Shin, In-Gu and Yee, Jennifer C. and Zang, Weicheng and Yang, Hongjing and Hwang, Kyu-Ha and Han, Cheongho and Gould, Andrew and Udalski, Andrzej and Bond, Ian A. and Albrow, Michael D. and Chung, Sun-Ju and Jung, Youn Kil and Ryu, Yoon-Hyun and Shvartzvald, Yossi and Cha, Sang-Mok and Kim, Dong-Jin and Kim, Seung-Lee and Lee, Chung-Uk and Lee, Dong-Joo and Lee, Yongseok and Park, Byeong-Gon and Pogge, Richard W. and Mróz, Przemek and Szymański, Michał K. and Skowron, Jan and Poleski, Radosław and Soszyński, Igor and Pietrukowicz, Paweł and Kozłowski, Szymon and Rybicki, Krzysztof A. and Iwanek, Patryk and Ulaczyk, Krzysztof and Wrona, Marcin and Gromadzki, Mariusz and Abe, Fumio and Barry, Richard and Bennett, David P. and Bhattacharya, Aparna and Fujii, Hirosane and Fukui, Akihiko and Hamada, Ryusei and Hirao, Yuki and Silva, Stela Ishitani and Itow, Yoshitaka and Kirikawa, Rintaro and Kondo, Iona and Koshimoto, Naoki and Matsubara, Yutaka and Miyazaki, Shota and Muraki, Yasushi and Olmschenk, Greg and Ranc, Clément and Rattenbury, Nicholas J. and Satoh, Yuki and Sumi, Takahiro and Suzuki, Daisuke and Tomoyoshi, Mio and Tristram, Paul J. and Vandorou, Aikaterini and Yama, Hibiki and Yamashita, Kansuke (2023) Systematic KMTNet Planetary Anomaly Search. IX. Complete Sample of 2016 Prime-field Planets. The Astronomical Journal, 166 (3). p. 104. ISSN 0004-6256
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Abstract
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.
| Item Type: | Article |
|---|---|
| Subjects: | GO for ARCHIVE > Physics and Astronomy |
| Depositing User: | Unnamed user with email support@goforarchive.com |
| Date Deposited: | 11 Nov 2023 05:43 |
| Last Modified: | 11 Nov 2023 05:43 |
| URI: | http://eprints.go4mailburst.com/id/eprint/1726 |
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