Showing 1–20 of 20 results
/ Date/ Name
Jan 18, 2024Improving the light curves of gravitationally lensed quasars with Gaia proper motion dataSep 7, 2023Gaia22dkvLb: A Microlensing Planet Potentially Accessible to Radial-Velocity CharacterizationApr 5, 2021OGLE-2018-BLG-1185b : A Low-Mass Microlensing Planet Orbiting a Low-Mass DwarfOct 27, 2017OGLE-2016-BLG-1190Lb: First Spitzer Bulge Planet Lies Near the Planet/Brown-Dwarf BoundarySep 21, 2016The First Circumbinary Planet Found by Microlensing: OGLE-2007-BLG-349L(AB)cAug 26, 2015Spitzer Microlens Measurement of a Massive Remnant in a Well-Separated BinaryNov 26, 2014Pathway to the Galactic Distribution of Planets: Combined Spitzer and Ground-Based Microlens Parallax Measurements of 21 Single-Lens EventsDec 13, 2013A Sub-Earth-Mass Moon Orbiting a Gas Giant Primary or a High Velocity Planetary System in the Galactic BulgeOct 9, 2013A Super-Jupiter orbiting a late-type star: A refined analysis of microlensing event OGLE-2012-BLG-0406Sep 30, 2013MOA-2010-BLG-328Lb: a sub-Neptune orbiting very late M dwarf ?Nov 16, 2012MOA-2010-BLG-073L: An M-Dwarf with a Substellar Companion at the Planet/Brown Dwarf BoundaryApr 13, 2012Characterizing Low-Mass Binaries From Observation of Long Time-scale Caustic-crossing Gravitational Microlensing EventsSep 15, 2011Microlensing Binaries Discovered through High-Magnification ChannelApr 27, 2011OGLE-2005-BLG-018: Characterization of Full Physical and Orbital Parameters of a Gravitational Binary LensMay 6, 2010OGLE 2008--BLG--290: An accurate measurement of the limb darkening of a Galactic Bulge K Giant spatially resolved by microlensingJul 20, 2009Mass measurement of a single unseen star and planetary detection efficiency for OGLE 2007-BLG-050Feb 20, 2008The time-delay of the gravitationally lensed double quasar UM 673Sep 11, 2006OGLE 2004-BLG-254: a K3 III Galactic Bulge Giant spatially resolved by a single microlensMay 24, 2005Microlensing in the double quasar SBS1520+530Jan 7, 2004Probing the atmosphere of the bulge G5III star OGLE-2002-BUL-069 by analysis of microlense H alpha line