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MOA-2022-BLG-033Lb, KMT-2023-BLG-0119Lb, and KMT-2023-BLG-1896Lb: Three low mass-ratio microlensing planets detected through dip signals.

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Title: MOA-2022-BLG-033Lb, KMT-2023-BLG-0119Lb, and KMT-2023-BLG-1896Lb: Three low mass-ratio microlensing planets detected through dip signals.
Authors: Han, Cheongho1 (AUTHOR) cheongho@astroph.chungbuk.ac.kr, Bond, Ian A.2 (AUTHOR), Jung, Youn Kil3 (AUTHOR), Albrow, Michael D.4 (AUTHOR), Chung, Sun-Ju3 (AUTHOR), Gould, Andrew5,6 (AUTHOR), Hwang, Kyu-Ha3 (AUTHOR), Lee, Chung-Uk3 (AUTHOR), Ryu, Yoon-Hyun3 (AUTHOR), Shvartzvald, Yossi7 (AUTHOR), Shin, In-Gu8 (AUTHOR), Yee, Jennifer C.8 (AUTHOR), Yang, Hongjing9 (AUTHOR), Zang, Weicheng8,9 (AUTHOR), Cha, Sang-Mok3,10 (AUTHOR), Kim, Doeon1 (AUTHOR), Kim, Dong-Jin3 (AUTHOR), Kim, Seung-Lee3 (AUTHOR), Lee, Dong-Joo3 (AUTHOR), Lee, Yongseok3,10 (AUTHOR)
Source: Astronomy & Astrophysics / Astronomie et Astrophysique. 2025, Vol. 694, p1-9. 9p.
Database: Academic Search Ultimate
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  Data: MOA-2022-BLG-033Lb, KMT-2023-BLG-0119Lb, and KMT-2023-BLG-1896Lb: Three low mass-ratio microlensing planets detected through dip signals.
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