M
Myung-Jin Kim
Researcher at Korea Astronomy and Space Science Institute
Publications - 62
Citations - 952
Myung-Jin Kim is an academic researcher from Korea Astronomy and Space Science Institute. The author has contributed to research in topics: Asteroid & Geometric albedo. The author has an hindex of 13, co-authored 62 publications receiving 800 citations. Previous affiliations of Myung-Jin Kim include Yonsei University.
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Journal ArticleDOI
Comparative study of transrectal ultrasonography, pelvic computerized tomography, and magnetic resonance imaging in preoperative staging of rectal cancer.
TL;DR: Both transrectal ultrasonography and magnetic resonance imaging with endorectal coil exhibited similar accuracy and were superior to conventional computed tomography in preoperative assessment of depth of invasion and adjacent organ invasion.
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Hayabusa-2 Mission Target Asteroid 162173 Ryugu (1999 JU3): Searching for the Object's Spin-Axis Orientation
T. G. Müller,Josef Ďurech,Masateru Ishiguro,Michael Mueller,Thomas Krühler,Hongu Yang,Myung-Jin Kim,Laurence O'Rourke,Fumihiko Usui,Cs. Kiss,Bruno Altieri,Benoit Carry,Young-Jun Choi,Marco Delbo,Josh Emery,Jochen Greiner,Sunao Hasegawa,Joseph L. Hora,Fabian Knust,Daisuke Kuroda,David J. Osip,Arne Rau,Andrew S. Rivkin,Patricia Schady,Joanna Thomas-Osip,David E. Trilling,Seitaro Urakawa,Esa Vilenius,Paul R. Weissman,P. Zeidler +29 more
TL;DR: In this paper, the authors combine radiometric and lightcurve inversion techniques in different ways to find the object's key physical and thermal parameters, and find that the solution which best matches their data sets leads to this C class asteroid having a retrograde rotation with a spin-axis orientation of (lambda = 310-340 deg; beta = -40+/-15 deg) in ecliptic coordinates, an effective diameter (of an equal-volume sphere) of 850 to 880 m, a geometric albedo of 0.044 to 0.050 and a
Journal ArticleDOI
Hayabusa-2 mission target asteroid 162173 Ryugu (1999 JU3): Searching for the object's spin-axis orientation
T. G. Müller,Josef Ďurech,Masateru Ishiguro,Michael Mueller,Thomas Krühler,Hongu Yang,Myung-Jin Kim,Laurence O'Rourke,Fumihiko Usui,Cs. Kiss,Bruno Altieri,Benoit Carry,Young-Jun Choi,Marco Delbo,Josh Emery,Jochen Greiner,Sunao Hasegawa,Joseph L. Hora,Fabian Knust,Daisuke Kuroda,David J. Osip,Arne Rau,Andrew S. Rivkin,Patricia Schady,Joanna Thomas-Osip,David E. Trilling,Seitaro Urakawa,Esa Vilenius,Paul R. Weissman,P. Zeidler +29 more
TL;DR: In this article, the authors combine radiometric and lightcurve inversion techniques in different ways to find the object's spin-axis orientation, its shape and to improve the quality of the key physical and thermal parameters.
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Stardust-NExT, Deep Impact, and the accelerating spin of 9P/Tempel 1
Michael J. S. Belton,Karen J. Meech,Steven R. Chesley,Jana Pittichova,Brian Carcich,Michal Drahus,Alan W. Harris,S. D. Gillam,Joseph Veverka,Nicholas Mastrodemos,William M. Owen,Michael F. A'Hearn,Stefano Bagnulo,J. M. Bai,L. Barrera,Fabienne A. Bastien,James M. Bauer,J. Bedient,Bhuwan C. Bhatt,Hermann Boehnhardt,Noah Brosch,Marc W. Buie,Pablo Candia,Wen Ping Chen,P. Chiang,Young-Jun Choi,Anita L. Cochran,C. J. Crockett,S. R. Duddy,Tony L. Farnham,Yan Fernandez,Pedro J. Gutiérrez,Olivier Hainaut,Donald Hampton,Kimberly A. Herrmann,Henry H. Hsieh,M. A. Kadooka,H. M. Kaluna,Jacqueline V. Keane,Myung-Jin Kim,Kenneth P. Klaasen,Jan T. Kleyna,Kevin Krisciunas,Luisa Lara,Tod R. Lauer,Jian-Yang Li,Javier Licandro,Javier Licandro,Carey M. Lisse,Stephen C. Lowry,Lucy A. McFadden,Nicholas Moskovitz,Beatrice E. A. Mueller,David Polishook,N. S. Raja,Timm Riesen,D. K. Sahu,Nalin H. Samarasinha,G. Sarid,Tomohiko Sekiguchi,Sarah Sonnett,Nicholas B. Suntzeff,Brian W. Taylor,Brian W. Taylor,Peter C. Thomas,Gian Paolo Tozzi,R. Vasundhara,Jean-Baptiste Vincent,Lawrence H. Wasserman,Bryant Webster-Schultz,Bin Yang,T. Zenn,Haibin Zhao +72 more
TL;DR: The evolution of the spin rate of Comet 9P/Tempel 1 through two perihelion passages (in 2000 and 2005) is determined from 1922 Earth-based observations taken over a period of 13 year as part of a World Wide Observations campaign and from 2888 observations taken for 50 days from the Deep Impact spacecraft as mentioned in this paper.
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Spectral and rotational properties of near-Earth asteroid (162173) Ryugu, target of the Hayabusa2 sample return mission
D. Perna,M. A. Barucci,Masateru Ishiguro,Alvaro Alvarez-Candal,D. Kuroda,Makoto Yoshikawa,Myung-Jin Kim,Sonia Fornasier,Sunao Hasegawa,Dong-Goo Roh,T. G. Müller,Yoonyoung Kim +11 more
TL;DR: In this paper, the authors obtained high-quality photometric time-series data with the FORS2 instrument at the Very Large Telescope of the European Southern Observatory (ESO-VLT, Chile), and also acquired four visible spectra and three X-shooter spectra in the 0.35−2.15 μ m range, at different rotational phases.