Mass Production of 2023 KMTNet Microlensing Planets. II: Two Planets and A Brown Dwarf

Fuente: arXiv
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Auteurs principaux: Li, Zhixing, Li, Hongyu, Zang, Weicheng, Ryu, Yoon-Hyun, Udalski, Andrzej, Sumi, Takahiro, Yang, Hongjing, Tang, Yuchen, Zhang, Jiyuan, Mao, Shude, Albrow, Michael D., Chung, Sun-Ju, Gould, Andrew, Han, Cheongho, Hwang, Kyu-Ha, Jung, Youn Kil, Shin, In-Gu, Shvartzvald, Yossi, Yee, Jennifer C., Cha, Sang-Mok, Kim, Dong-Jin, Kim, Seung-Lee, Lee, Chung-Uk, Lee, Dong-Joo, Lee, Yongseok, Park, Byeong-Gon, Pogge, Richard W., Mróz, Przemek, Szymański, Michał K., Skowron, Jan, Poleski, Radoslaw, Soszyński, Igor, Pietrukowicz, Paweł, Kozłowski, Szymon, Rybicki, Krzysztof A., Iwanek, Patryk, Ulaczyk, Krzysztof, Wrona, Marcin, Gromadzki, Mariusz, Mróz, Mateusz J., Abe, Fumio, Bando, Ken, Bennett, David P., Bhattacharya, Aparna, Bond, Ian A., Fukui, Akihiko, Hamada, Ryusei, Hamada, Shunya, Hamasak, Naoto, Hirao, Yuki, Silva, Stela Ishitani, Koshimoto, Naoki, Matsubara, Yutaka, Miyazaki, Shota, Muraki, Yasushi, Nagai, Tutumi, Nunota, Kansuke, Olmschenk, Greg, Ranc, Clément, Rattenbury, Nicholas J., Satoh, Yuki, Suzuki, Daisuke, Terry, Sean, Tristram, Paul J., Vandorou, Aikaterini, Yama, Hibiki
Format: Preprint
Publié: 2026
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_version_ 1866917349590827008
author Li, Zhixing
Li, Hongyu
Zang, Weicheng
Ryu, Yoon-Hyun
Udalski, Andrzej
Sumi, Takahiro
Yang, Hongjing
Tang, Yuchen
Zhang, Jiyuan
Mao, Shude
Albrow, Michael D.
Chung, Sun-Ju
Gould, Andrew
Han, Cheongho
Hwang, Kyu-Ha
Jung, Youn Kil
Shin, In-Gu
Shvartzvald, Yossi
Yee, Jennifer C.
Cha, Sang-Mok
Kim, Dong-Jin
Kim, Seung-Lee
Lee, Chung-Uk
Lee, Dong-Joo
Lee, Yongseok
Park, Byeong-Gon
Pogge, Richard W.
Mróz, Przemek
Szymański, Michał K.
Skowron, Jan
Poleski, Radoslaw
Soszyński, Igor
Pietrukowicz, Paweł
Kozłowski, Szymon
Rybicki, Krzysztof A.
Iwanek, Patryk
Ulaczyk, Krzysztof
Wrona, Marcin
Gromadzki, Mariusz
Mróz, Mateusz J.
Abe, Fumio
Bando, Ken
Bennett, David P.
Bhattacharya, Aparna
Bond, Ian A.
Fukui, Akihiko
Hamada, Ryusei
Hamada, Shunya
Hamasak, Naoto
Hirao, Yuki
Silva, Stela Ishitani
Koshimoto, Naoki
Matsubara, Yutaka
Miyazaki, Shota
Muraki, Yasushi
Nagai, Tutumi
Nunota, Kansuke
Olmschenk, Greg
Ranc, Clément
Rattenbury, Nicholas J.
Satoh, Yuki
Suzuki, Daisuke
Terry, Sean
Tristram, Paul J.
Vandorou, Aikaterini
Yama, Hibiki
author_facet Li, Zhixing
Li, Hongyu
Zang, Weicheng
Ryu, Yoon-Hyun
Udalski, Andrzej
Sumi, Takahiro
Yang, Hongjing
Tang, Yuchen
Zhang, Jiyuan
Mao, Shude
Albrow, Michael D.
Chung, Sun-Ju
Gould, Andrew
Han, Cheongho
Hwang, Kyu-Ha
Jung, Youn Kil
Shin, In-Gu
Shvartzvald, Yossi
Yee, Jennifer C.
Cha, Sang-Mok
Kim, Dong-Jin
Kim, Seung-Lee
Lee, Chung-Uk
Lee, Dong-Joo
Lee, Yongseok
Park, Byeong-Gon
Pogge, Richard W.
Mróz, Przemek
Szymański, Michał K.
Skowron, Jan
Poleski, Radoslaw
Soszyński, Igor
Pietrukowicz, Paweł
Kozłowski, Szymon
Rybicki, Krzysztof A.
Iwanek, Patryk
Ulaczyk, Krzysztof
Wrona, Marcin
Gromadzki, Mariusz
Mróz, Mateusz J.
Abe, Fumio
Bando, Ken
Bennett, David P.
Bhattacharya, Aparna
Bond, Ian A.
