Showing 1–18 of 18 results
/ Date/ Name
Mar 8, 2022Precision measurement of a brown dwarf mass in a binary system in the microlensing event OGLE-2019-BLG-0033/MOA-2019-BLG-035Apr 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 BoundaryAug 5, 2016Orbital alignment and starspot properties in the WASP-52 planetary systemMay 19, 2016Many new variable stars discovered in the core of the globular cluster NGC 6715 (M54) with EMCCD observationsMar 10, 2016High-resolution Imaging of Transiting Extrasolar Planetary systems (HITEP). I. Lucky imaging observations of 101 systems in the southern hemisphereJan 7, 2016Spitzer Observations of OGLE-2015-BLG-1212 Reveal a New Path to Breaking Strong Microlens DegeneraciesDec 17, 2015High-precision photometry by telescope defocussing. VIII. WASP-22, WASP-41, WASP-42 and WASP-55Nov 26, 2014Pathway to the Galactic Distribution of Planets: Combined Spitzer and Ground-Based Microlens Parallax Measurements of 21 Single-Lens EventsNov 11, 2014High-precision photometry by telescope defocussing. VII. The ultra-short period planet WASP-103Oct 31, 2014Searching for variable stars in the cores of five metal rich globular clusters using EMCCD observationsOct 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 ChannelOct 22, 2010Searching for Galactic hidden gas through interstellar scintillation: Results from a test with the NTT-SOFI detectorMay 6, 2010OGLE 2008--BLG--290: An accurate measurement of the limb darkening of a Galactic Bulge K Giant spatially resolved by microlensing