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Hongyu Gao

4 papers here

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

author position
  • first author3
  • middle author1

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

fields
  • astro-ph.GA2
  • astro-ph.CO1
  • cond-mat.soft1
ORCID 0000-0003-0695-0122
same name
  • Hongyu Gao — 3 papers
  • Hongyu Gao — 3 papers
  • Hongyu Gao — 2 papers
  • Hongyu Gao — 1 paper
  • Hongyu Gao — 1 paper

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 DESI One-Percent Survey: A concise model for galactic conformity of ELGs

2 citations · 2 across the 4 of their papers we have counts for

collaborators

4 papers

cond-mat.soft2023

On the shear-thinning of alkanes

Hongyu Gao, Martin H. Müser

The approximate power-law dependence of the apparent viscosity of liquids on shear rate is often argued to arise from a distribution of energy barriers. However, recent work on the…

astro-ph.CO2023

Extending the unified subhalo model to warm dark matter

Feihong He, Jiaxin Han, Hongyu Gao +1

Using a set of high-resolution N-body simulations, we extend the unified distribution model of cold dark matter (CDM) subhaloes to the warm dark matter(WDM) case. The same model fr…

astro-ph.GA2023★ 2 cited

The DESI One-Percent Survey: A concise model for galactic conformity of ELGs

Hongyu Gao, Y. P. Jing, Kun Xu +27

Galactic conformity is the phenomenon in which a galaxy of a certain physical property is correlated with its neighbors of the same property, implying a possible causal relationshi…

astro-ph.GA2023

The DESI One-Percent survey: constructing galaxy-halo connections for ELGs and LRGs using auto and cross correlations

Hongyu Gao, Y. P. Jing, Shanquan Gui +31

In the current Dark Energy Spectroscopic Instrument (DESI) survey, emission line galaxies (ELGs) and luminous red galaxies (LRGs) are essential for mapping the dark matter distribu…

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