Systematic Reanalysis of KMTNet Microlensing Events. II. Two New Planets in Giant-source Events

Abstract In this work, we continue to apply the updated KMTNet tender-love care photometric pipeline to historical microlensing events. We apply the pipeline to a subsample of events from the KMTNet database, which we refer to as the giant source sample. Leveraging the improved photometric data, we conduct a systematic search for anomalies within this sample. The search successfully uncovers four new planet-like anomalies and recovers two previously known planetary signals. After detailed analysis, two of the newly discovered anomalies are confirmed as clear planets: KMT-2019-BLG-0578 and KMT-2021-BLG-0736. Their planet-to-host mass ratios are q ∼ 4 × 10 −3 and q ∼ 1 × 10 −4 , respectively. Another event, OGLE-2018-BLG-0421 (KMT-2018-BLG-0831), remains ambiguous. Both a stellar companion and a giant planet in the lens system could potentially explain the observed anomaly. The anomaly signal of the last event, MOA-2022-BLG-038 (KMT-2022-BLG-2342), is attributed to an extra source star. Within this sample, our procedure doubles the number of confirmed planets, demonstrating a significant enhancement in the survey sensitivity.

Authors

Publication Details

Journal
The Astronomical Journal
Published
2025-05-07
DOI
https://doi.org/10.3847/1538-3881/adc73e
Citations
2
Primary Topic
Astro and Planetary Science
Type
article
Field-Weighted Citation Impact
2.31

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article

Systematic Reanalysis of KMTNet Microlensing Events. II. Two New Planets in Giant-source Events

Sang-Mok Cha, Yongseok Lee, I. Soszyński, Michael D. Albrow et al.
2 citations
The Astronomical Journal
Astro and Planetary Science
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article

Systematic Reanalysis of KMTNet Microlensing Events. II. Two New Planets in Giant-source Events

Sang-Mok Cha, Yongseok Lee, I. Soszyński, Michael D. Albrow, Weicheng Zang, Hongjing Yang, Yuki Satoh, Y. Itow, Sean K. Terry, Kyu‐Ha Hwang, Akihiko Fukui, Shude Mao, Hibiki Yama, ‪Clément Ranc, Naoto Hamasaki, D. P. Bennett, M. K. Szymański, J. Skowron, Byeong-Gon Park, R. Poleski, Yoon-Hyun Ryu, Yossi Shvartzvald, Seung‐Lee Kim, Chung‐Uk Lee, Dong-Joo Lee, Aparna Bhattacharya, Naoki Koshimoto, Sun‐Ju Chung, Cheongho Han, T. Sumi, Aikaterini Vandorou, A. Udalski, Youn Kil Jung, Qiyue Qian, Patryk Iwanek, Shota Miyazaki, Stela Ishitani Silva, Jiyuan Zhang, I. A. Bond, P. Pietrukowicz, P. Mróz, K. Ulaczyk, Nicholas J. Rattenbury, Hyoun-Woo Kim, In-Gu Shin, Greg Olmschenk, Yuki Hirao, Jennifer C. Yee, Y. Matsubara, Dong-Jin Kim, P. J. Tristram, S. Kozłowski, Richard W. Pogge, Ryusei Hamada, Marcin Wrona, Y. Muraki, Kansuke Nunota, Tutumi Nagai, Krzysztof A. Rybicki, Daisuke Suzuki, Fumio Abe, Shunya Hamada, Andrew Gould, Ken Bando
article en
2 citations

Abstract

Abstract In this work, we continue to apply the updated KMTNet tender-love care photometric pipeline to historical microlensing events. We apply the pipeline to a subsample of events from the KMTNet database, which we refer to as the giant source sample. Leveraging the improved photometric data, we conduct a systematic search for anomalies within this sample. The search successfully uncovers four new planet-like anomalies and recovers two previously known planetary signals. After detailed analysis, two of the newly discovered anomalies are confirmed as clear planets: KMT-2019-BLG-0578 and KMT-2021-BLG-0736. Their planet-to-host mass ratios are q ∼ 4 × 10 −3 and q ∼ 1 × 10 −4 , respectively. Another event, OGLE-2018-BLG-0421 (KMT-2018-BLG-0831), remains ambiguous. Both a stellar companion and a giant planet in the lens system could potentially explain the observed anomaly. The anomaly signal of the last event, MOA-2022-BLG-038 (KMT-2022-BLG-2342), is attributed to an extra source star. Within this sample, our procedure doubles the number of confirmed planets, demonstrating a significant enhancement in the survey sensitivity.

The Astronomical JournalVol. 169(6)
National Science Foundation, National Natural Science Foundation of China, China Postdoctoral Science Foundation, Korea Astronomy and Space Science Institute, Tsinghua University, Ministry of Science and ICT, South Korea, Korea Research Environment Open Network, Japan Society for the Promotion of Science
Openalex Percentile: Top 12%
Astro and Planetary Science
2.31
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