activity
20172023
most citedNo large population of unbound or wide-orbit Jupiter-mass planets

336 citations · 807 across the 31 of their papers we have counts for

collaborators

88 papers

astro-ph.GA2021

A Survey Length for AGN Variability Studies

Szymon Kozłowski

The damped random walk (DRW) process is one of the most commonly used and simplest stochastic models to describe variability of active galactic nuclei (AGN). An AGN light curve can…

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.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.SR202147 cited

Binarity as the Origin of Long Secondary Periods in Red Giant Stars

I. Soszyński, A. Olechowska, M. Ratajczak +13

Long secondary periods (LSPs), observed in a third of pulsating red giant stars, are the only unexplained type of large-amplitude stellar variability known at this time. Here we sh…

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…

astro-ph.EP2021

KMT-2019-BLG-1715: planetary microlensing event with three lens masses and two source stars

Cheongho Han, Andrzej Udalski, Doeone Kim +61

We investigate the gravitational microlensing event KMT-2019-BLG-1715, of which light curve shows two short-term anomalies from a caustic-crossing binary-lensing light curve: one w…