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

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2023-08-14

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American Astronomical Society

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(c) 2023 The Author/s
CC BY 4.0

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.

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Gravitational microlensing exoplanet detection

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Shin IG, Yee JC, Zang W, Yang H, Hwang KH, Han C, Gould A, Udalski A, Bond IA, Albrow MD, Chung SJ, Jung YK, Ryu YH, Shvartzvald Y, Cha SM, Kim DJ, Kim SL, Lee CU, Lee DJ, Lee Y, Park BG, Pogge RW, Mróz P, Szymański MK, Skowron J, Poleski R, Soszyński I, Pietrukowicz P, Kozłowski S, Rybicki KA, Iwanek P, Ulaczyk K, Wrona M, Gromadzki M, Abe F, Barry R, Bennett DP, Bhattacharya A, Fujii H, Fukui A, Hamada R, Hirao Y, Silva SI, Itow Y, Kirikawa R, Kondo I, Koshimoto N, Matsubara Y, Miyazaki S, Muraki Y, Olmschenk G, Ranc C, Rattenbury NJ, Satoh Y, Sumi T, Suzuki D, Tomoyoshi M, Tristram PJ, Vandorou A, Yama H, Yamashita K. (2023). Systematic KMTNet Planetary Anomaly Search. IX. Complete Sample of 2016 Prime-field Planets. Astronomical Journal. 166. 3.

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Except where otherwised noted, this item's license is described as (c) 2023 The Author/s