Showing 641–660 of 1,045 results
/ Date/ Name
Jun 21, 2019A super-Earth and sub-Neptune transiting the late-type M dwarf LP 791-18Jun 4, 2019BlueMUSE: Project Overview and Science CasesMay 29, 2019Reinforcement Learning for Slate-based Recommender Systems: A Tractable Decomposition and Practical MethodologyMay 16, 2019Electron Densities and Nitrogen Abundances in Ionized Gas Derived Using [NII] Fine-structure and Hydrogen Recombination linesMay 14, 2019Quasi-elastic polarization-transfer measurements on the deuteron in anti-parallel kinematicsMay 7, 2019Regulation of accretion by its outflow in a symbiotic star: the 2016 outflow fast state of MWC 560Apr 24, 2019Spectral Variability of a Sample of Extreme Variability Quasars and Implications for the MgII Broad-line RegionApr 18, 2019Performance of the Gemini Planet Imager Non-Redundant Mask and spectroscopy of two close-separation binaries HR 2690 and HD 142527Apr 9, 2019The Detailed Science Case for the Maunakea Spectroscopic Explorer, 2019 editionApr 9, 2019Context-Aware Query Selection for Active Learning in Event RecognitionMar 30, 2019The molecular-gas properties in the gravitationally lensed merger HATLAS J142935.3-002836Mar 28, 2019Measurement of the cross section for hard exclusive $π^0$ leptoproductionMar 21, 2019The ALMA Spectroscopic Survey in the HUDF: Nature and physical properties of gas-mass selected galaxies using MUSE spectroscopyMar 21, 2019Towards Standardization of Data Licenses: The Montreal Data LicenseMar 19, 2019Supermassive Black-hole Demographics & Environments With Pulsar Timing ArraysMar 14, 2019Astro2020 Science White Paper: First Stars and Black Holes at Cosmic Dawn with Redshifted 21-cm ObservationsMar 13, 2019Opportunities for Astrophysical Science from the Inner and Outer Solar SystemMar 13, 2019Convection in a volatile nitrogen-ice-rich layer drives Pluto's geological vigorMar 12, 2019Messengers from the Early Universe: Cosmic Neutrinos and Other Light RelicsMar 11, 2019The US Program in Ground-Based Gravitational Wave Science: Contribution from the LIGO Laboratory