Shin I-GYee JCZang WYang HHwang K-HHan CGould AUdalski ABond IAAlbrow MDChung S-JJung YKRyu Y-HShvartzvald YCha S-MKim D-JKim S-LLee C-ULee D-JLee YPark B-GPogge RWMróz PSzymański MKSkowron JPoleski RSoszyński IPietrukowicz PKozłowski SRybicki KAIwanek PUlaczyk KWrona MGromadzki MAbe FBarry RBennett DPBhattacharya AFujii HFukui AHamada RHirao YIshitani Silva SItow YKirikawa RKondo IKoshimoto NMatsubara YMiyazaki SMuraki YOlmschenk GRanc CRattenbury NJSatoh YSumi TSuzuki DTomoyoshi MTristram PJVandorou AYama HYamashita K2024-05-072024-05-072023-08-14Shin 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. 3.0004-6256https://mro.massey.ac.nz/handle/10179/69501As 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.(c) 2023 The Author/sCC BY 4.0https://creativecommons.org/licenses/by/4.0/Gravitational microlensing exoplanet detectionJournal article10.3847/1538-3881/ace96d1538-3881journal-article104