F. Li

most citedUltra-high-energy

γ

-ray emission associated with the tail of a bow-shock pulsar wind nebula

3 citations · 3 across the 2 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

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 $\sim$ 2.5 $\arcmin$. Although no extension…

hep-ex2020

Measurement of the Born cross sections for $e^{+} e^{-} \to η^{'} π^{+} π^{-}$ at center-of-mass energies between $2.00$ and $3.08$ GeV

BESIII Collaboration, M. Ablikim, M. N. Achasov +487

The Born cross sections for the process $e^{+} e^{-} \to η^{'} π^{+} π^{-}$ at different center-of-mass energies between $2.00$ and $3.08$ GeV are reported with improved precision fro…

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

Broadband γ-ray spectrum of supernova remnant Cassiopeia A

Measurement of the Born cross sections for e+e−→η′π+π− at center-of-mass energies between 2.00 and 3.08 GeV

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

Broadband $γ$ -ray spectrum of supernova remnant Cassiopeia A

Measurement of the Born cross sections for $e^{+} e^{-} \to η^{'} π^{+} π^{-}$ at center-of-mass energies between $2.00$ and $3.08$ GeV