JF
J. H. Fan
astro-ph.HEastro-ph.GAhep-exastro-ph.IMgr-qchep-phhep-thphysics.ins-det
On Valency
published · living versionsW_p3bttx2a·v1 · currentpublished
Very high energy gamma-ray emission beyond 10 TeV from GRB 221009A
with Zhen Cao, F. Aharonian, Q. An, A. Axikegu +275
1 version
Preprints & journals
10 papers in the corpus · 2019–2025Broadband -ray spectrum of supernova remnant Cassiopeia A2502.04848v1 · Zhen Cao, F. Aharonian, Y.X. Bai et al.2025 · 10 citationsarXiv
An Enigmatic PeVatron in an Area around HII Region G35.6$-$0.52412.00379v2 · Zhen Cao, F. Aharonian, Axikegu et al.2024 · 0 citationsarXiv
Detection of very high-energy gamma-ray emission from the radio galaxy M87 with LHAASO2410.15353v3 · Zhen Cao, F. Aharonian, Axikegu et al.2024 · 12 citationsarXiv
Stringent Tests of Lorentz Invariance Violation from LHAASO Observations of GRB 221009A.39213544 · Cao, Zhen, Aharonian, F, Axikegu et al.2024 · 42 citationsPhysical review letters. 2024;133(7):071501
Evidence for particle acceleration approaching PeV energies in the W51 complex2407.00624v3 · Zhen Cao, F. Aharonian, Axikegu et al.2024 · 9 citationsScience Bulletin,2024
Data quality control system and long-term performance monitor of the LHAASO-KM2A2405.11826v3 · Zhen Cao, F. Aharonian, Axikegu et al.2024 · 0 citationsarXiv
Systematic Search and Study of Short-Timescale Flare Structures in BL Lac object Gamma-ray Emission2405.07028v1 · Jinjie Yu, Nan Ding, Junhui Fan et al.2024 · 0 citationsarXiv
Does or did the supernova remnant Cassiopeia A operate as a PeVatron?2310.17082v1 · Zhen Cao, F. Aharonian, Q. An et al.2023 · 10 citationsarXiv
The radio dichotomy of active galactic nuclei2202.07199v1 · Hubing Xiao, Jingtian Zhu, Liping Fu et al.2022 · 17 citationsarXiv
Correlation Analysis for Gamma-ray (radio) and Broad Line Emissions of Fermi Blazars1903.05849v1 · Lixia Zhang, Junhui Fan, Yuhai Yuan2019 · 1 citationarXiv
Career total: 27 works. 10 are in this corpus.
Profile built from the corpus for this byline.
Author records are still filling in while the Hub is in alpha. If this is your page, you'll be able to claim it soon. Spot a mistake? Tell us.