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Chung-Uk Lee

Researcher at Korea Astronomy and Space Science Institute

Publications -  235
Citations -  3087

Chung-Uk Lee 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 21, co-authored 198 publications receiving 2510 citations. Previous affiliations of Chung-Uk Lee include Max Planck Society & Korea University of Science and Technology.

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Journal ArticleDOI

Kmtnet: a network of 1.6 m wide-field optical telescopes installed at three southern observatories

Seung-Lee Kim, +8 more
- 29 Feb 2016 - 
TL;DR: The Korea Microlensing Telescope Network (KMTNet) as mentioned in this paper is a wide-field photometric system installed by the Korea Astronomy and Space Science Institute (KASI).
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THE sdB+M ECLIPSING SYSTEM HW VIRGINIS AND ITS CIRCUMBINARY PLANETS

Jae Woo Lee, +7 more
- 28 Jan 2009 - 
TL;DR: For the very short period subdwarf B eclipsing binary HW Vir, this article presented new CCD photometry made from 2000 through 2008, showing sharp eclipses and a striking reflection effect, were analyzed simultaneously with previously published radial velocity data.
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Multi-colour optical monitoring of eight red blazars

Minfeng Gu, +6 more
- 01 Apr 2006 - 
TL;DR: In this paper, the authors present the observational results of multi-colour optical monitoring of eight red blazars from 2003 September to 2004 February, and investigate the relationship between the colour index and source brightness for each source.
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Distance and Properties of NGC 4993 as the Host Galaxy of the Gravitational-wave Source GW170817

Myungshin Im, +12 more
- 26 Oct 2017 - 
TL;DR: In this paper, the authors analyzed the multi-wavelength data to characterize the host galaxy property and its distance to examine if the properties of NGC 4993 are consistent with this picture.
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Distance and properties of NGC 4993 as the host galaxy of a gravitational wave source, GW170817

Myungshin Im, +12 more
- 16 Oct 2017 - 
TL;DR: In this article, the authors analyzed the multi-wavelength data to characterize the host galaxy property and its distance to examine if the properties of NGC 4993 are consistent with this picture.