• [1]

    J. Ballet, P. Bruel, T. H. Burnett, et al. Fermi Large Area Telescope Fourth Source Catalog Data Release 4 (4FGL-DR4). arXiv e-prints, July 2023.

  • [2]

    A. Albert, R. Alfaro, C. Alvarez, et al., ApJ 905(1), 76 (2020)

  • [3]

    H. Abdalla, A. Abramowski, F. Aharonian, et al., Astronomy & Astrophysics 612, A2 (2018)

  • [4]

    H. Abdalla, A. Abramowski, F. Aharonian, et al., Astronomy & Astrophysics 612, A1 (2018)

  • [5]

    Zhen Cao, F. Aharonian, Q. An, et al., ApJS 271(1), 25 (2024)

  • [6]

    Zhen Cao, F. Aharonian, Axikegu, et al., Science China Physics, Mechanics, and Astronomy 68(7), 279504 (2025)

  • [7]

    Zhen Cao, F. Aharonian, Axikegu, et al., Science China Physics, Mechanics, and Astronomy 68(7), 279503 (2025)

  • [8]

    Zhen Cao, F. Aharonian, Y. X. Bai, et al. Ultra-high-energy γ-ray emission associated with the tail of a bow-shock pulsar wind nebula. arXiv e-prints, page arXiv: 2502.15447, February 2025.

  • [9]

    Zhen Cao, F. Aharonian, Y. X. Bai, et al. An extreme particle accelerator powered by pulsar PSR J1849-0001. Nature Astronomy, April 2026.

  • [10]

    F Aharonian, AG Akhperjanian, AR Bazer-Bachi, et al., Astronomy & Astrophysics 448(2), L43 (2006)

  • [11]

    P de Wilt, N Maxted, and G Rowell. Probing the extent of the non-thermal emission from the vela x region at tev energies with hess. 2012.

  • [12]

    F. Aharonian, A. G. Akhperjanian, A. R. Bazer-Bachi, et al. Energy dependent \gamma-ray morphology in the pulsar wind nebula HESS J1825-137. Astronomy & Astrophysics, 460(2): 365–374, December 2006.

  • [13]

    H. Abdalla, F. Aharonian, F. Ait Benkhali, et al., Astronomy & Astrophysics 621, A116 (2019)

  • [14]

    A. Abramowski, F. Acero, F. Aharonian, et al. Identification of HESS J1303-631 as a pulsar wind nebula through \gamma-ray, X-ray, and radio observations. Astronomy & Astrophysics, 548: A46, December 2012.

  • [15]

    A. U. Abeysekara, A. Albert, R. Alfaro, et al., Science 358(6365), 911 (November 2017)

  • [16]

    F. Aharonian, Q. An, L. X. Axikegu, Bai, et al., PRL 126(24), 241103 (2021)

  • [17]

    Tobias Prinz and Werner Becker. A Search for X-ray Counterparts of Radio Pulsars. arXiv e-prints, page arXiv: 1511.07713, November 2015.

  • [18]

    A. A. Abdo, M. Ackermann, M. Ajello, et al., Science 325(5942), 840 (2009)

  • [19]

    S. Abdollahi, F. Acero, M. Ackermann, et al., ApJS 247(1), 33 (2020)

  • [20]

    Gregory T. Richards. A Search for Very High-Energy Gamma-Ray Emission from Pulsars with VERITAS. Ph.d. dissertation, Georgia Institute of Technology, December 2017.

  • [21]

    Alba Fernández Barral. Extreme particle acceleration in microquasar jets and pulsar wind nebulae with the MAGIC telescopes. Springer, 2018.

  • [22]

    M Amenomori, XJ Bi, D Chen, et al., The Astrophysical Journal Letters 709(1), L6 (2009)

  • [23]

    A. A. Abdo, A. U. Abeysekara, B. T. Allen, et al., Astroparticle Physics 57, 16 (2014)

  • [24]

    Zhen Cao, F. Aharonian, Q. An, et al., Science 373, 425 (2021)

  • [25]

    Huihai He and LHAASO collaboration. Design of the lhaaso detectors. Radiation Detection Technology and Methods, 2: 1–8, 2018.

