activity
20142021
most citedThe Unanticipated Phenomenology of the Blazar PKS~2131021: A Unique Super-Massive Black Hole Binary Candidate

79 citations · 806 across the 30 of their papers we have counts for

collaborators
Showing astro-ph.EPShow all

17 papers · 1 filter

astro-ph.EP2021

OGLE-2019-BLG-0468Lb,c: two microlensing giant planets around a G-type star

Cheongho Han, Andrzej Udalski, Chung-Uk Lee +37

With the aim of interpreting anomalous lensing events with no suggested models, we conducted a project of reinvestigating microlensing data in and before the 2019 season. In this w…

astro-ph.EP2021

Three faint-source microlensing planets detected via resonant-caustic channel

Cheongho Han, Andrzej Udalski, Doeon Kim +32

We conducted a project of reinvestigating the 2017--2019 microlensing data collected by the high-cadence surveys with the aim of finding planets that were missed due to the deviati…

astro-ph.EP2021★ 48 cited

Systematic KMTNet Planetary Anomaly Search, Paper II: Six New Mass-ratio Planets

Kyu-Ha Hwang, Weicheng Zang, Andrew Gould +62

We apply the automated AnomalyFinder algorithm of Paper I (Zang et al. 2021b) to 2018-2019 light curves from the covered by the six KMTNet prime fields, wi…

astro-ph.EP2021★ 18 cited

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…

astro-ph.EP2021★ 14 cited

KMT-2018-BLG-1025Lb: microlensing super-Earth planet orbiting a low-mass star

Cheongho Han, Andrzej Udalski, Chung-Uk Lee +32

We aim to find missing microlensing planets hidden in the unanalyzed lensing events of previous survey data. For this purpose, we conduct a systematic inspection of high-magnificat…

astro-ph.EP2020★ 13 cited

Four Microlensing Planets with Faint-source Stars Identified in the 2016 and 2017 Season Data

Cheongho Han, Andrzej Udalski, Doeon Kim +32

Microlensing planets occurring on faint source stars can escape detection due to their weak signals. Occasionally, detections of such planets are not reported due to the difficulty…