Systematic KMTNet Planetary Anomaly Search. IX. Complete Sample of 2016 Prime-field Planets

In-Gu Shin,Jennifer Yee,Weicheng Zang,Hongjing Yang,Kyu-Ha A. Hwang,Cheongho D. Han,Andrew Gould,Andrzej Udalski,Ian Bond,Michael Albrow,Sun-Ju Chung,Youn Kil Jung,Yoon-Hyun Ryu,Yossi Shvartzvald,Sang-Mok Cha,Dong-Jin Kim,Seung-Lee Kim,Chung-Uk W. Lee,Dong-Joo Lee,Yongseok Lee,Byeong-Gon Park,Richard Pogge, Przemek KMTNet Collaboration,Przemek Mroz,Michal K. Szymanski,Jan A. Skowron,Radoslaw Poleski,Igor Soszynski,Pawel Pietrukowicz,Szymon Kozlowski,Krzysztof Rybicki,Patryk Iwanek,Krzysztof P. Ulaczyk,Marcin Wrona,Mariusz Gromadzki, Richard OGLE Collaboration,Fumio Abe,Richard Barry,David Bennett,Aparna Bhattacharya,Hirosane Fujii,Akihiko Fukui,Ryusei Hamada,Yuki Hirao,Stela Ishitani Silva,Yoshitaka Itow,Rintaro Kirikawa,Iona Kondo,Naoki J. Koshimoto,Yutaka Matsubara,Shota Miyazaki,Yasushi Muraki,Greg Olmschenk,Clement J. Ranc,Nicholas Rattenbury,Yuki Satoh,Takahiro Sumi,Daisuke Suzuki,Mio Tomoyoshi,Paul Tristram,Aikaterini Vandorou,Hibiki Yama,Kansuke Yamashita, MOA Collaboration

ASTRONOMICAL JOURNAL（2023）

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摘要

As a part of the "Systematic KMTNet Planetary Anomaly Search" series, we report five new planets (namely, OGLE-2016-BLG-1635Lb, MOA-2016-BLG-532Lb, KMT-2016-BLG-0625Lb, OGLE-2016-BLG-1850Lb, and KMT-2016-BLG-1751Lb) and one planet candidate (KMT-2016-BLG-1855), which were found by searching 2016 KMTNet prime fields. These buried planets show a wide range of masses from Earth-class to super-Jupiter-class and are located in both the disk and the bulge. The ultimate goal of this series is to build a complete planet sample. Because our work provides a complementary sample to other planet detection methods, which have different detection sensitivities, our complete sample will help us to obtain a better understanding of planet demographics in our Galaxy.

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prime-field

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