activity
20152022
most citedMicrolensing Results Challenge the Core Accretion Runaway Growth Scenario for Gas Giants

98 citations · 613 across the 33 of their papers we have counts for

collaborators

71 papers

astro-ph.SR20229 cited

Brown-dwarf companions in microlensing binaries detected during the 2016--2018 seasons

Cheongho Han, Yoon-Hyun Ryu, In-Gu Shin +60

With the aim of finding microlensing binaries containing brown-dwarf (BD) companions, we investigate the microlensing survey data collected during the 2016--2018 seasons. For this…

astro-ph.EP20224 cited

OGLE-2016-BLG-1093Lb: A Sub-Jupiter-mass Spitzer Planet Located in Galactic Bulge

In-Gu Shin, Jennifer C. Yee, Kyu-Ha Hwang +61

OGLE-2016-BLG-1093 is a planetary microlensing event that is part of the statistical microlens parallax sample. The precise measurement of the microlens parallax effect f…

astro-ph.EP202180 cited

A Jovian analogue orbiting a white dwarf star

J. W. Blackman, J-P. Beaulieu, D. P. Bennett +13

Studies have shown that remnants of destroyed planets and debris-disk planetesimals can survive the volatile evolution of their host stars into white dwarfs, but detection of intac…

astro-ph.EP202120 cited

No Large Dependence of Planet Frequency on Galactocentric Distance

Naoki Koshimoto, David P. Bennett, Daisuke Suzuki +1

Gravitational microlensing is currently the only technique that helps study the Galactic distribution of planets as a function of distance from the Galactic center. The Galactic lo…

astro-ph.EP20213 cited

OGLE-2017-BLG-1434Lb: Confirmation of a Cold Super-Earth using Keck Adaptive Optics

J. W. Blackman, J. -P. Beaulieu, A. A. Cole +5

The microlensing event OGLE-2017-BLG-1434 features a cold super-Earth planet which is one of eleven microlensing planets with a planet-host star mass ratio .…

astro-ph.EP20211 cited

New Giant Planet beyond the Snow Line for an Extended MOA Exoplanet Microlens Sample

Clément Ranc, David P. Bennett, Richard K. Barry +28

Characterizing a planet detected by microlensing is hard if the planetary signal is weak or the lens-source relative trajectory is far from caustics. However, statistical analyses…