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Bond, Igor Soszy\\'nski, In-Gu Shin, Iona Kondo, Jan Skowron, Jennifer C. Yee, Krzysztof A. Rybicki, Krzysztof Ulaczyk, Kyu-Ha Hwang, Marcin Wrona, Mariusz Gromadzki, Matthew T. Penny, Michael D. Albrow, Michal K. Szyma\\'nski, Naoki Koshimoto, Nicholas J. Rattenbury, Pascal Fouqu\\'e, Patryk Iwanek, Paul J. Tristram, Pawel Pietrukowicz, Przemek Mr\\'oz, Radek Poleski, Richard Barry, Richard W. Pogge, Rintaro Kirikawa, Sang-Mok Cha, Seung-Lee Kim, Shota Miyazaki, Shude Mao, Stela Ishitani Silva, Sun-Ju Chung, Szymon Kozlowski, Takahiro Sumi, Weicheng Zang, Wei Zhu, Xiangyu Zhang, Yasushi Muraki, Yongseok Lee, Yoon-Hyun Ryu, Yoshitaka Itow, Yossi Shvartzvald, Youn Kil Jung, Yuki Hirao, Yuki K. Satoh, Yutaka Matsubara","submitted_at":"2021-06-12T04:38:48Z","abstract_excerpt":"We apply the automated AnomalyFinder algorithm of Paper I (Zang et al. 2021b) to 2018-2019 light curves from the $\\simeq 13\\,{\\rm deg}^2$ covered by the six KMTNet prime fields, with cadences $\\Gamma \\geq 2\\,{\\rm hr}^{-1}$. We find a total of 11 planets with mass ratios $q<2\\times 10^{-4}$, including six newly discovered planets, one planet that was reported in Paper I, and recovery of four previously discovered planets. 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