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researcher

Kun Xu

4 papers here

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

author position
  • sole author1
  • first author1
  • middle author2

Across the 4 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph.CO2
  • astro-ph.GA2
same name
  • Kun Xu — 52 papers, h 54
  • Kun Xu — 20 papers, h 28
  • Kun Xu — 18 papers
  • Kun Xu — 16 papers, h 56
  • Kun Xu — 10 papers
  • Kun Xu — 7 papers, h 35

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

collaborators

4 papers

astro-ph.CO2025

Abundance and phase-space distribution of subhalos in cosmological N-body simulations: testing numerical convergence and correction methods

Kun Xu

Subhalos play a crucial role in accurately modeling galaxy formation and galaxy-based cosmological probes within the highly nonlinear, virialized regime. However, numerical converg…

astro-ph.GA2025

Describing the Nonuniversal Galaxy Merger Timescales in IllustrisTNG: Effects of Host Halo Mass, Baryons, and Sample Selection

Kun Xu, Y. P. Jing

Galaxy merger timescales are crucial for understanding and modeling galaxy formation in our hierarchically structured Universe. However, previous studies have reported widely varyi…

astro-ph.CO2025

Photometric Objects Around Cosmic Webs (PAC) Delineated in a Spectroscopic Survey. VIII. Revisiting the Lensing is Low Effect

Xiaolin Luo, Kun Xu, Yipeng Jing +6

The issue of over-predicting the galaxy-galaxy lensing (GGL) signal using conventional galaxy-halo connection models has become well-known as the ``Lensing is Low'' problem, which…

astro-ph.GA2025

Photometric Objects Around Cosmic Webs (PAC). VII. Disentangling Mass and Environment Quenching with the Aid of Galaxy-halo Connection in Simulations

Yun Zheng, Kun Xu, Donghai Zhao +4

Star formation quenching in galaxies is a critical process in galaxy formation. It is widely believed that the quenching process is dominated by the mass of galaxies and/or their e…

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