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researcher

S. Shao

22 papers hereh-index 10388 citations25 works total

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

author position
  • first author8
  • middle author10
  • last author3

Across the 21 of 22 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA18
  • astro-ph.CO2
  • astro-ph.HE2
same name
  • S. Shao — 37 papers, h 17
  • S. Shao — 2 papers, h 10
  • S. Shao — 1 paper, h 8
  • S. Shao — 1 paper, h 33
  • S. Shao — 1 paper, h 2
  • S. Shao — 1 paper, h 3

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
20122026
most citedThe phase space density of fermionic dark matter haloes

94 citations · 573 across the 22 of their papers we have counts for

collaborators
Showing 2020Show all

4 papers · 1 filter

astro-ph.GA2020★ 20 cited

The survival of globular clusters in a cuspy Fornax

Shi Shao, Marius Cautun, Carlos S. Frenk +5

It has long been argued that the radial distribution of globular clusters (GCs) in the Fornax dwarf galaxy requires its dark matter halo to have a core of size ∼1 kpc. We rev…

astro-ph.HE2020★ 8 cited

Measuring the Mass of Missing Baryons in the Halo of Andromeda Galaxy with Gamma-Ray Observations

Yi Zhang, Ruo-Yu Liu, Hui Li +4

One of the biggest mysteries in the modern cosmology and galaxy formation is the hideout of the "missing baryons". The leading theory of galaxy formation predicts that a huge amoun…

astro-ph.GA2020★ 21 cited

Galaxy properties in the cosmic web of EAGLE simulation

Wenxiao Xu, Qi Guo, Haonan Zheng +8

We investigate the dependence of the galaxy properties on cosmic web environments using the most up-to-date hydrodynamic simulation: Evolution and Assembly of Galaxies and their En…

astro-ph.GA2020★ 30 cited

The twisted dark matter halo of the Milky Way

Shi Shao, Marius Cautun, Alis J. Deason +1

We analyse systems analogous to the Milky Way (MW) in the EAGLE cosmological hydrodynamics simulation in order to deduce the likely structure of the MW's dark matter halo. We ident…

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