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Ying Li

4 papers here

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

author position
  • first author2
  • last author2

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

fields
  • astro-ph.GA2
  • astro-ph.SR1
  • cs.LG1
ORCID 0009-0006-5561-7878
same name
  • Ying Li — 32 papers, h 21
  • Ying Li — 19 papers, h 26
  • Ying Li — 13 papers, h 17
  • Ying Li — 13 papers, h 18
  • Ying Li — 12 papers
  • Ying Li — 11 papers, h 15

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
20232025
collaborators

4 papers

astro-ph.SR2025

The Samples and Binary Fractions of Red Supergiant in M31 and M33 by the HST Observations

Min Dai, Shu Wang, Biwei Jiang +1

The binarity of red supergiants (RSGs) influences their evolution and the fate of supernovae. We investigate the binary fraction of RSGs in the Andromeda Galaxy (M31) and Triangulu…

astro-ph.GA2025

Metallicity Distribution in M31 and M33 Based on the Tip-RGB Near-infrared Color

Ying Li, Biwei Jiang, Yi Ren

This study investigates the metallicity distribution in M31 and M33 by using the near-infrared color index J−K of tip-red-giant-branch (TRGB) of the member stars from \cite{2021A…

astro-ph.GA2024

The Metallicity Distribution in the LMC and the SMC based on the Tip-RGB Colors

Ying Li, Biwei Jiang, Yi Ren

The color index (J−K)0​ of tip-red giant branch (TRGB) is used to study the metallicity distribution in the Large and Small Magellanic Cloud. With the most complete and pure samp…

cs.LG2023

PMNN:Physical Model-driven Neural Network for solving time-fractional differential equations

Zhiying Ma, Jie Hou, Wenhao Zhu +2

In this paper, an innovative Physical Model-driven Neural Network (PMNN) method is proposed to solve time-fractional differential equations. It establishes a temporal iteration sch…

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