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20172021
most citedOGLE-2015-BLG-1771Lb: A Microlens Planet Orbiting an Ultracool Dwarf?

23 citations · 59 across the 4 of their papers we have counts for

collaborators

12 papers

astro-ph.IM202110 cited

Light Curve Calculations for Triple Microlensing Systems

Renkun Kuang, Shude Mao, Tianshu Wang +2

We present a method to compute the magnification of a finite source star lensed by a triple lens system based on the image boundary (contour integration) method. We describe a new…

astro-ph.EP201923 cited

OGLE-2015-BLG-1771Lb: A Microlens Planet Orbiting an Ultracool Dwarf?

Xiangyu Zhang, Weicheng Zang, Andrzej Udalski +31

We report the discovery and the analysis of the short (tE < 5 days) planetary microlensing event, OGLE-2015-BLG-1771. The event was discovered by the Optical Gravitational Lensing…

astro-ph.EP2019

KMT-2016-BLG-1836Lb: A Super-Jovian Planet From A High-Cadence Microlensing Field

Hongjing Yang, Xiangyu Zhang, Kyu-Ha Hwang +24

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's high-cadence observation…

astro-ph.EP2019

OGLE-2018-BLG-1011L\lowercase{b,c}: Microlensing Planetary System with Two Giant Planets Orbiting a Low-mass Star

Cheongho Han, David P. Bennett, Andrzej Udalski +70

We report a multiplanetary system found from the analysis of microlensing event OGLE-2018-BLG-1011, for which the light curve exhibits a double-bump anomaly around the peak. We fin…

astro-ph.EP2019

OGLE-2018-BLG-0532Lb: Cold Neptune With Possible Jovian Sibling

Yoon-Hyun Ryu, Andrzej Udalski, Jennifer C. Yee +34

We report the discovery of the planet OGLE-2018-BLG-0532Lb, with very obvious signatures in the light curve that lead to an estimate of the planet-host mass ratio $q=M_{\rm planet}…

astro-ph.EP201917 cited

Parallax of OGLE-2018-BLG-0596: A Low-mass-ratio Planet around an M-dwarf

Youn Kil Jung, Andrew Gould, Andrzej Udalski +63

We report the discovery of a microlensing planet OGLE-2018-BLG-0596Lb, with preferred planet-host mass ratio . The planetary signal, which is chara…