OGLE-2018-BLG-0971, MOA-2023-BLG-065, and OGLE-2023-BLG-0136: Microlensing events with prominent orbital effects

Fuente: arXiv
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Hauptverfasser: Han, Cheongho, Udalski, Andrzej, Bond, Ian A., Lee, Chung-Uk, Gould, Andrew, Albrow, Michael D., Chung, Sun-Ju, Hwang, Kyu-Ha, Jung, Youn Kil, Kim, Hyoun-Woo, Ryu, Yoon-Hyun, Shvartzvald, Yossi, Shin, In-Gu, Yee, Jennifer C., Yang, Hongjing, Zang, Weicheng, Cha, Sang-Mok, Kim, Doeon, Kim, Dong-Jin, Kim, Seung-Lee, Lee, Dong-Joo, 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, Barry, Richard, Bennett, David P., Bhattacharya, Aparna, Fujii, Hirosame, Fukui, Akihiko, Hamada, Ryusei, Hirao, Yuki, Silva, Stela Ishitani, Itow, Yoshitaka, Kirikawa, Rintaro, Koshimoto, Naoki, Matsubara, Yutaka, Miyazaki, Shota, Muraki, Yasushi, Olmschenk, Greg, Ranc, Clément, Rattenbury, Nicholas J., Satoh, Yuki, Sumi, Takahiro, Suzuki, Daisuke, Tomoyoshi, Mio, Tristram, Paul J., Vandorou, Aikaterini, Yama, Hibiki, Yamashita, Kansuke
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Veröffentlicht: 2024
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author Han, Cheongho
Udalski, Andrzej
Bond, Ian A.
Lee, Chung-Uk
Gould, Andrew
Albrow, Michael D.
Chung, Sun-Ju
Hwang, Kyu-Ha
Jung, Youn Kil
Kim, Hyoun-Woo
Ryu, Yoon-Hyun
Shvartzvald, Yossi
Shin, In-Gu
Yee, Jennifer C.
Yang, Hongjing
Zang, Weicheng
Cha, Sang-Mok
Kim, Doeon
Kim, Dong-Jin
Kim, Seung-Lee
Lee, Dong-Joo
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
Barry, Richard
Bennett, David P.
Bhattacharya, Aparna
Fujii, Hirosame
Fukui, Akihiko
Hamada, Ryusei
Hirao, Yuki
Silva, Stela Ishitani
Itow, Yoshitaka
Kirikawa, Rintaro
Koshimoto, Naoki
Matsubara, Yutaka
Miyazaki, Shota
Muraki, Yasushi
Olmschenk, Greg
Ranc, Clément
Rattenbury, Nicholas J.
Satoh, Yuki
Sumi, Takahiro
Suzuki, Daisuke
Tomoyoshi, Mio
Tristram, Paul J.
Vandorou, Aikaterini
Yama, Hibiki
Yamashita, Kansuke
author_facet Han, Cheongho
Udalski, Andrzej
Bond, Ian A.
Lee, Chung-Uk
Gould, Andrew
Albrow, Michael D.
Chung, Sun-Ju
Hwang, Kyu-Ha
Jung, Youn Kil
Kim, Hyoun-Woo
Ryu, Yoon-Hyun
Shvartzvald, Yossi
Shin, In-Gu
Yee, Jennifer C.
Yang, Hongjing
Zang, Weicheng
Cha, Sang-Mok
Kim, Doeon
Kim, Dong-Jin
Kim, Seung-Lee
Lee, Dong-Joo
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
Barry, Richard
Bennett, David P.
Bhattacharya, Aparna
Fujii, Hirosame
Fukui, Akihiko
Hamada, Ryusei
Hirao, Yuki
Silva, Stela Ishitani
Itow, Yoshitaka
Kirikawa, Rintaro
Koshimoto, Naoki
Matsubara, Yutaka
Miyazaki, Shota
Muraki, Yasushi
Olmschenk, Greg
Ranc, Clément
Rattenbury, Nicholas J.
Satoh, Yuki
Sumi, Takahiro
Suzuki, Daisuke
Tomoyoshi, Mio
Tristram, Paul J.
