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Lei Liu

4 papers hereh-index 5268 citations5 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.GA3
  • astro-ph1
same name
  • Lei Liu — 17 papers, h 14
  • Lei Liu — 16 papers, h 12
  • Lei Liu — 14 papers, h 11
  • Lei Liu — 13 papers, h 16
  • Lei Liu — 12 papers, h 25
  • Lei Liu — 11 papers, h 11

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
20082020
most citedA catalog of newly identified star clusters in GAIA DR2

233 citations · 347 across the 4 of their papers we have counts for

collaborators

4 papers

astro-ph.GA2020★ 7 cited

Emergent gravity fails to explain color-dependent galaxy-galaxy lensing signals from SDSS Dr7

Wentao Luo, Jiajun Zhang, Vitali Halenka +6

We test the Emergent Gravity(EG) theory using the galaxy-galaxy lensing technique based on SDSS DR7 data. In the EG scenario, we do not expect color dependence of the galaxy sample…

astro-ph.GA2019★ 233 cited

A catalog of newly identified star clusters in GAIA DR2

Lei Liu, Xiaoying Pang

We present the Star cluster Hunting Pipeline (SHiP) which can identify star clusters in GAIA DR2 data, and establish a star cluster catalog for the Galactic disk. A Friend of Frien…

astro-ph.GA2009★ 50 cited

The Stellar Mass Components of Galaxies: Comparing Semi-Analytical Models with Observation

Lei Liu, Xiaohu Yang, H. J. Mo +2

We compare the stellar masses of central and satellite galaxies predicted by three independent semianalytical models with observational results obtained from a large galaxy group c…

astro-ph2008★ 57 cited

An ideal mass assignment scheme for measuring the Power Spectrum with FFTs

Weiguang Cui, Lei Liu, Xiaohu Yang +3

In measuring the power spectrum of the distribution of large numbers of dark matter particles in simulations, or galaxies in observations, one has to use Fast Fourier Transforms (F…

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