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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... -
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... -
SDSS Quasar Lens Search. V. Final catalog
We present the final statistical sample of lensed quasars from the Sloan Digital Sky Survey (SDSS) Quasar Lens Search (SQLS). The well-defined statistical lens sample consists... -
SDSS Quasar Lens Search. IV.
We present the second report of our systematic search for strongly lensed quasars from the data of the Sloan Digital Sky Survey (SDSS). From extensive follow-up observations of... -
SDSS quasar lens search. II.
We report the first results of our systematic search for strongly lensed quasars using the spectroscopically confirmed quasars in the Sloan Digital Sky Survey (SDSS). Among... -
Gravitational lenses among z>=4.0 quasars
We report on i-band snapshot observations of 157 Sloan Digital Sky Survey quasars at 4.0 -
Predicted Microlensing Events by nearby VLM objects
Microlensing events can be used to directly measure the masses of single field stars to a precision of ~1-10%. The majority of direct mass measurements for stellar and... -
Predicted Microlensing Events for the 21st Century
Using Gaia data release 2 (GDR2, Cat. I/345), we present an almanac of 2509 predicted microlensing events, caused by 2130 unique lens stars, that will peak between July 25, 2026... -
OGLE-II DIA microlensing events
We present a sample of microlensing events discovered in the Difference Image Analysis (DIA) of the OGLE-II images collected during three observing seasons, 1997-1999. 4424... -
OGLE-II DIA BUL_SC1 field
We present an implementation of the difference image photometry based on the Alard and Lupton optimal PSF matching algorithm. The most important feature distinguishing this...
