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arXiv · 2512.09325

Four Giant Planets from 2024 KMTNet Microlensing Campaign

Cheongho Han·Andrzej Udalski·Ian A. Bond·Chung-Uk Lee·Jiyuan Zhang·Michael D. Albrow·Sun-Ju Chung·Andrew Gould·Youn Kil Jung·Kyu-Ha Hwang·Yoon-Hyun Ryu·Yossi Shvartzvald·In-Gu Shin·Jennifer C. Yee·Weicheng Zang·Hongjing Yang·Doeon Kim·Dong-Jin Kim·Byeong-Gon Park·Przemek Mróz·Michał K. Szymański·Jan Skowron·Radosław Poleski·Igor Soszyński·Paweł Pietrukowicz·Szymon Kozłowski·Krzysztof A. Rybicki·Patryk Iwanek·Krzysztof Ulaczyk·Marcin Wrona·Mariusz Gromadzki·Mateusz J. Mróz·Fumio Abe·David P. Bennett·Aparna Bhattacharya·Ryusei Hamada·Stela Ishitani Silva·Yuki Hirao·Asahi Idei·Shota Miyazaki·Yasushi Muraki·Tutumi Nagai·Kansuke Nunota·Greg Olmschenk·Clément Ranc·Nicholas J. Rattenbury·Yuki Satoh·Takahiro Sumi·Daisuke Suzuki·Takuto Tamaoki·Sean K. Terry·Paul J. Tristram·Aikaterini Vandorou·Hibiki Yama·Yuchen Tang·Yunyi Tang·Shude Mao·Dan Maoz·Wei Zhu
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Abstract

In this work, we present analyses of four newly discovered planetary microlensing events from the 2024 KMTNet survey season: KMT-2024-BLG-0176, KMT-2024-BLG-0349, KMT-2024-BLG-1870, and KMT-2024-BLG-2087. In each case, the planetary nature was revealed through distinct types of anomalies in the lensing light curves: a positive bump near the peak for KMT-2024-BLG-0176, an asymmetric peak for KMT-2024-BLG-0349, a short-duration central dip for KMT-2024-BLG-1870, and a caustic-crossing feature for KMT-2024-BLG-2087. Detailed modeling of the light curves confirms that these anomalies are produced by planetary companions with planet-to-host mass ratios in the range of $(1.5\text{--}17.9)\times 10^{-3}$. Despite the diversity of signal morphologies, all planets detected in these events are giant planets with masses comparable to or exceeding that of Jupiter in the Solar System. Each planet orbits a host star less massive than the Sun, emphasizing the strength of microlensing in uncovering planetary systems around low-mass stellar hosts.

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Cheongho Han, Andrzej Udalski, Ian A. Bond, Chung-Uk Lee, Jiyuan Zhang, Michael D. Albrow, Sun-Ju Chung, Andrew Gould, Youn Kil Jung, Kyu-Ha Hwang, Yoon-Hyun Ryu, Yossi Shvartzvald, In-Gu Shin, Jennifer C. Yee, Weicheng Zang, Hongjing Yang, Doeon Kim, Dong-Jin Kim, Byeong-Gon Park, Przemek Mróz, Michał K. Szymański, Jan Skowron, Radosław Poleski, Igor Soszyński, Paweł Pietrukowicz, Szymon Kozłowski, Krzysztof A. Rybicki, Patryk Iwanek, Krzysztof Ulaczyk, Marcin Wrona, Mariusz Gromadzki, Mateusz J. Mróz, Fumio Abe, David P. Bennett, Aparna Bhattacharya, Ryusei Hamada, Stela Ishitani Silva, Yuki Hirao, Asahi Idei, Shota Miyazaki, Yasushi Muraki, Tutumi Nagai, Kansuke Nunota, Greg Olmschenk, Clément Ranc, Nicholas J. Rattenbury, Yuki Satoh, Takahiro Sumi, Daisuke Suzuki, Takuto Tamaoki, Sean K. Terry, Paul J. Tristram, Aikaterini Vandorou, Hibiki Yama, Yuchen Tang, Yunyi Tang, Shude Mao, Dan Maoz, Wei Zhu. 2025-12-10. Four Giant Planets from 2024 KMTNet Microlensing Campaign. https://arxiv.org/abs/2512.09325

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