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20062021
most citedOGLE-2017-BLG-0173Lb: Low Mass-Ratio Planet in a "Hollywood" Microlensing Event

35 citations · 134 across the 7 of their papers we have counts for

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astro-ph.EP2021★ 8 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.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.EP2018

Spitzer Opens New Path to Break Classic Degeneracy for Jupiter-Mass Microlensing Planet OGLE-2017-BLG-1140Lb

S. Calchi Novati, J. Skowron, Y. K. Jung +36

We analyze the combined Spitzer and ground-based data for OGLE-2017-BLG-1140 and show that the event was generated by a Jupiter-class planet orbiting…

astro-ph.EP2018

The KMTNet 2016 Data Release

H. -W. Kim, K. -H. Hwang, D. -J. Kim +18

We present Korea Microlensing Telescope Network (KMTNet) light curves for microlensing-event candidates for the 2016 season, which covers an area of 97 sq.deg observed at cadences…

astro-ph.EP2018

OGLE-2017-BLG-1130: The First Binary Gravitational Microlens Detected From Spitzer Only

Tianshu Wang, S. Calchi Novati, A. Udalski +36

We analyze the binary gravitational microlensing event OGLE-2017-BLG-1130 (mass ratio q~0.45), the first published case in which the binary anomaly was only detected by the Spitzer…

astro-ph.EP2018

OGLE-2017-BLG-1434Lb: Eighth q < 1 * 10^-4 Mass-Ratio Microlens Planet Confirms Turnover in Planet Mass-Ratio Function

A. Udalski, Y. -H. Ryu, S. Sajadian +55

We report the discovery of a cold Super-Earth planet (m_p=4.4 +/- 0.5 M_Earth) orbiting a low-mass (M=0.23 +/- 0.03 M_Sun) M dwarf at projected separation a_perp = 1.18 +/- 0.10 AU…