Showing 41–60 of 116 results
/ Date/ Name
Mar 19, 2019Masses and Distances of Planetary Microlens Systems with High Angular Resolution ImagingMar 19, 2019The Scientific Context of WFIRST Microlensing in the 2020sMar 5, 2020KMT-2019-BLG-1339L: an M Dwarf with a Giant Planet or a Companion Near the Planet/Brown Dwarf BoundaryJul 7, 2021Multiwavelength properties of MirasApr 13, 2021Three microlensing planets with no caustic-crossing featuresSep 29, 2021The OGLE Collection of Variable Stars. One Thousand Heartbeat Stars in the Galactic Bulge and Magellanic CloudsSep 15, 2021Three faint-source microlensing planets detected via resonant-caustic channelJul 24, 2017No large population of unbound or wide-orbit Jupiter-mass planetsMay 13, 2014OGLE-III Microlensing Events and the Structure of the Galactic BulgeMay 13, 2024KMT-2023-BLG-1866Lb: Microlensing super-Earth around an M dwarf hostJul 26, 2011A Southern Sky and Galactic Plane Survey for Bright Kuiper Belt ObjectsOct 5, 2015Interstellar Extinction Curve Variations Toward the Inner Milky Way: A Challenge to Observational CosmologyMay 29, 2025MOA-2022-BLG-091Lb and KMT-2024-BLG-1209Lb: Microlensing planets detected through weak caustic-crossing signalsAug 14, 2025Four binary microlenses with directly measured massesDec 31, 2025A free-floating-planet microlensing event caused by a Saturn-mass objectApr 9, 2026Candidate Microlensing Brown Dwarfs in Binary Lens Systems from the 2023--2025 Observing SeasonsJan 19, 2026A Newly Identified Degeneracy Keeps the Planetary Interpretation Viable for OGLE-2011-BLG-0950Feb 13, 2026KMT-2016-BLG-1337L: A Saturn-mass planet orbiting within a binary system of low-mass starsFeb 17, 2026Three Saturn-mass Microlensing Planets Identified through Signals from Peripheral-caustic PerturbationsMar 14, 2026Mass Production of 2023 KMTNet Microlensing Planets. II: Two Planets and A Brown Dwarf