activity
20172024
most citedMOA-2016-BLG-227Lb: A Massive Planet Characterized by Combining Lightcurve Analysis and Keck AO Imaging

45 citations · 294 across the 21 of their papers we have counts for

collaborators

69 papers

astro-ph.EP20215 cited

OGLE-2019-BLG-0304: Competing Interpretations between a Planet-binary Model and a Binary-source + Binary-lens model

Cheongho Han, Andrzej Udalski, Chung-Uk Lee +31

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 ~days…

astro-ph.EP20218 cited

Kepler K2 Campaign 9: I. Candidate short-duration events from the first space-based survey for planetary microlensing

I. McDonald, E. Kerins, R. Poleski +6

We present the first short-duration candidate microlensing events from the Kepler K2 mission. From late April to early July 2016, Campaign 9 of K2 obtained high temporal cadence ob…

astro-ph.EP202111 cited

KMT-2018-BLG-1743: Planetary Microlensing Event Occurring on Two Source Stars

Cheongho Han, Michael D. Albrow, Sun-Ju Chung +18

We present the analysis of the microlensing event KMT-2018-BLG-1743. The light curve of the event, with a peak magnification , exhibits two anomaly features,…

astro-ph.EP2021

OGLE-2018-BLG-1185b : A Low-Mass Microlensing Planet Orbiting a Low-Mass Dwarf

Iona Kondo, Jennifer C. Yee, David P. Bennett +94

We report the analysis of planetary microlensing event OGLE-2018-BLG-1185, which was observed by a large number of ground-based telescopes and by the Space Telescope. The…

astro-ph.EP2021

Shortest Microlensing Event with a Bound Planet: KMT-2016-BLG-2605

Yoon-Hyun Ryu, Kyu-Ha Hwang, Andrew Gould +17

KMT-2016-BLG-2605, with planet-host mass ratio , has the shortest Einstein timescale, $t_\e = 3.41\pm 0.13\,$days, of any planetary microlensing event to date. Th…

astro-ph.EP2021

Three microlensing planets with no caustic-crossing features

Cheongho Han, Andrzej Udalski, Doeon Kim +31

We search for microlensing planets with signals exhibiting no caustic-crossing features, considering the possibility that such signals may be missed due to their weak and featurele…