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researcher

Weiwei Xu

10 papers hereh-index 427 citations10 works total

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

author position
  • first author2
  • middle author8

Across the 10 of 10 papers where every author was matched, so the position is known.

fields
  • astro-ph.CO4
  • astro-ph.GA4
  • astro-ph.HE1
  • astro-ph.IM1
same name
  • Weiwei Xu — 20 papers
  • Weiwei Xu — 10 papers, h 2
  • Weiwei Xu — 9 papers, h 21
  • Weiwei Xu — 9 papers, h 8
  • Weiwei Xu — 8 papers, h 8
  • Weiwei Xu — 6 papers, h 8

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
20202026
most citedRam pressure stripping of HI-rich galaxies infalling into massive clusters

19 citations · 48 across the 10 of their papers we have counts for

collaborators
Showing astro-ph.COShow all

4 papers · 1 filter

astro-ph.CO2025

A Comparative Study of Halo Mass Estimates from Group Catalogs and Lensing Signals

Xinyue Chen, Weiwei Xu, Ran Li +3

We compare halo mass estimates from three galaxy group catalogs (redMaPPer, Yang21, and Zou21) with those derived from gravitational lensing measurements. Each catalog employs dist…

astro-ph.CO2024

The measurement of the splashback radius of dark matter halo

Weiwei Xu, Huanyuan Shan, Ran Li +4

In the hierarchical evolution framework of cosmology, larger halos grow through matter accretion and halo mergers. To clarify the halo evolution, we need to define the halo mass an…

astro-ph.CO2022★ 1 cited

Spectroscopic Confirmation of Two X-ray Diffuse and Massive Galaxy Clusters at Low Redshift

Kaiyuan Chen, Weiwei Xu, Linhua Jiang

We present MMT spectroscopic observations of two massive galaxy cluster candidates at redshift z∼0.07 that show extended and diffuse X-ray emission in the ROSAT All Sky Survey…

astro-ph.CO2021★ 10 cited

Halo Mass-Concentration Relation at High-Mass End

Weiwei Xu, Huanyuan Shan, Ran Li +6

The concentration-mass (c-M) relation encodes the key information of the assembly history of the dark matter halos, however its behavior at the high mass end has not been measured…

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