Candidate Microlensing Brown Dwarfs in Binary Lens Systems from the 2023--2025 Observing Seasons

Fuente: arXiv
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Autores principales: Han, Cheongho, Udalski, Andrzej, Bond, Ian A., Lee, Chung-Uk, Albrow, Michael D., Chung, Sun-Ju, Gould, Andrew, Jung, Youn Kil, Hwang, Kyu-Ha, Ryu, Yoon-Hyun, Shvartzvald, Yossi, Shin, In-Gu, Yee, Jennifer C., Zang, Weicheng, Yang, Hongjing, Kim, Doeon, Kim, Dong-Jin, Kim, Seung-Lee, Lee, Dong-Joo, Cha, Sang-Mok, Lee, Yongseok, Park, Byeong-Gon, Pogge, Richard W., Mróz, Przemek, Szymański, Michał K., Skowron, Jan, Poleski, Radosław, Soszyński, Igor, Pietrukowicz, Paweł, Kozłowski, Szymon, Rybicki, Krzysztof A., Iwanek, Patryk, Ulaczyk, Krzysztof, Wrona, Marcin, Gromadzki, Mariusz, Mróz, Mateusz J., Abe, Fumio, Bennett, David P., Bhattacharya, Aparna, Hamada, Ryusei, Hirao, Yuki, Idei, Asahi, Silva, Stela Ishitani, Makida, Shuma, Miyazaki, Shota, Muraki, Yasushi, Nagai, Tutumi, Nagano, Togo, Nakayama, Seiya, Nishio, Mayu, Nunota, Kansuke, Ogawa, Ryo, Oishi, Ryunosuke, Okumoto, Yui, Olmschenk, Greg, Ranc, Clément, Rattenbury, Nicholas J., Satoh, Yuki, Sumi, Takahiro, Suzuki, Daisuke, Tamaoki, Takuto, Terry, Sean K., Tristram, Paul J., Vandorou, Aikaterini, Yama, Hibiki
Formato: Preprint
Publicado: 2026
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author Han, Cheongho
Udalski, Andrzej
Bond, Ian A.
Lee, Chung-Uk
Albrow, Michael D.
Chung, Sun-Ju
Gould, Andrew
Jung, Youn Kil
Hwang, Kyu-Ha
Ryu, Yoon-Hyun
Shvartzvald, Yossi
Shin, In-Gu
Yee, Jennifer C.
Zang, Weicheng
Yang, Hongjing
Kim, Doeon
Kim, Dong-Jin
Kim, Seung-Lee
Lee, Dong-Joo
Cha, Sang-Mok
Lee, Yongseok
Park, Byeong-Gon
Pogge, Richard W.
Mróz, Przemek
Szymański, Michał K.
Skowron, Jan
Poleski, Radosław
Soszyński, Igor
Pietrukowicz, Paweł
Kozłowski, Szymon
Rybicki, Krzysztof A.
Iwanek, Patryk
Ulaczyk, Krzysztof
Wrona, Marcin
Gromadzki, Mariusz
Mróz, Mateusz J.
Abe, Fumio
Bennett, David P.
Bhattacharya, Aparna
Hamada, Ryusei
Hirao, Yuki
Idei, Asahi
Silva, Stela Ishitani
Makida, Shuma
Miyazaki, Shota
Muraki, Yasushi
Nagai, Tutumi
Nagano, Togo
Nakayama, Seiya
Nishio, Mayu
Nunota, Kansuke
Ogawa, Ryo
Oishi, Ryunosuke
Okumoto, Yui
Olmschenk, Greg
Ranc, Clément
Rattenbury, Nicholas J.
Satoh, Yuki
Sumi, Takahiro
Suzuki, Daisuke
Tamaoki, Takuto
Terry, Sean K.
Tristram, Paul J.
Vandorou, Aikaterini
Yama, Hibiki
author_facet Han, Cheongho
Udalski, Andrzej
Bond, Ian A.
Lee, Chung-Uk
Albrow, Michael D.
Chung, Sun-Ju
Gould, Andrew
Jung, Youn Kil
Hwang, Kyu-Ha
Ryu, Yoon-Hyun
Shvartzvald, Yossi
Shin, In-Gu
Yee, Jennifer C.
Zang, Weicheng
Yang, Hongjing
Kim, Doeon
Kim, Dong-Jin
Kim, Seung-Lee
Lee, Dong-Joo
Cha, Sang-Mok
Lee, Yongseok
Park, Byeong-Gon
Pogge, Richard W.
Mróz, Przemek
Szymański, Michał K.
Skowron, Jan
Poleski, Radosław
Soszyński, Igor
Pietrukowicz, Paweł
Kozłowski, Szymon
Rybicki, Krzysztof A.
Iwanek, Patryk
Ulaczyk, Krzysztof
Wrona, Marcin
Gromadzki, Mariusz
Mróz, Mateusz J.
Abe, Fumio
Bennett, David P.
Bhattacharya, Aparna
Hamada, Ryusei
Hirao, Yuki
Idei, Asahi
Silva, Stela Ishitani
Makida, Shuma
Miyazaki, Shota
Muraki, Yasushi
Nagai, Tutumi
Nagano, Togo
Nakayama, Seiya
Nishio, Mayu
Nunota, Kansuke
Ogawa, Ryo
Oishi, Ryunosuke
Okumoto, Yui
Olmschenk, Greg
Ranc, Clément
Rattenbury, Nicholas J.
