Han CJung YKKim DGould ABozza VBond IAChung S-JAlbrow MDHwang K-HRyu Y-HShin I-GShvartzvald YYang HZang WCha S-MKim D-JKim H-WKim S-LLee C-ULee D-JYee JCLee YPark B-GPogge RWAbe FBarry RBennett DPBhattacharya AFujii HFukui AHirao YSilva SIKirikawa RKondo IKoshimoto NMatsubara YMatsumoto SMiyazaki SMuraki YOkamura AOlmschenk GRanc CRattenbury NJSatoh YSumi TSuzuki DToda TTristram PJVandorou AYama HItow Y2024-09-122024-09-122023-07-04Han C, Kil Jung Y, Kim D, Gould A, Bozza V, Bond IA, Chung SJ, Albrow MD, Hwang KH, Ryu YH, Shin IG, Shvartzvald Y, Yang H, Zang W, Cha SM, Kim DJ, Kim HW, Kim SL, Lee CU, Lee DJ, Yee JC, Lee Y, Park BG, Pogge RW, Abe F, Barry R, Bennett DP, Bhattacharya A, Fujii H, Fukui A, Hirao Y, Ishitani Silva S, Kirikawa R, Kondo I, Koshimoto N, Matsubara Y, Matsumoto S, Miyazaki S, Muraki Y, Okamura A, Olmschenk G, Ranc C, Rattenbury NJ, Satoh Y, Sumi T, Suzuki D, Toda T, Tristram PJ, Vandorou A, Yama H, Itow Y. (2023). Probable brown dwarf companions detected in binary microlensing events during the 2018- 2020 seasons of the KMTNet survey. Astronomy and Astrophysics. 675.0004-6361https://mro.massey.ac.nz/handle/10179/71450Aims. We inspect the microlensing data of the KMTNet survey collected during the 2018-2020 seasons in order to find lensing events produced by binaries with brown dwarf (BD) companions. Methods. In order to pick out binary-lens events with candidate BD lens companions, we conducted systematic analyses of all anomalous lensing events observed during the seasons from 2018 to 2020. By applying a selection criterion of mass ratio between the lens components of 0.03 q 0.1, we identify four binary-lens events with candidate BD companions, namely KMT-2018-BLG-0321, KMT-2018-BLG-0885, KMT-2019-BLG-0297, and KMT-2019-BLG-0335. For the individual events, we present interpretations of the lens systems and measure the observables that can be used to constrain the physical lens parameters. Results. The masses of the lens companions estimated from the Bayesian analyses based on the measured observables indicate high probabilities that the lens companions are in the BD mass regime; that is, 59%, 68%, 66%, and 66% for the four respective events.(c) 2023 The Author/sCC BY 4.0https://creativecommons.org/licenses/by/4.0/ravitational lensing: micro / brown dwarfsJournal article10.1051/0004-6361/2022454551432-0746journal-articleA71