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researcher

Yong Zhang

4 papers here

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

author position
  • middle author2

Across the 2 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA2
  • astro-ph.HE1
  • cs.DS1
ORCID 0000-0003-2179-3698
same name
  • Yong Zhang — 71 papers, h 30
  • Yong Zhang — 65 papers, h 20
  • Yong Zhang — 37 papers, h 16
  • Yong Zhang — 33 papers, h 23
  • Yong Zhang — 32 papers, h 10
  • Yong Zhang — 28 papers, h 13

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
20152022
most citedThe Stellar "Snake" I: Whole Structure and Properties

12 citations · 26 across the 4 of their papers we have counts for

collaborators

4 papers

astro-ph.HE2022★ 11 cited

Flux Variations of Cosmic Ray Air Showers Detected by LHAASO-KM2A During a Thunderstorm on 10 June 2021

LHAASO Collaboration, F. Aharonian, Q. An +268

The Large High Altitude Air Shower Observatory (LHAASO) has three sub-arrays, KM2A, WCDA and WFCTA. The flux variations of cosmic ray air showers were studied by analyzing the KM2A…

astro-ph.GA2021★ 12 cited

The Stellar "Snake" I: Whole Structure and Properties

Fan Wang, Hai-Jun Tian, Dan Qiu +10

To complement our previous discovery of the young snake-like structure in the solar neighborhood and reveal the structure's full extent, we build two samples of stars within the Sn…

cs.DS2019★ 3 cited

A constant FPT approximation algorithm for hard-capacitated k-means

Yicheng Xu, Rolf H. Möhring, Dachuan Xu +2

Hard-capacitated k-means (HCKM) is one of the fundamental problems remaining open in combinatorial optimization and data mining areas. In this problem, one is required to partiti…

astro-ph.GA2015

The M-giant star candidates identified in the LAMOST data release 1

Jing Zhong, Sebastien Lepine, Jing Li +6

We perform a discrimination procedure with the spectral index diagram of TiO5 and CaH2+CaH3 to separate M giants from M dwarfs. Using the M giant spectra identified from the LAMOST…

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