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.
Papers
More filters
Journal ArticleDOI
KMT-2017-BLG-2820 and the Nature of the Free-Floating Planet Population
Yoon-Hyun Ryu,Przemek Mróz,Andrew Gould,Kyu-Ha Hwang,Hyoun-Woo Kim,Jennifer C. Yee,Michael D. Albrow,Sun-Ju Chung,Youn Kil Jung,In-Gu Shin,Yossi Shvartzvald,Weicheng Zang,Sang-Mok Cha,Dong-Jin Kim,Seung-Lee Kim,Chung-Uk Lee,Dong-Joo Lee,Yongseok Lee,Byeong-Gon Park,Cheongho Han,Richard W. Pogge,Andrzej Udalski,Radek Poleski,Jan Skowron,Michał K. Szymański,Igor Soszyński,Paweł Pietrukowicz,Szymon Kozłowski,Krzysztof Ulaczyk,Krzysztof A. Rybicki,Patryk Iwanek +30 more
TL;DR: In this paper, the authors report a new free-floating planet (FFP) candidate, KMT-2017-BLG-2820, with Einstein radius $t_\e=6.5\,$hr.
Posted Content
OGLE-2019-BLG-0960Lb: The Smallest Microlensing Planet
Jennifer C. Yee,Weicheng Zang,Andrzej Udalski,Yoon-Hyun Ryu,Jonathan T. Green,Steve Hennerley,Andrew Marmont,Takahiro Sumi,Shude Mao,Mariusz Gromadzki,Przemek Mróz,Jan Skowron,Radosław Poleski,Michał K. Szymański,Igor Soszyński,Paweł Pietrukowicz,Szymon Kozłowski,Krzysztof Ulaczyk,Krzysztof A. Rybicki,Patryk Iwanek,Marcin Wrona,Michael D. Albrow,Sun-Ju Chung,Andrew Gould,Cheongho Han,Kyu-Ha Hwang,Youn Kil Jung,Hyoun-Woo Kim,In-Gu Shin,Yossi Shvartzvald,Sang-Mok Cha,Dong-Jin Kim,Seung-Lee Kim,Chung-Uk Lee,Dong-Joo Lee,Yongseok Lee,Byeong-Gon Park,Richard W. Pogge,Etienne Bachelet,G. W. Christie,M. Hundertmark,Dan Maoz,Jennie McCormick,Tim Natusch,Matthew T. Penny,Rachel Street,Yiannis Tsapras,Charles Beichman,Geoffery Bryden,Sebastiano Calchi Novati,Sean Carey,B. Scott Gaudi,Calen B. Henderson,Samson A. Johnson,Wei Zhu,Ian A. Bond,Fumio Abe,Richard K. Barry,David P. Bennett,Aparna Bhattacharya,Martin Donachie,Hirosane Fujii,Akihiko Fukui,Yuki Hirao,Stela Ishitani Silva,Yoshitaka Itow,Rintaro Kirikawa,Iona Kondo,Naoki Koshimoto,Man Cheung Alex Li,Yutaka Matsubara,Yasushi Muraki,Shota Miyazaki,Greg Olmschenk,Clément Ranc,Nicholas J. Rattenbury,Yuki Satoh,Hikaru Shoji,Daisuke Suzuki,Yuzuru Tanaka,Paul J. Tristram,Tsubasa Yamawaki,Atsunori Yonehara +82 more
TL;DR: The OGLE-2019-BLG-0960 microlensing system as discussed by the authors contains the smallest mass-ratio micro-lensing planet found to date (q = 1.2--1.6 x 10^{-5} at 1-sigma).
Journal ArticleDOI
One Planet or Two Planets? The Ultra-sensitive Extreme-magnification Microlensing Event KMT-2019-BLG-1953
Cheongho Han,Doeon Kim,Youn Kil Jung,Andrew Gould,Ian A. Bond,Michael D. Albrow,Sun-Ju Chung,Kyu-Ha Hwang,Chung-Uk Lee,Yoon-Hyun Ryu,In-Gu Shin,Yossi Shvartzvald,Jennifer C. Yee,Weicheng Zang,Sang-Mok Cha,Dong-Jin Kim,Hyoun-Woo Kim,Seung-Lee Kim,Dong-Joo Lee,Yongseok Lee,Byeong-Gon Park,Richard W. Pogge,Woong-Tae Kim,Fumio Abe,Richard K. Barry,David P. Bennett,Aparna Bhattacharya,Martin Donachie,Hirosane Fujii,Akihiko Fukui,Yoshitaka Itow,Yuki Hirao,Rintaro Kirikawa,Iona Kondo,Naoki Koshimoto,Man Cheung Alex Li,Yutaka Matsubara,Yasushi Muraki,Shota Miyazaki,Masayuki Nagakane,Clément Ranc,Nicholas J. Rattenbury,Yuki Satoh,Hikaru Shoji,Haruno Suematsu,Takahiro Sumi,Daisuke Suzuki,Yuzuru Tanaka,Paul J. Tristram,Tsubasa Yamawaki,Atsunori Yonehara +50 more
TL;DR: In this article, the authors presented the analysis of a very high-magnification microlensing event KMT-2019-BLG-1953, where the residuals from a single-lens single-source (1L1S) model exhibited small but obvious deviations in the peak region.
Journal ArticleDOI
Detection of Variable Stars in the Open Cluster M11 Using Difference Image Analysis Pipeline
TL;DR: In this article, a photometric pipeline using the difference image analysis (DIA) method was developed for the photometry of star dense field such as the Galactic bulge, which was used for wide field survey.
Journal ArticleDOI
Photometric Properties of the Variable Star LZ Herculis
TL;DR: In this article, the BV photometric results of the variable star LZ Her were presented, which showed that it is not an SX Phe star but rather a W UMa-type eclipsing binary, as reported by Garrido et al.