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OGLE, KMTNet & Spitzer EWS2017-BLG-1038 light curve
We report the analysis of microlensing event OGLE-2017-BLG-1038, observed by the Optical Gravitational Lensing Experiment, Korean Microlensing Telescope Network, and Spitzer... -
Systematic KMTNet Planetary Anomaly Search. II.
We apply the automated AnomalyFinder algorithm of Paper I to 2018-2019 light curves from the ~13deg^2^ covered by the six KMTNet prime fields, with cadences {Gamma}>~2/hr. We... -
R, I and L bands light curve of OGLE-2016-BLG-1093Lb
OGLE-2016-BLG-1093 is a planetary microlensing event that is part of the statistical Spitzer microlens parallax sample. The precise measurement of the microlens parallax effect... -
Prediction of microlensing events with Gaia EDR3
Astrometric microlensing is a unique tool to measure stellar masses. It allows us to determine the mass of the lensing star with an accuracy of a few percent. In this paper, we... -
I-band light curve of KMT-2016-BLG-2605 with KMTNet
With a planet-host mass ratio q=0.012{+/-}0.001, KMT-2016-BLG-2605 has the shortest Einstein timescale, tE=3.41{+/-}0.13days, of any planetary microlensing event to date. This... -
I-band light curve of OGLE-2019-BLG-1058 with KMTNet
We show that because the conditions for producing terrestrial microlens parallax (TPRX; i.e., a nearby disk lens) will also tend to produce a large lens-source relative proper... -
Photometry of OGLE-2019-BLG-0304 with OGLE & KMTNet
We analyze the microlensing event OGLE-2019-BLG-0304, whose light curve exhibits two distinctive features: a deviation in the peak region and a second bump appearing ~61days... -
Systematic KMTNet Planetary Anomaly Search. I.
In order to exhume the buried signatures of "missing planetary caustics" in Korea Microlensing Telescope Network (KMTNet) data, we conducted a systematic anomaly search of the... -
VRI photometry of MOA 2009-BLG-319
We present an adaptive optics (AO) analysis of images from the KeckII telescope NIRC2 instrument of the planetary microlensing event MOA-2009-BLG-319. The ~10yr baseline between... -
LCs of OGLE-2018-BLG-0567 and OGLE-2018-BLG-0962
We present the analyses of two microlensing events, OGLE-2018-BLG-0567 and OGLE-2018-BLG-0962. In both events, the short-lasting anomalies were densely and continuously covered... -
OGLE, MOA & KMTNet RI light curve of KMT-2019-BLG-1715
We investigate the gravitational microlensing event KMT-2019-BLG-1715, the light curve of which shows two short-term anomalies from a caustic-crossing binary-lensing light... -
I-band LC of the microlensing event KMT-2017-BLG-2820
We report a new free-floating planet (FFP) candidate, KMT-2017-BLG-2820, with Einstein radius {theta}E~6{mu}as, lens-source relative proper motion {mu}rel~8mas/yr, and Einstein... -
Optical and IR photometry of OGLE-2017-BLG-0406
We report the discovery and analysis of the planetary microlensing event OGLE-2017-BLG-0406, which was observed both from the ground and by the Spitzer satellite in a solar... -
KMTNet & OGLE I-band photometry of KMT-2019-BLG-0842
We report the discovery of a cold planet with a very low planet/host mass ratio of q=(4.09{+/-}0.27)x10^-5^, which is similar to the ratio of Uranus/Sun (q=4.37x10^-5^) in the... -
RI-band LC of microlensing event OGLE-2018-BLG-1269Lb
We report the discovery of a planet in the microlensing event OGLE-2018-BLG-1269 with a planet-host mass ratio q~6x10^-4^, i.e., 0.6 times smaller than the Jupiter/Sun mass... -
I-band LC of the microlensing event KMT-2016-BLG-1836
We report the discovery of a super-Jovian planet in the microlensing event KMT-2016-BLG-1836, which was found by the Korea Microlensing Telescope Network (KMTNet) high-cadence... -
OGLE/KMTnet VI bands photometry of OGLE-2019-BLG-0551
High-cadence observations of the Galactic bulge by the microlensing surveys led to the discovery of a handful of extremely short-timescale microlensing events that can be... -
LC of microlensing event OGLE-2012-BLG-0838
We present the discovery of a planet on a very wide orbit in the microlensing event OGLE-2012-BLG-0838. The signal of the planet is well separated from the main peak of the... -
Light curve of OGLE-2018-BLG-0677
We report the analysis of the microlensing event OGLE-2018-BLG-0677. A small feature in the light curve of the event leads to the discovery that the lens is a star-planet... -
I-band light curves of OGLE-2015-BLG-1771Lb
We report the discovery and the analysis of the short (t_E_<5days) planetary microlensing event, OGLE-2015-BLG-1771. The event was discovered by the Optical Gravitational...