Four Giant Planets from 2024 KMTNet Microlensing Campaign
/ Authors
C. Han, A. Udalski, I. Bond, Chung-Uk Lee, Jiyuan Zhang, M. Albrow, S. Chung, A. Gould, Y. Jung, K. Hwang
and 49 more authors
Y. Ryu, Y. Shvartzvald, I. Shin, J. Yee, W. Zang, Hongjing Yang, Doeon Kim, Dong-Jin Kim, B.-G. Park, P. Mr'oz, M. K. Szyma'nski, J. Skowron, R. Poleski, I. Soszy'nski, P. Pietrukowicz, S. Kozłowski, K. Rybicki, P. Iwanek, K. Ulaczyk, M. Wrona, M. Gromadzki, M. Mr'oz, F. Abe, D. Bennett, A. Bhattacharya, R. Hamada, Stela Ishitani Silva, Y. Hirao, A. Idei, S. Miyazaki, Y. Muraki, T. Nagai, K. Nunota, G. Olmschenk, C. Ranc, N. Rattenbury, Y. Satoh, T. Sumi, D. Suzuki, Takuto Tamaoki, S. Terry, P. Tristram, A. Vandorou, H. Yama, Yuchen Tang, Yunyi Tang, S. Mao, D. Maoz, Wei Zhu
/ 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 (1.5−17.9) × 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.
Journal: Publications of the Astronomical Society of the Pacific