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KMT-2025-BLG-1616Lb: First Microlensing Bound Planet From DREAMS

  • Authors: Hongjing Yang, 弘靖 杨, Weicheng Zang, 伟呈 臧, Yoon-Hyun Ryu, Takahiro Sumi, Jiyuan Zhang, 纪元 张, Hongyu Li, 弘禹 李, Cheongho Han, Yuchen Tang, Qiyue Qian, Zhixing Li, Yuxin Shang, Xikai Shan, Shude Mao, Guillermo Damke, Alfredo Zenteno, Steve Heathcote, Konstantina Boutsia, Przemek Mróz, Xiurui Zhao, Matthew Penny, Sean Terry, Patrick Tamburo, Timothy Cunningham, Quanzhi Ye, Eric W. Peng, Rachel Street, Katarzyna Kruszyńska, Etienne Bachelet, Yiannis Tsapras, Markus Hundertmark, Michael D. Albrow, Sun-Ju Chung, Andrew Gould, Kyu-Ha Hwang, Youn Kil Jung, In-Gu Shin, Yossi Shvartzvald, Jennifer C. Yee, Dong-Jin Kim, Chung-Uk Lee, Byeong-Gon Park, David P. Bennett, Ian A. Bond, Ryusei Hamada, Yuki Hirao, Asahi Idei, Shuma Makida, Shota Miyazaki, Tutumi Nagai, Togo Nagano, Seiya Nakayama, Mayu Nishio, Kansuke Nunota, Ryo Ogawa, Ryunosuke Oishi, Yui Okumoto, Nicholas J. Rattenbury, Yuki K. Satoh, Daisuke Suzuki, Motohide Tamura, Takuto Tamaoki, Hibiki Yama

Hongjing Yang et al 2026 The Astronomical Journal 171 .

  • Provider: AAS Journals

Caption: Figure 4.

Color–magnitude diagram for KMT-2025-BLG-1616. Black dots show OGLE-III field stars (M. K. Szymański et al. 2011) within a ﹩1\mathop{.}\limits^{{\rm{^{\prime} }}}5﹩ from the event position. The red asterisk and blue dot mark the centroid of the red clump and the source star, respectively. Green points show the HST CMD from J. A. Holtzman et al. (1998), and the HST red clump centroid, (V − I, I)cl,HST = (1.62, 15.15) (D. P. Bennett et al. 2008), has been shifted to match the OGLE-III red clump.

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