Systematic KMTNet Planetary Anomaly Search, Paper II: Six New $q<2\times 10^{-4}$ Mass-ratio Planets
Kyu-Ha Hwang, Weicheng Zang, Andrew Gould, Andrzej Udalski, Ian A., Bond, Hongjing Yang, Shude Mao, Michael D. Albrow, Sun-Ju Chung, Cheongho, Han, Youn Kil Jung, Yoon-Hyun Ryu, In-Gu Shin, Yossi Shvartzvald, Jennifer C., Yee, Sang-Mok Cha, Dong-Jin Kim, Hyoun-Woo Kim

TL;DR
This paper applies an automated algorithm to identify six new low-mass-ratio exoplanets in microlensing data, revealing that such planets may be more common than previously thought.
Contribution
The study introduces new low-mass-ratio planets discovered via an automated search, expanding the known population and demonstrating the effectiveness of the AnomalyFinder algorithm.
Findings
Six new planets with $q<2\times 10^{-4}$ discovered
Subtle signals missed in previous searches identified
Planets in this mass-ratio range may be more prevalent
Abstract
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, with cadences . We find a total of 11 planets with mass ratios , including six newly discovered planets, one planet that was reported in Paper I, and recovery of four previously discovered planets. One of the new planets, OGLE-2018-BLG-0977Lb, is in a planetary-caustic event, while the other five (OGLE-2018-BLG-0506Lb, OGLE-2018-BLG-0516Lb, OGLE-2019-BLG-1492Lb, KMT-2019-BLG-0253, and KMT-2019-BLG-0953) are revealed by a "dip" in the light curve as the source crosses the host-planet axis on the opposite side of the planet. These subtle signals were missed in previous by-eye searches. The planet-host separations (scaled to the Einstein radius), , and planet-host…
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