_version_ 1866913102155481088
author Li, Hongyu
Li, Zhixing
Zang, Weicheng
Ryu, Yoon-Hyun
Udalski, Andrzej
Sumi, Takahiro
Yang, Hongjing
Zhang, Jiyuan
Mao, Shude
Albrow, Michael
Chung, Sun-Ju
Gould, Andrew
Han, Cheongho
Hwang, Kyu-Ha
Jung, Youn Kil
Shin, In-Gu
Shvartzvald, Yossi
Yee, Jennifer
Cha, Sang-Mok
Kim, Dong-Jin
Kim, Seung-Lee
Lee, Chung-Uk
Lee, Dong-Joo
Lee, Yongseok
Park, Byeong-Gon
Pogge, Richard
Mróz, Przemek
Szymański, Michał
Skowron, Jan
Poleski, Radoslaw
Soszyński, Igor
Pietrukowicz, Pawel
Kozłowski, Szymon
Rybicki, Krzysztof
Iwanek, Patryk
Ulaczyk, Krzysztof
Wrona, Marcin
Gromadzki, Mariusz
Mróz, Mateusz J.
Abe, Fumio
Bennett, David
Bhattacharya, Aparna
Bond, Ian
Hamada, Ryusei
Hirao, Yuki
Silva, Stela
Miyazaki, Shota
Muraki, Yasushi
Nunota, Kansuke
Olmschenk, Greg
Ranc, Clément
Rattenbury, Nicholas
Satoh, Yuki
Suzuki, Daisuke
Tamaoki, Takuto
Terry, Sean
Tristram, Paul
Vandorou, Aikaterini
Yama, Hibiki
author_facet Li, Hongyu
Li, Zhixing
Zang, Weicheng
Ryu, Yoon-Hyun
Udalski, Andrzej
Sumi, Takahiro
Yang, Hongjing
Zhang, Jiyuan
Mao, Shude
Albrow, Michael
Chung, Sun-Ju
Gould, Andrew
Han, Cheongho
Hwang, Kyu-Ha
Jung, Youn Kil
Shin, In-Gu
Shvartzvald, Yossi
Yee, Jennifer
Cha, Sang-Mok
Kim, Dong-Jin
Kim, Seung-Lee
Lee, Chung-Uk
Lee, Dong-Joo
Lee, Yongseok
Park, Byeong-Gon
Pogge, Richard
Mróz, Przemek
Szymański, Michał
Skowron, Jan
Poleski, Radoslaw
Soszyński, Igor
Pietrukowicz, Pawel
Kozłowski, Szymon
Rybicki, Krzysztof
Iwanek, Patryk
Ulaczyk, Krzysztof
Wrona, Marcin
Gromadzki, Mariusz
Mróz, Mateusz J.
Abe, Fumio
Bennett, David
Bhattacharya, Aparna
Bond, Ian
Hamada, Ryusei
Hirao, Yuki
Silva, Stela
Miyazaki, Shota
Muraki, Yasushi
Nunota, Kansuke
Olmschenk, Greg
Ranc, Clément
Rattenbury, Nicholas
Satoh, Yuki
Suzuki, Daisuke
Tamaoki, Takuto
Terry, Sean
Tristram, Paul
Vandorou, Aikaterini
Yama, Hibiki
contents To complete the analysis of the 2023 KMTNet subprime-field microlensing planetary events identified by its AlertFinder system, we present the analysis of six events, KMT-2023-BLG-(1810, 0084, 1118, 0584, 1697, 2218). We find that the first three events are securely confirmed as planetary, with inferred mass ratios of $\log q \sim -1.9$, $-2.0$, and $-2.6$, respectively. The remaining three events exhibit the well-known degeneracy between binary-lens/single-source (2L1S) and single-lens/binary-source (1L2S) models, and two of these also admit viable stellar binary solutions. A Bayesian analysis indicates that the companions in the confirmed planetary events are likely either super-Jupiters orbiting beyond the snow line of M- or K-dwarf hosts or, for two degenerate solutions of KMT-2023-BLG-1118, Saturn-mass planets orbiting late-type M dwarfs. To date, the 2023 KMTNet sample contains 25 unambiguous planetary events, and its mass-ratio distribution is consistent with that of the KMTNet planetary sample from 2016--2019.
format Preprint
id arxiv_https___arxiv_org_abs_2605_07392
institution arXiv
publishDate 2026
record_format arxiv
spellingShingle Mass Production of 2023 KMTNet Microlensing Planets. III: Three Planets from the Subprime Field
Li, Hongyu
Li, Zhixing
Zang, Weicheng
Ryu, Yoon-Hyun
Udalski, Andrzej
Sumi, Takahiro
Yang, Hongjing
Zhang, Jiyuan
Mao, Shude
Albrow, Michael
Chung, Sun-Ju
Gould, Andrew
Han, Cheongho
Hwang, Kyu-Ha
Jung, Youn Kil
Shin, In-Gu
Shvartzvald, Yossi
Yee, Jennifer
Cha, Sang-Mok
Kim, Dong-Jin
Kim, Seung-Lee
Lee, Chung-Uk
Lee, Dong-Joo
Lee, Yongseok
Park, Byeong-Gon
Pogge, Richard
Mróz, Przemek
Szymański, Michał
Skowron, Jan
Poleski, Radoslaw
Soszyński, Igor
Pietrukowicz, Pawel
Kozłowski, Szymon
Rybicki, Krzysztof
Iwanek, Patryk
Ulaczyk, Krzysztof
Wrona, Marcin
Gromadzki, Mariusz
Mróz, Mateusz J.
Abe, Fumio
Bennett, David
Bhattacharya, Aparna
Bond, Ian
Hamada, Ryusei
Hirao, Yuki
Silva, Stela
Miyazaki, Shota
Muraki, Yasushi
Nunota, Kansuke
Olmschenk, Greg
Ranc, Clément
Rattenbury, Nicholas
Satoh, Yuki
Suzuki, Daisuke
Tamaoki, Takuto
Terry, Sean
Tristram, Paul
Vandorou, Aikaterini
Yama, Hibiki
Earth and Planetary Astrophysics
Astrophysics of Galaxies
To complete the analysis of the 2023 KMTNet subprime-field microlensing planetary events identified by its AlertFinder system, we present the analysis of six events, KMT-2023-BLG-(1810, 0084, 1118, 0584, 1697, 2218). We find that the first three events are securely confirmed as planetary, with inferred mass ratios of $\log q \sim -1.9$, $-2.0$, and $-2.6$, respectively. The remaining three events exhibit the well-known degeneracy between binary-lens/single-source (2L1S) and single-lens/binary-source (1L2S) models, and two of these also admit viable stellar binary solutions. A Bayesian analysis indicates that the companions in the confirmed planetary events are likely either super-Jupiters orbiting beyond the snow line of M- or K-dwarf hosts or, for two degenerate solutions of KMT-2023-BLG-1118, Saturn-mass planets orbiting late-type M dwarfs. To date, the 2023 KMTNet sample contains 25 unambiguous planetary events, and its mass-ratio distribution is consistent with that of the KMTNet planetary sample from 2016--2019.
title Mass Production of 2023 KMTNet Microlensing Planets. III: Three Planets from the Subprime Field
topic Earth and Planetary Astrophysics
Astrophysics of Galaxies
url https://arxiv.org/abs/2605.07392