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Yi-Zhong Fan

5 papers hereh-index 257 citations6 works total

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

author position
  • middle author1
  • last author1

Across the 2 of 5 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE3
  • astro-ph2
same name
  • Yi-zhong Fan — 27 papers, h 11
  • Yi-Zhong Fan — 21 papers, h 13
  • Yi-Zhong Fan — 12 papers, h 5
  • Yi-Zhong Fan — 10 papers, h 2
  • Yi-Zhong Fan — 9 papers, h 3
  • Yi-Zhong Fan — 6 papers, 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
20032025
most citedStrong GeV Emission Accompanying TeV Blazar H1426+428

30 citations · 66 across the 5 of their papers we have counts for

collaborators

4 papers

astro-ph.HE2025★ 6 cited

Charge-dependent spectral softenings of primary cosmic-rays below the knee

DAMPE Collaboration, Francesca Alemanno, Qi An +146

In most particle acceleration or propagation theories, the characteristic features of the cosmic ray spectra due to acceleration limits or propagation phase changes are charge depe…

astro-ph.HE2025

Leptohadronic Multimessenger Modeling of Two High-redshift (z > 1) Neutrino Emission Blazar Candidates

Xiong Jiang, Neng-Hui Liao, Xue Rui +2

The blazars are one of the leading candidate sources of high-energy neutrinos. Recently, two blazars have been found to be temporally and spatially correlated with some IceCube hig…

astro-ph.HE2024

A nearby FR I type radio galaxy 3C 120 as a possible PeV neutrino emitter

Rong-Qing Chen, Neng-Hui Liao, Xiong Jiang +1

Although connections between flaring blazars and some IceCube neutrinos have been established, the dominant sources for the bulk extragalactic neutrino emissions are still unclear…

astro-ph2003★ 30 cited

Strong GeV Emission Accompanying TeV Blazar H1426+428

Y. Z. Fan, Z. G. Dai, D. M. Wei

For High frequency BL Lac objects (HBLs) like H1426+428, a significant fraction of their TeV gamma-rays emitted are likely to be absorbed in interactions with the diffuse IR backgr…

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