Fukui, Akihiko
Hamada, Ryusei
Hamada, Shunya
Hamasak, Naoto
Hirao, Yuki
Silva, Stela Ishitani
Koshimoto, Naoki
Matsubara, Yutaka
Miyazaki, Shota
Muraki, Yasushi
Nagai, Tutumi
Nunota, Kansuke
Olmschenk, Greg
Ranc, Clément
Rattenbury, Nicholas J.
Satoh, Yuki
Suzuki, Daisuke
Terry, Sean
Tristram, Paul J.
Vandorou, Aikaterini
Yama, Hibiki
contents To expand the homogeneous microlensing planetary sample of the Korea Microlensing Telescope Network (KMTNet), we investigate six planetary candidates identified by the AnomalyFinder search in the 2023 prime-field data, namely KMT-2023-BLG-1592, OGLE-2023-BLG-0766, KMT-2023-BLG-0332, KMT-2023-BLG-0486, KMT-2023-BLG-0792, and OGLE-2023-BLG-1043. Light-curve modeling indicates that the first two events have planetary mass ratios of $\log q \sim -3.0$ and $-2.6$, while the third exhibits a brown dwarf mass ratio of $\log q \sim -1.4$. The remaining three events show the well-known degeneracy between the binary-lens single-source (2L1S) and single-lens binary-source (1L2S) interpretations. A Bayesian analysis yields companion masses of about 0.6 and 1.2 Jupiter masses for the two planetary systems, likely orbiting beyond the snow lines of M- or K-dwarf hosts. A review of the KMTNet planetary sample shows that candidates discovered by AnomalyFinder are significantly more likely to exhibit the 2L1S/1L2S degeneracy, consistent with the tendency of AnomalyFinder to detect subtler planetary signals.
format Preprint
id arxiv_https___arxiv_org_abs_2603_13887
institution arXiv
publishDate 2026
record_format arxiv
spellingShingle Mass Production of 2023 KMTNet Microlensing Planets. II: Two Planets and A Brown Dwarf
Li, Zhixing
Li, Hongyu
Zang, Weicheng
Ryu, Yoon-Hyun
Udalski, Andrzej
Sumi, Takahiro
Yang, Hongjing
Tang, Yuchen
Zhang, Jiyuan
Mao, Shude
Albrow, Michael D.
Chung, Sun-Ju
Gould, Andrew
Han, Cheongho
Hwang, Kyu-Ha
Jung, Youn Kil
Shin, In-Gu
Shvartzvald, Yossi
Yee, Jennifer C.
Cha, Sang-Mok
Kim, Dong-Jin
Kim, Seung-Lee
Lee, Chung-Uk
Lee, Dong-Joo
Lee, Yongseok
Park, Byeong-Gon
Pogge, Richard W.
Mróz, Przemek
Szymański, Michał K.
Skowron, Jan
Poleski, Radoslaw
Soszyński, Igor
Pietrukowicz, Paweł
Kozłowski, Szymon
Rybicki, Krzysztof A.
Iwanek, Patryk
Ulaczyk, Krzysztof
Wrona, Marcin
Gromadzki, Mariusz
Mróz, Mateusz J.
Abe, Fumio
Bando, Ken
Bennett, David P.
Bhattacharya, Aparna
Bond, Ian A.
Fukui, Akihiko
Hamada, Ryusei
Hamada, Shunya
Hamasak, Naoto
Hirao, Yuki
Silva, Stela Ishitani
Koshimoto, Naoki
Matsubara, Yutaka
Miyazaki, Shota
Muraki, Yasushi
Nagai, Tutumi
Nunota, Kansuke
Olmschenk, Greg
Ranc, Clément
Rattenbury, Nicholas J.
Satoh, Yuki
Suzuki, Daisuke
Terry, Sean
Tristram, Paul J.
Vandorou, Aikaterini
Yama, Hibiki
Earth and Planetary Astrophysics
Astrophysics of Galaxies
To expand the homogeneous microlensing planetary sample of the Korea Microlensing Telescope Network (KMTNet), we investigate six planetary candidates identified by the AnomalyFinder search in the 2023 prime-field data, namely KMT-2023-BLG-1592, OGLE-2023-BLG-0766, KMT-2023-BLG-0332, KMT-2023-BLG-0486, KMT-2023-BLG-0792, and OGLE-2023-BLG-1043. Light-curve modeling indicates that the first two events have planetary mass ratios of $\log q \sim -3.0$ and $-2.6$, while the third exhibits a brown dwarf mass ratio of $\log q \sim -1.4$. The remaining three events show the well-known degeneracy between the binary-lens single-source (2L1S) and single-lens binary-source (1L2S) interpretations. A Bayesian analysis yields companion masses of about 0.6 and 1.2 Jupiter masses for the two planetary systems, likely orbiting beyond the snow lines of M- or K-dwarf hosts. A review of the KMTNet planetary sample shows that candidates discovered by AnomalyFinder are significantly more likely to exhibit the 2L1S/1L2S degeneracy, consistent with the tendency of AnomalyFinder to detect subtler planetary signals.
title Mass Production of 2023 KMTNet Microlensing Planets. II: Two Planets and A Brown Dwarf
topic Earth and Planetary Astrophysics
Astrophysics of Galaxies
url https://arxiv.org/abs/2603.13887