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arxiv: 2303.16881 · v1 · pith:TI4LQ5YUnew · submitted 2023-03-29 · 🌌 astro-ph.EP · astro-ph.GA

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

In-Gu Shin , Jennifer C. Yee , Weicheng Zang , Hongjing Yang , Kyu-Ha Hwang , Cheongho Han , Andrew Gould , Andrzej Udalski
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Ian A. Bond Michael D. Albrow Sun-Ju Chung Youn Kil Jung Yoon-Hyun Ryu Yossi Shvartzvald Sang-Mok Cha Dong-Jin Kim Seung-Lee Kim Chung-Uk Lee Dong-Joo Lee Yongseok Lee Byeong-Gon Park Richard W. Pogge Przemek Mr\'oz Micha{\l} K. Szyma\'nski Jan Skowron Rados{\l}aw Poleski Igor Soszy\'nski Pawe{\l} Pietrukowicz Szymon Koz{\l}owski Krzysztof A. Rybicki Patryk Iwanek Krzysztof Ulaczyk Marcin Wrona Mariusz Gromadzki Fumio Abe Richard Barry David P. Bennett Aparna Bhattacharya Hirosane Fujii Akihiko Fukui Ryusei Hamada Yuki Hirao Stela Ishitani Silva Yoshitaka Itow Rintaro Kirikawa Iona Kondo Naoki Koshimoto Yutaka Matsubara Shota Miyazaki Yasushi Muraki Greg Olmschenk Cl\'ement Ranc Nicholas J. Rattenbury Yuki Satoh Takahiro Sumi Daisuke Suzuki Mio Tomoyoshi Paul J. Tristram Aikaterini Vandorou Hibiki Yama Kansuke Yamashita
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keywords planetsamplecompletekmtnetplanetsanomalydetectionplanetary
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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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