S
Seung-Lee Kim
Researcher at Korea Astronomy and Space Science Institute
Publications - 194
Citations - 3699
Seung-Lee Kim is an academic researcher from Korea Astronomy and Space Science Institute. The author has contributed to research in topics: Gravitational microlensing & Light curve. The author has an hindex of 24, co-authored 161 publications receiving 3125 citations. Previous affiliations of Seung-Lee Kim include Universidad Mayor & Korea University of Science and Technology.
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Journal ArticleDOI
OGLE-2019-BLG-1470LABc: Another Microlensing Giant Planet in a Binary System?
Renkun Kuang,Weicheng Zang,Y. K. Jung,Andrzej Udalski,Hongjing Yang,Shude Mao,Michael Albrow,Sun-Ju Chung,Andrew Gould,Cheongho Han,K.-H. Hwang,Yoon-Hyun Ryu,In-Gu Shin,Yossi Shvartzvald,Jennifer C. Yee,Sang-Mok Cha,Dong-Jin Kim,Hyoung-Woo Kim,Seung-Lee Kim,Chung-Uk Lee,Dong-Joo Lee,Yongseok Lee,Byeong-Gon Park,Richard W. Pogge,P. Mr'oz,Jan Skowron,Radosław Poleski,Michał K. Szymański,I. Soszy'nski,P. Pietrukowicz,Szymon Kozłowski,Krzysztof Ulaczyk,K. Rybicki,Patryk Iwanek,Marcin Wrona,Mariusz Gromadzki,Hanyue Wang Shuo Huang Wei Zhu +36 more
TL;DR: The OGLE-2019-BLG-1470 microlensing event was first classified as a normal binary-lens single-source (2L1S) event, but a careful 2L 1S modelling showed that it needed an additional lens or source to fit the observed data as mentioned in this paper .
Posted ContentDOI
OGLE-2019-BLG-0304: Competing Interpretations between a Planet-binary Model and a Binary-source + Binary-lens model
Cheongho Han,Andrzej Udalski,Chung-Uk Lee,Doeon Kim,Yoon-Hyun Ryu,Michael D. Albrow,Sun-Ju Chung,Andrew Gould,Kyu-Ha Hwang,Youn Kil Jung,Hyoun-Woo Kim,In-Gu Shin,Yossi Shvartzvald,Jennifer C. Yee,Weicheng Zang,Sang-Mok Cha,Dong-Jin Kim,Seung-Lee Kim,Dong-Joo Lee,Yongseok Lee,Byeong-Gon Park,Richard W. Pogge,Przemek Mróz,Michał K. Szymański,Jan Skowron,Radosław Poleski,Igor Soszyński,Paweł Pietrukowicz,Szymon Kozłowski,Krzysztof Ulaczyk,Krzysztof A. Rybicki,Patryk Iwanek,Marcin Wrona,Mariusz Gromadzki +33 more
TL;DR: In this paper, the OGLE-2019-BLG-0304 microlensing event was analyzed and the authors found that the residuals can be explained by the presence of either a planetary companion located close to the primary of the binary lens (3L1S model) or an additional close companion to the source (2L2S model).
Journal ArticleDOI
Observational Properties of GSC 2855-0585 in the Vicinity of the Eclipsing Binary V432 Per
TL;DR: In this article, the authors detected the same light variations with a period of about 2.406 days in all B, V, and R bands of GSC 2855-0585 and confirmed the period and transitlike features were confirmed by photometric follow-up observations at a predicted epoch in 2010 November.
Posted Content
Systematic KMTNet Planetary Anomaly Search, Paper II: Five New $q<2\times 10^{-4}$ Mass-ratio Planets
Kyu-Ha Hwang,Weicheng Zang,Andrew Gould,Andrzej Udalski,Ian A. Bond,Hongjing Yang,Shude Mao,Michael D. Albrow,Sun-Ju Chung,Cheongho Han,Youn Kil Jung,Yoon-Hyun Ryu,In-Gu Shin,Yossi Shvartzvald,Jennifer C. Yee,Sang-Mok Cha,Dong-Jin Kim,Hyoun-Woo Kim,Seung-Lee Kim,Chung-Uk Lee,Dong-Joo Lee,Yongseok Lee,Byeong-Gon Park,Richard W. Pogge,Przemek Mróz,Radek Poleski,Jan Skowron,Michał K. Szymański,Igor Soszyński,Paweł Pietrukowicz,Szymon Kozłowski,Krzysztof Ulaczyk,Krzysztof A. Rybicki,Patryk Iwanek,Marcin Wrona,Mariusz Gromadzki,Fumio Abe,Richard K. Barry,David P. Bennett,Aparna Bhattacharya,Hirosame Fujii,Akihiko Fukui,Yuki Hirao,Yoshitaka Itow,Rintaro Kirikawa,Iona Kondo,Naoki Koshimoto,Brandon Munford,Yutaka Matsubara,Shota Miyazaki,Yasushi Muraki,Greg Olmschenk,Clément Ranc,Nicholas J. Rattenbury,Yuki Satoh,Hikaru Shoji,Stela Ishitani Silva,Takahiro Sumi,Daisuke Suzuki,Paul J. Tristram,Atsunori Yonehara,Xiangyu Zhang,Wei Zhu,Matthew T. Penny,Pascal Fouqué +64 more
TL;DR: Zhang et al. as mentioned in this paper applied the automated anomaly-finder algorithm to 2018-2019 light curves from the six KMTNet prime fields, with cadences $\Gamma \geq 2\,{\rm hr}^{-1}".
Journal ArticleDOI
KMT-2016-BLG-2052L: Microlensing Binary Composed of M Dwarfs Revealed from a Very Long Timescale Event
Cheongho Han,Youn Kil Jung,Yossi Shvartzvald,Michael D. Albrow,Sun-Ju Chung,Sun-Ju Chung,Andrew Gould,Andrew Gould,Andrew Gould,Kyu-Ha Hwang,Doeon Kim,Chung-Uk Lee,Woong-Tae Kim,Hyoun-Woo Kim,Yoon-Hyun Ryu,In-Gu Shin,Jennifer C. Yee,Chun-Hwey Kim,Sang-Mok Cha,Sang-Mok Cha,Seung-Lee Kim,Seung-Lee Kim,Dong-Jin Kim,Dong-Joo Lee,Yongseok Lee,Yongseok Lee,Byeong-Gon Park,Byeong-Gon Park,Richard W. Pogge,Charles Beichman,Geoff Bryden,Sebastiano Calchi Novati,B. Scott Gaudi,Calen B. Henderson,T. P. Matthew,Savannah Jacklin +35 more
TL;DR: In this paper, the mass of a binary microlensing event KMT-2016-BLG-2052 was determined from the combined measurements of the microlens parallax πE and angular Einstein radius θE.