Satoh, Yuki
Sumi, Takahiro
Suzuki, Daisuke
Tamaoki, Takuto
Terry, Sean K.
Tristram, Paul J.
Vandorou, Aikaterini
Yama, Hibiki
contents We present detailed light-curve analyses of ten binary-lens microlensing events observed during the 2023--2025 seasons and selected as candidates for hosting brown-dwarf companions. The sample includes OGLE-2023-BLG-0249, KMT-2023-BLG-1246, OGLE-2023-BLG-0079, KMT-2024-BLG-0072, KMT-2024-BLG-0897, KMT-2024-BLG-1876, KMT-2024-BLG-2379, KMT-2025-BLG-0922, KMT-2025-BLG-1056, and KMT-2025-BLG-2427. For each event, we carry out modeling of the light curve, explore relevant degeneracies, and, when finite-source effects are present, determine the angular Einstein radius. For OGLE-2023-BLG-0249, we additionally measure the microlens parallax, which allows a direct determination of the lens masses and distance. For the remaining events, we estimate the physical lens properties via Bayesian analyses incorporating Galactic priors. The resulting posteriors show that the lens companions in all systems have median masses in the brown-dwarf regime, and the lenses of two events (KMT-2025-BLG-0922 and KMT-2025-BLG-1056) are consistent with binaries in which both lens components fall within the brown-dwarf mass range. Spanning a wide range of projected separations and distances, these detections illustrate the power of high-cadence microlensing surveys to build a census of brown-dwarf companions, including faint and distant systems beyond the reach of flux-limited methods.
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publishDate 2026
record_format arxiv
spellingShingle Candidate Microlensing Brown Dwarfs in Binary Lens Systems from the 2023--2025 Observing Seasons
Han, Cheongho
Udalski, Andrzej
Bond, Ian A.
Lee, Chung-Uk
Albrow, Michael D.
Chung, Sun-Ju
Gould, Andrew
Jung, Youn Kil
Hwang, Kyu-Ha
Ryu, Yoon-Hyun
Shvartzvald, Yossi
Shin, In-Gu
Yee, Jennifer C.
Zang, Weicheng
Yang, Hongjing
Kim, Doeon
Kim, Dong-Jin
Kim, Seung-Lee
Lee, Dong-Joo
Cha, Sang-Mok
Lee, Yongseok
Park, Byeong-Gon
Pogge, Richard W.
Mróz, Przemek
Szymański, Michał K.
Skowron, Jan
Poleski, Radosław
Soszyński, Igor
Pietrukowicz, Paweł
Kozłowski, Szymon
Rybicki, Krzysztof A.
Iwanek, Patryk
Ulaczyk, Krzysztof
Wrona, Marcin
Gromadzki, Mariusz
Mróz, Mateusz J.
Abe, Fumio
Bennett, David P.
Bhattacharya, Aparna
Hamada, Ryusei
Hirao, Yuki
Idei, Asahi
Silva, Stela Ishitani
Makida, Shuma
Miyazaki, Shota
Muraki, Yasushi
Nagai, Tutumi
Nagano, Togo
Nakayama, Seiya
Nishio, Mayu
Nunota, Kansuke
Ogawa, Ryo
Oishi, Ryunosuke
Okumoto, Yui
Olmschenk, Greg
Ranc, Clément
Rattenbury, Nicholas J.
Satoh, Yuki
Sumi, Takahiro
Suzuki, Daisuke
Tamaoki, Takuto
Terry, Sean K.
Tristram, Paul J.
Vandorou, Aikaterini
Yama, Hibiki
Solar and Stellar Astrophysics
Earth and Planetary Astrophysics
We present detailed light-curve analyses of ten binary-lens microlensing events observed during the 2023--2025 seasons and selected as candidates for hosting brown-dwarf companions. The sample includes OGLE-2023-BLG-0249, KMT-2023-BLG-1246, OGLE-2023-BLG-0079, KMT-2024-BLG-0072, KMT-2024-BLG-0897, KMT-2024-BLG-1876, KMT-2024-BLG-2379, KMT-2025-BLG-0922, KMT-2025-BLG-1056, and KMT-2025-BLG-2427. For each event, we carry out modeling of the light curve, explore relevant degeneracies, and, when finite-source effects are present, determine the angular Einstein radius. For OGLE-2023-BLG-0249, we additionally measure the microlens parallax, which allows a direct determination of the lens masses and distance. For the remaining events, we estimate the physical lens properties via Bayesian analyses incorporating Galactic priors. The resulting posteriors show that the lens companions in all systems have median masses in the brown-dwarf regime, and the lenses of two events (KMT-2025-BLG-0922 and KMT-2025-BLG-1056) are consistent with binaries in which both lens components fall within the brown-dwarf mass range. Spanning a wide range of projected separations and distances, these detections illustrate the power of high-cadence microlensing surveys to build a census of brown-dwarf companions, including faint and distant systems beyond the reach of flux-limited methods.
title Candidate Microlensing Brown Dwarfs in Binary Lens Systems from the 2023--2025 Observing Seasons
topic Solar and Stellar Astrophysics
Earth and Planetary Astrophysics
url https://arxiv.org/abs/2604.07932