activity
20162021
most citedMicrolensing Results Challenge the Core Accretion Runaway Growth Scenario for Gas Giants

98 citations · 304 across the 18 of their papers we have counts for

collaborators

50 papers

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…

astro-ph.EP202112 cited

MOA-2006-BLG-074: recognizing xallarap contaminants in planetary microlensing

P. Rota, Y. Hirao, V. Bozza +23

MOA-2006-BLG-074 was selected as one of the most promising planetary candidates in a retrospective analysis of the MOA collaboration: its asymmetric high-magnification peak can be…

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

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…

astro-ph.EP2021

KMT-2019-BLG-0371 and the Limits of Bayesian Analysis

Yun Hak Kim, Sun-Ju Chung, Jennifer C. Yee +54

We show that the perturbation at the peak of the light curve of microlensing event KMT-2019-BLG-0371 is explained by a model with a mass ratio between the host star and planet of $…

astro-ph.EP2021

OGLE-2019-BLG-0960Lb: The Smallest Microlensing Planet

Jennifer C. Yee, Weicheng Zang, Andrzej Udalski +80

We report the analysis of OGLE-2019-BLG-0960, which contains the smallest mass-ratio microlensing planet found to date (q = 1.2--1.6 x 10^{-5} at 1-sigma). Although there is substa…