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Ho Seong Hwang

5 papers hereh-index 343 citations7 works total

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

author position
  • middle author4
  • last author1

Across the 5 of 5 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA3
  • astro-ph.CO2
same name
  • Ho Seong Hwang — 35 papers, h 7
  • Ho Seong Hwang — 6 papers
  • Ho Seong Hwang — 5 papers, h 1
  • Ho Seong Hwang — 5 papers, h 1
  • Ho Seong Hwang — 2 papers, h 0
  • Ho Seong Hwang — 1 paper, h 1

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
20142026
most citedConstraining the galaxy mass content in the core of A383 using velocity dispersion measurements for individual cluster members

36 citations · 59 across the 5 of their papers we have counts for

collaborators
Showing 2026Show all

1 paper · 1 filter

astro-ph.CO2026

New classification method for the dynamical state of galaxy clusters with a Gaussian mixture model

Hyowon Kim, Marco Canducci, Rory Smith +5

Galaxy clusters are the largest gravitationally bound systems, and they continue their growth through mergers in a hierarchical ΛCDM Universe. Therefore, we can describe the merger…

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