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Ji-hoon Kim

18 papers hereh-index 9287 citations23 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • first author2
  • middle author14
  • last author1

Across the 17 of 18 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA16
  • astro-ph.CO2
same name
  • Ji-Hoon Kim — 22 papers, h 9
  • Ji-hoon Kim — 16 papers, h 47
  • Ji-Hoon Kim — 11 papers, h 12
  • Ji-hoon Kim — 8 papers, h 2
  • Ji-Hoon Kim — 3 papers, h 14
  • Ji-Hoon Kim — 2 papers, h 2

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
20122026
most citedThe AGORA High-Resolution Galaxy Simulations Comparison Project

282 citations · 474 across the 18 of their papers we have counts for

collaborators
Showing 2025Show all

3 papers · 1 filter

astro-ph.GA2025★ 3 cited

The AGORA High-resolution Galaxy Simulations Comparison Project. X: Formation and Evolution of Galaxies at the High-redshift Frontier

Hyeonyong Kim, Ji-hoon Kim, Minyong Jung +22

Recent observations from JWST have revealed unexpectedly luminous galaxies, exhibiting stellar masses and luminosities significantly higher than predicted by theoretical models at…

astro-ph.GA2025★ 10 cited

The AGORA High-Resolution Galaxy Simulations Comparison Project VII: Satellite quenching in zoom-in simulation of a Milky Way-mass halo

R. Rodríguez-Cardoso, S. Roca-Fàbrega, Minyong Jung +19

Context: Satellite galaxies experience multiple physical processes when interacting with their host halos, often leading to the quenching of star formation. In the Local Group (LG)…

astro-ph.GA2025★ 4 cited

The AGORA High-resolution Galaxy Simulations Comparison Project. VIII: Disk Formation and Evolution of Simulated Milky Way Mass Galaxy Progenitors at 1<z<5

Minyong Jung, Ji-hoon Kim, Thinh H. Nguyen +24

We investigate how differences in the stellar feedback produce disks with different morphologies in Milky Way-like progenitors over 1 ≤z≤5, using eight state-of-the-art…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.