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Xiaoyu Wang

4 papers hereh-index 322 citations7 works total

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

author position
  • first author2
  • 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
  • Xiaoyu Wang — 63 papers, h 15
  • Xiaoyu Wang — 14 papers, h 20
  • Xiaoyu Wang — 12 papers, h 12
  • Xiaoyu Wang — 12 papers, h 8
  • Xiaoyu Wang — 11 papers, h 3
  • Xiaoyu Wang — 9 papers, h 15

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
20172022
most citedHosts and triggers of AGNs in the Local Universe

23 citations · 38 across the 4 of their papers we have counts for

collaborators

4 papers

astro-ph.GA2022★ 5 cited

Anisotropy and characteristic scales in halo density gradient profiles

X. Wang, H. Wang, H. J. Mo

We use a large N-body simulation to study the characteristic scales in the density gradient profiles in and around halos with masses ranging from 1012 to $10^{15} h^{-1}{\rm M…

astro-ph.CO2021★ 5 cited

Evaluating the origins of the secondary bias based on the correlation of halo properties with the linear density field

Xiaoyu Wang, Huiyuan Wang, H. J. Mo +2

Using two sets of large N-body simulations, we study the origin of the correlations of halo assembly time (zf​), concentration (vmax​/v200​) and spin (λ)…

astro-ph.GA2020★ 23 cited

Hosts and triggers of AGNs in the Local Universe

Ziwen Zhang, Huiyuan Wang, Wentao Luo +11

Based on the spectroscopic and shear catalogs for SDSS galaxies in the local Universe, we compare optically-selected active galactic nuclei (AGNs) with control star-forming and qui…

astro-ph.CO2017★ 5 cited

Bimodal Formation Time Distribution for Infall Dark Matter Halos

Jingjing Shi, Huiyuan Wang, H. J. Mo +4

We use a 200 h−1Mpc a side N-body simulation to study the mass accretion history (MAH) of dark matter halos to be accreted by larger halos, which we call infall halos. We defi…

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