Vandorou, Aikaterini
Yama, Hibiki
Yamashita, Kansuke
contents We undertake a project to reexamine microlensing data gathered from high-cadence surveys. The aim of the project is to reinvestigate lensing events with light curves exhibiting intricate anomaly features associated with caustics, yet lacking prior proposed models to explain these features. Through detailed reanalyses considering higher-order effects, we identify that accounting for orbital motions of lenses is vital in accurately explaining the anomaly features observed in the light curves of the lensing events OGLE-2018-BLG-0971, MOA-2023-BLG-065, and OGLE-2023-BLG-0136. We estimate the masses and distances to the lenses by conducting Bayesian analyses using the lensing parameters of the newly found lensing solutions. From these analyses, we identify that the lenses of the events OGLE-2018-BLG-0971 and MOA-2023-BLG-065 are binaries composed of M dwarfs, while the lens of OGLE-2023-BLG-0136 is likely to be a binary composed of an early K-dwarf primary and a late M-dwarf companion. For all lensing events, the probability of the lens residing in the bulge is considerably higher than that of it being located in the disk.
format Preprint
id arxiv_https___arxiv_org_abs_2404_05912
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle OGLE-2018-BLG-0971, MOA-2023-BLG-065, and OGLE-2023-BLG-0136: Microlensing events with prominent orbital effects
Han, Cheongho
Udalski, Andrzej
Bond, Ian A.
Lee, Chung-Uk
Gould, Andrew
Albrow, Michael D.
Chung, Sun-Ju
Hwang, Kyu-Ha
Jung, Youn Kil
Kim, Hyoun-Woo
Ryu, Yoon-Hyun
Shvartzvald, Yossi
Shin, In-Gu
Yee, Jennifer C.
Yang, Hongjing
Zang, Weicheng
Cha, Sang-Mok
Kim, Doeon
Kim, Dong-Jin
Kim, Seung-Lee
Lee, Dong-Joo
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
Barry, Richard
Bennett, David P.
Bhattacharya, Aparna
Fujii, Hirosame
Fukui, Akihiko
Hamada, Ryusei
Hirao, Yuki
Silva, Stela Ishitani
Itow, Yoshitaka
Kirikawa, Rintaro
Koshimoto, Naoki
Matsubara, Yutaka
Miyazaki, Shota
Muraki, Yasushi
Olmschenk, Greg
Ranc, Clément
Rattenbury, Nicholas J.
Satoh, Yuki
Sumi, Takahiro
Suzuki, Daisuke
Tomoyoshi, Mio
Tristram, Paul J.
Vandorou, Aikaterini
Yama, Hibiki
Yamashita, Kansuke
Solar and Stellar Astrophysics
Earth and Planetary Astrophysics
Instrumentation and Methods for Astrophysics
We undertake a project to reexamine microlensing data gathered from high-cadence surveys. The aim of the project is to reinvestigate lensing events with light curves exhibiting intricate anomaly features associated with caustics, yet lacking prior proposed models to explain these features. Through detailed reanalyses considering higher-order effects, we identify that accounting for orbital motions of lenses is vital in accurately explaining the anomaly features observed in the light curves of the lensing events OGLE-2018-BLG-0971, MOA-2023-BLG-065, and OGLE-2023-BLG-0136. We estimate the masses and distances to the lenses by conducting Bayesian analyses using the lensing parameters of the newly found lensing solutions. From these analyses, we identify that the lenses of the events OGLE-2018-BLG-0971 and MOA-2023-BLG-065 are binaries composed of M dwarfs, while the lens of OGLE-2023-BLG-0136 is likely to be a binary composed of an early K-dwarf primary and a late M-dwarf companion. For all lensing events, the probability of the lens residing in the bulge is considerably higher than that of it being located in the disk.
title OGLE-2018-BLG-0971, MOA-2023-BLG-065, and OGLE-2023-BLG-0136: Microlensing events with prominent orbital effects
topic Solar and Stellar Astrophysics
Earth and Planetary Astrophysics
Instrumentation and Methods for Astrophysics
url https://arxiv.org/abs/2404.05912