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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 1.

Light curve of the microlensing event, KMT-2025-BLG-1616, with the 2L1S models (solid black and orange lines) and the underlying 1L1S model (dashed gray line). Different datasets are plotted in different colors. The upper panels shows the 8 days data around the peak. The lower panels present a close-up of the planetary anomaly and the residuals relative to the 2L1S models.

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