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X. Ye

3 papers here

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

author position
  • first author1
  • middle author1

Across the 2 of 3 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE3
same name
  • X. Ye — 17 papers, h 34
  • X. Ye — 16 papers, h 39
  • X. Ye — 13 papers, h 25
  • X. Ye — 10 papers
  • X. Ye — 6 papers, h 51
  • X. Ye — 5 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

most citedUltra-high-energy γ-ray emission associated with the tail of a bow-shock pulsar wind nebula

3 citations · 3 across the 3 of their papers we have counts for

collaborators

3 papers

astro-ph.HE2025★ 3 cited

Ultra-high-energy γ-ray emission associated with the tail of a bow-shock pulsar wind nebula

Zhen Cao, F. Aharonian, Y. X. Bai +292

In this study, we present a comprehensive analysis of an unidentified point-like ultra-high-energy (UHE) γ-ray source, designated as 1LHAASO J1740+0948u, situated in the vicinity…

astro-ph.HE2025

The Influence of Sun's and Moon's Shadows on Cosmic-Ray Anisotropy

Xuan'ang Ye, Yi Zhang, Jiayin He +1

Large-scale anisotropy, with amplitudes reaching approximately 0.1% at TeV energies, has been observed by multiple cosmic-ray experiments. The obstruction of cosmic rays by the Sun…

astro-ph.HE2025

Broadband γ-ray spectrum of supernova remnant Cassiopeia A

Zhen Cao, F. Aharonian, Y. X. Bai +311

The core-collapse supernova remnant (SNR) Cassiopeia A (Cas A) is one of the brightest galactic radio sources with an angular radius of ∼ 2.5 $\arcmin$. Although no extension…

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