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researcher

Shuai Liu

4 papers here

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

author position
  • middle author3

Across the 3 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR2
  • astro-ph.HE1
  • astro-ph.IM1
ORCID 0000-0001-5193-1727
same name
  • Shuai Liu — 36 papers, h 52
  • Shuai Liu — 14 papers, h 7
  • Shuai Liu — 9 papers, h 19
  • Shuai Liu — 8 papers
  • Shuai Liu — 5 papers, h 8
  • Shuai Liu — 3 papers

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

most citedThe Mini-SiTian Array: first-two-year operation

12 citations · 20 across the 4 of their papers we have counts for

collaborators

4 papers

astro-ph.SR2025

Revisiting the Li abundances of Stars with and without Detected Planets from the High Resolution Spectroscopy

Jinxiao Qin, Hong-Liang Yan, Wenyuan Cui +12

Whether the presence of planets affects the lithium (Li) abundance of their host stars is still an open question. To investigate the difference of the Li abundance between planet-h…

astro-ph.HE2025

Pair-Instability Gap Black Holes in Population III Star Clusters: Pathways, Dynamics, and Gravitational Wave Implications

Weiwei Wu, Long Wang, Shuai Liu +3

The detection of the gravitational wave (GW) event GW190521 raises questions about the formation of black holes within the pair-instability mass gap (PIBHs). We propose that Popula…

astro-ph.IM2025★ 12 cited

The Mini-SiTian Array: first-two-year operation

Min He, Hong Wu, Liang Ge +70

The SiTian project, designed to utilize 60 telescopes distributed across multiple sites in China, is a next-generation time-domain survey initiative. As a pathfinder for the SiTian…

astro-ph.SR2024★ 8 cited

Discovery of an Extremely r-process-enhanced Thin-disk Star with [Eu/H] = +0.78

Xiao-Jin Xie, Jianrong Shi, Hong-Liang Yan +9

Highly r-process-enhanced stars are rare and usually metal-poor ([Fe/H] < - 1.0), and mainly populate the Milky Way halo and dwarf galaxies. This study presents the discovery of a…

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