  • [26]

    F. Aharonian, Q. An, Axikegu, et al., Chinese Physics C 45(2), 025002 (2021)

  • [27]

    F. Aharonian, Q. An, Axikegu, et al., Chinese Physics C 45(8), 085002 (2021)

  • [28]

    Zhen Cao, F Aharonian, Q An, et al. Lhaaso-km2a detector simulation using geant4. Radiation Detection Technology and Methods, pages 1–11, 2024.

  • [29]

    S. R. Kelner, F. A. Aharonian, and V. V. Bugayov. Energy spectra of gamma rays, electrons, and neutrinos produced at proton-proton interactions in the very high energy regime. PRD, 74(3): 034018, August 2006.

  • [30]

    D. A. Smith, S. Abdollahi, M. Ajello, et al., ApJ 958(2), 191 (2023)

  • [31]

    Sasha Brownsberger and Roger W Romani, The Astrophysical Journal 784(2), 154 (2014)

  • [32]

    Jianli Zhang, Hui Zhu, Guanhong Lin, et al. FAST Discovery of μJy Radio Pulsations from PSR J2238+5903, Providing a DM Distance Anchor for the Candidate TeV Halo 1LHAASO J2238+5900. 2026.

  • [33]

    Yang Su, Ji Yang, Shaobo Zhang, et al., The Astrophysical Journal Supplement Series 240(1), 9 (2019)

  • [34]

    Marc-Antoine Miville-Deschênes, Norman Murray, and Eve J. Lee, ApJ 834(1), 57 (2017)

  • [35]

    V. Zabalza. Naima: a Python package for inference of particle distribution properties from nonthermal spectra. In 34th International Cosmic Ray Conference (ICRC2015), volume 34 of International Cosmic Ray Conference, page 922, July 2015.

  • [36]

    D. Khangulyan, F. A. Aharonian, and S. R. Kelner, ApJ 783(2), 100 (2014)

  • [37]

    F. A. Aharonian, S. R. Kelner, and A. Yu. Prosekin, PRD 82(4), 043002 (2010)

  • [38]

    Giovanni Natale, Cristina C. Popescu, Mark Rushton, et al., MNRAS 509(2), 2339 (January 2022)

  • [39]

    F. Mattana, M. Falanga, D. Götz, et al., ApJ 694(1), 12 (March 2009)

  • [40]

    Ruo-Yu Liu, Huirong Yan, and Heshou Zhang, PRL 123(22), 221103 (2019)

  • [41]

    Qi-Zuo Wu, Chao-Ming Li, Xuan-Han Liang, Chong Ge, and Ruo-Yu Liu, ApJ 969(1), 9 (2024)

  • [42]

    Kun Fang, Frontiers in Astronomy and Space Sciences 9, 1022100 (2022)

  • [43]

    Roger A. Chevalier and Stephen P. Reynolds, ApJL 740(1), L26 (2011)

  • [44]

    Yiwei Bao, Siming Liu, and Yang Chen, ApJ 877(1), 54 (2019)

  • [45]

    Yiwei Bao and Yang Chen, ApJ 881(2), 148 (2019)

  • [46]

    Jiaxu Sun, Yang Chen, Yiwei Bao, Xiao Zhang, and Xin Zhou, ApJ 9801, 98 (2025)

  • [47]

    Tim Linden, Katie Auchettl, Joseph Bramante, et al., PRD 96(10), 103016 (2017)

  • [48]

    A. Albert, R. Alfaro, J. C. Arteaga-Velázquez, et al., ApJL 944(2), L29 (2023)

  • [49]

    Dong Zheng and Zhongxiang Wang, ApJ 968(2), 117 (2024)