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researcher

Li Zhang

36 papers hereh-index 222.2k citations129 works total

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

author position
  • middle author10
  • last author23

Across the 33 of 36 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE33
  • astro-ph2
  • astro-ph.CO1
same name
  • Li Zhang — 41 papers, h 10
  • Li Zhang — 37 papers, h 42
  • Li Zhang — 24 papers, h 13
  • Li Zhang — 22 papers, h 6
  • Li Zhang — 20 papers, h 20
  • Li Zhang — 19 papers, h 16

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
20062021
most citedThe Large High Altitude Air Shower Observatory (LHAASO) Science Book (2021 Edition)

95 citations · 846 across the 36 of their papers we have counts for

collaborators
Showing 2010Show all

4 papers · 1 filter

astro-ph.HE2010★ 28 cited

Lepto-Hadronic Origin of gamma-rays from the G54.1+0.3 Pulsar Wind Nebula

Hui Li, Yang Chen, Li Zhang

G54.1+0.3 is a Crab-like pulsar wind nebula (PWN) with the highest γ-ray to X-ray luminosity ratio among all the nebulae driven by young rotation-powered pulsars. We model the sp…

astro-ph.HE2010★ 16 cited

Multiband Nonthermal Radiative Properties of HESS J1813-178

Jun Fang, Li Zhang

The source HESS J1813-178 was detected in the survey of the inner Galaxy in TeV gamma-rays, and a SNR G12.8-0.0 was identified in the radio band to be associated with it. The PWN e…

astro-ph.HE2010★ 9 cited

The Correlated Multi-color Optical Variations of BL Lac Object S5 0716+714

Bingkai Zhang, Benzhong Dai, Li Zhang +2

S5 0716+714 is a well-studied BL Lac object in the sky. Verifying the existence of correlations among the flux variations in different bands serves as an important tool to investig…

astro-ph.HE2010★ 8 cited

On the Nonthermal Emission from the Supernova Remnant W51C

Jun Fang, Li Zhang

The middle-aged supernova remnant (SNR) W51C is an interesting source for the interaction of the shell with a molecular cloud. The shell emits intense radio synchrotron photons, an…

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