in the LUX-ZEPLIN experimentSep 18, 2025Low-energy nuclear recoil calibration of the LUX-ZEPLIN experiment with a photoneutron sourceMar 27, 2026Pushing the Limits of Pulse Shape Discrimination in a Large Liquid Xenon DetectorMar 11, 2022Large inverted band-gap in strained three-layer InAs/GaInSb quantum wellsJul 27, 2022The cosmology dependence of the concentration-mass-redshift relationFeb 23, 2015The galaxy - dark matter halo connection: which galaxy properties are correlated with the host halo mass?May 9, 2017Angular momentum evolution in Dark Matter haloes: a study of the Bolshoi and Millennium simulationsOct 7, 2025Study of few-electron backgrounds in the LUX-ZEPLIN detectorFeb 24, 2026Low-Energy Radon Backgrounds from Electrode Grids in Dual-Phase Xenon TPCsDec 8, 2025Searches for Light Dark Matter and Evidence of Coherent Elastic Neutrino-Nucleus Scattering of Solar Neutrinos with the LUX-ZEPLIN (LZ) ExperimentJan 17, 2020The better half -- Asymmetric star-formation due to ram pressure in the EAGLE simulationsFeb 18, 2026Measurement of the Muon Flux at the Sanford Underground Research Facility with the LUX-ZEPLIN Dark Matter DetectorApr 26, 2013KAPAO: a MEMS-based natural guide star adaptive optics system