Showing 121–140 of 264 results
/ Date/ Name
Feb 16, 2018Projected WIMP sensitivity of the LUX-ZEPLIN (LZ) dark matter experimentJan 8, 2018The Astropy Project: Building an inclusive, open-science project and status of the v2.0 core packageNov 29, 2017Astrophysical S-factor of the $^{14}\textrm{N(p,}γ\textrm{)}^{15}\textrm{O}$ reaction at 0.4 -- 1.3\,MeVOct 16, 2017Search for High-energy Neutrinos from Binary Neutron Star Merger GW170817 with ANTARES, IceCube, and the Pierre Auger ObservatoryOct 16, 2017A gravitational-wave standard siren measurement of the Hubble constantSep 6, 2017The Large Enriched Germanium Experiment for Neutrinoless Double Beta Decay (LEGEND)Sep 5, 2017The wind and the magnetospheric accretion onto the T Tauri star S Coronae Australis at sub-au resolutionMay 13, 2017White Paper on East Asian Vision for mm/submm VLBI: Toward Black Hole Astrophysics down to Angular Resolution of 1~R$_{S}$May 9, 2017Limits on spin-dependent WIMP-nucleon cross section obtained from the complete LUX exposureApr 19, 2017The Hyper Suprime-Cam SSP Survey: Overview and Survey DesignApr 7, 2017First Searches for Axions and Axion-Like Particles with the LUX ExperimentMar 27, 2017LUX-ZEPLIN (LZ) Technical Design ReportFeb 8, 2017Identification of Radiopure Titanium for the LZ Dark Matter Experiment and Future Rare Event SearchesOct 6, 2016Signal yields, energy resolution, and recombination fluctuations in liquid xenonAug 27, 2016Results from a search for dark matter in the complete LUX exposureAug 18, 2016Low-energy (0.7-74 keV) nuclear recoil calibration of the LUX dark matter experiment using D-D neutron scattering kinematicsJul 19, 2016Ideal charge density wave order in the high-field state of superconducting YBCOJun 13, 2016Supplement: The Rate of Binary Black Hole Mergers Inferred from Advanced LIGO Observations Surrounding GW150914Jun 3, 2016Directly comparing GW150914 with numerical solutions of Einstein's equations for binary black hole coalescenceMay 30, 2016AMiBA: Cluster Sunyaev-Zel'dovich Effect Observations with the Expanded 13-Element Array