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Doeon Kim

Researcher at Chungbuk National University

Publications -  79
Citations -  867

Doeon Kim is an academic researcher from Chungbuk National University. The author has contributed to research in topics: Gravitational microlensing & Planet. The author has an hindex of 15, co-authored 66 publications receiving 640 citations. Previous affiliations of Doeon Kim include Korea Astronomy and Space Science Institute.

Papers
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Properties of Central Caustics in Planetary Microlensing

TL;DR: In this paper, the authors derived analytic expressions for the location, size, and shape of the central caustic as a function of the star-planet separation, s, and the planet/star mass ratio, q, under the planetary perturbative approximation and compared the results with those based on numerical computations.
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Asteroid pairs: A complex picture

TL;DR: In this paper, the authors studied a sample of 93 asteroid pairs, i.e., pairs of genetically related asteroids that are on highly similar heliocentric orbits, and derived the absolute magnitude differences of the studied asteroid pairs that provided their mass ratios q.
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Gravitational Microlensing: A Tool for Detecting and Characterizing Free-Floating Planets

TL;DR: In this paper, a similar observational setup was used for the mass determinations of free-floating planets with masses ranging from several Earth masses to several Jupiter masses, which are the populations of planets that have not been previously probed.
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VLT/SPHERE imaging survey of the largest main-belt asteroids: Final results and synthesis

Pierre Vernazza, +69 more
TL;DR: In this article, a high-angular-resolution imaging survey of 42 large main-belt asteroids with VLT/SPHERE/ZIMPOL was conducted to constrain the formation and evolution of a representative sample of large asteroids.
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The Possibility of Detecting Planets in the Andromeda Galaxy

TL;DR: In this article, the authors investigate the feasibility of using a survey to detect planets in M31, and estimate the efficiency of detecting signals produced by planets with various masses and separations from the host star.