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OGLE-2016-BLG-0523: A Low-mass Brown Dwarf or Super-Jupiter in a >100 au Orbit

  • Authors: Hongjing Yang, 弘靖 杨, Weicheng Zang, 伟呈 臧, Yoon-Hyun Ryu, Andrzej Udalski, Yuchen Tang, 雨辰 唐, Michael D. Albrow, Sun-Ju Chung, Andrew Gould, Cheongho Han, Kyu-Ha Hwang, Youn Kil Jung, In-Gu Shin, Yossi Shvartzvald, Jennifer C. Yee, Sang-Mok Cha, Dong-Jin Kim, Hyoun-Woo Kim, Seung-Lee Kim, Chung-Uk Lee, Dong-Joo Lee, Yongseok Lee, Byeong-Gon Park, Richard W. Pogge, Przemek Mróz, Michał K. Szymański, Jan Skowron, Radoslaw Poleski, Igor Soszyński, Paweł Pietrukowicz, Szymon Kozłowski, Krzysztof A. Rybicki, Patryk Iwanek, Krzysztof Ulaczyk, Marcin Wrona, Mariusz Gromadzki, Mateusz J. Mróz, Jiyuan Zhang, 纪元 张, Shude Mao, 淑德 毛, Hongyu Li, 弘禹 李, Qiyue Qian, 奇玥 钱

Hongjing Yang et al 2026 The Astrophysical Journal Letters 1011 .

  • Provider: AAS Journals

Caption: Figure 3.

Posterior probability distributions of the lens and source physical parameters from the Bayesian analysis. The panels, from top to bottom and left to right, are the source distance DS, lens distance DL, lens-source relative proper motion μrel, the mass of the first and second lens ML1 and ML2, and their projected separation a⊥. The median and ±1σ values are marked in solid black and dashed blue vertical lines and are labeled on the top of each panel.

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