Ji-hoon Kim

Assistant/Associate Professor

Seoul National University

South Korea

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About

Ji-hoon Kim is an Assistant Professor at Seoul National University, South Korea. His research focuses on the formation and evolution of compact binaries, galaxy simulations, and cosmological parameters using advanced simulation techniques. Recent publications include work on dark-matter-deficient galaxy formation and the dynamics of star clusters within galaxies.

Articles (19)

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2025

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2022

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2022

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2021

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2020

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2020

Collaborators (7)

Yuan-Sen Ting

Associate Professor (tenured)

Australian National University

AUSTRALIA

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Boon Kiat Oh

Seoul National University

SOUTH KOREA

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Greg Bryan

Professor

Columbia University

UNITED STATES

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Rainer Spurzem

Professor

Heidelberg University

GERMANY

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Hyung Mok Lee

Prof.

Seoul National University

SOUTH KOREA

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Kentaro Nagamine

Professor

Osaka University

JAPAN

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Juhan Kim

Korea Institute for Advanced Study

SOUTH KOREA

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Ji-hoon Kim

Research Interests

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About

Articles (19)

Formation and Evolution of Compact Binaries Containing Intermediate-mass Black Holes in Dense Star Clusters

The AGORA High-Resolution Galaxy Simulations Comparison Project

The AGORA High-resolution Galaxy Simulations Comparison Project. IV. Halo and Galaxy Mass Assembly in a Cosmological Zoom-in Simulation at z ≤ 2

Multiple Beads on a String: Dark-matter-deficient Galaxy Formation in a Mini-Bullet Satellite–Satellite Galaxy Collision

Merger-tree-based Galaxy Matching: A Comparative Study across Different Resolutions

The AGORA High-resolution Galaxy Simulations Comparison Project. V. Satellite Galaxy Populations in a Cosmological Zoom-in Simulation of a Milky Way–Mass Halo

The AGORA High-resolution Galaxy Simulations Comparison Project. VI. Similarities and Differences in the Circumgalactic Medium

Inferring Cosmological Parameters on SDSS via Domain-generalized Neural Networks and Light-cone Simulations

Evolution of Star Clusters within Galaxies Using Self-consistent Hybrid Hydro/N-body Simulations

Star Formation Variability as a Probe for the Baryon Cycle within Galaxies

Calibrating Cosmological Simulations with Implicit Likelihood Inference Using Galaxy Growth Observables

Growth of a Massive Black Hole in a Dense Star Cluster Via Tidal Disruption Accretion

Machine-guided exploration and calibration of astrophysical simulations

Giant collision created galaxies devoid of dark matter

Dark Matter Deficient Galaxies and Their Member Star Clusters Form Simultaneously during High-velocity Galaxy Collisions in 1.25 pc Resolution Simulations

How Metals Are Transported in and out of a Galactic Disk: Dependence on the Hydrodynamic Schemes in Numerical Simulations

The AGORA High-resolution Galaxy Simulations Comparison Project. III. Cosmological Zoom-in Simulation of a Milky Way–mass Halo

Dark Matter Deficient Galaxies Produced via High-velocity Galaxy Collisions in High-resolution Numerical Simulations

Self-consistent proto-globular cluster formation in cosmological simulations of high-redshift galaxies

Collaborators (7)

Yuan-Sen Ting

Boon Kiat Oh

Greg Bryan

Rainer Spurzem

Hyung Mok Lee

Kentaro Nagamine

Juhan Kim

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