-
[1]
F. Krennrich, C. W. Akerlof, J. H. Buckley et al., Astropart. Phys. 8(4), 213 (1998)
-
[2]
M. Amenomori, Z. Cao, L. K. Ding et al., Phys. Rev. Lett. 69(17), 2468 (1992)
-
[3]
C. Bacci, K. Z. Bao, F. Barone et al., Astropart. Phys. 17(2), 151 (2002)
-
[4]
F. Aharonian, A. G. Akhperjanian, A. R. Bazer-Bachi et al., Astron. Astrophys. 457(3), 899 (2006)
-
[5]
E. Aliu, T. Arlen, T. Aune, et al., Science 334(6052), 69 (2011)
-
[6]
J. Aleksić, E. A. Alvarez, L. A. Antonelli et al., Astropart. Phys. 35(7), 435 (2012)
-
[7]
Z. Cao, D. della Volpe, S. M. Liu et al. The large high altitude air shower observatory (lhaaso) science book(2021 Ed.)., arXiv: 1905.02773
-
[8]
Z. Cao, F. A. Aharonian, Q. An et al., Nature 594(7861), 33 (2021)
-
[9]
Z. Cao, F. Aharonian, Q. An et al., Astrophys. J. Suppl. S. 271(1), 25 (2024)
-
[10]
Z. Cao, S. Z. Chen, R. Y. Liu et al., Annu. Rev. Nucl. Part. Sci. 73, 341 (2023)
-
[11]
B. S. Acharya, M. Actis, T. Aghajani et al., Astropart. phys. 43, 3 (2013)
-
[12]
S. Vercellone, C. Bigongiari, A. Burtovoi et al., J. High Energy Astrophys. 35, 1 (2022)
-
[13]
S. S. Zhang. Large Array of imaging atmospheric Cherenkov Telescopes (LACT): status and future plans. In Proceedings of 38th International Cosmic Ray Conference — PoS(ICRC2023), volume 444, page 808, 2024.
-
[14]
A. V. Plyasheshnikov, F. A. Aharonian, and H. J. Völk, J. Phys. G: Nucl. Part. 26(2), 183 (2000)
-
[15]
G. P. Rowell, V. Stamatescu, R. W. Clay et al., Nucl. Instrum. Meth. A 588(1-2), 48 (2008)
-
[16]
A. Nada, A. Ramos, Eur. Phys. J. C 81, 1 (2021)
-
[17]
S. C. Hu, G. M. Xiang, M. Zha et al., PoS ICRC2023(2), 655 (2023)
-
[18]
D. Heck, J. Knapp, J. N. Capdevielle et al. Corsika: A monte carlo code to simulate extensive air showers. 1998.
-
[19]
K. Bernlöhr, Astropart. Phys. 30(3), 149 (2008)
-
[20]
K. Bernlöhr, A. Barnacka, Y. Becherini et al., Astropart. Phys. 43, 171 (2013)
-
[21]
A. Michael Hillas. Cerenkov light images of eas produced by primary gamma. In 19th Intern. Cosmic Ray Conf-Vol. 3, number OG-9.5-3, 1985.
-
[22]
F. Pedregosa, G. Varoquaux, A. Gramfor et al., J. Mach. Learn. Res. 12, 2825 (2011)
-
[23]
P. Sommers and J. W. Elbert, J. Phys. G: Nucl. Phys. 13(4), 553 (1987)
-
[24]
A. Konopelko, F. Aharonian, M. Hemberger et al., J. Phys. G: Nucl. Phys. 25(9), 1989 (1999)
-
[25]
V. A. Acciari, S. Ansoldi, L. A. Antonelli et al., Astron. Astrophys. 635, A158 (2020)
-
[26]
C. B. Adams, W. Benbow, A. Brill et al., Astrophys. J. 913(2), 115 (2021)
-
[27]
C. C. Lu. Improving the hess angular resolution using the disp method, arXiv: 1310.1200
-
[28]
Z. P. Zhang et al., J. High Energy Astrophys. 43, 280 (2024)
-
[29]
E. Giro, R. Canestrari, G. Siron et al., Astron. Astrophys. 608, A86 (2017)
-
[30]
T. P. Li and Y. Q. Ma, Astrophys. J. 272, 317 (1983)
-
[31]
J. Zhao, J. Liu, X. D. Sheng et al., Chin. Phys. C 38(3), 036002 (2014)
-
[32]
H. Wang, C. Li, G. Xiao et al., Nucl. Instrum. Meth. A 956, 163416 (2020)
-
[33]
M. Peresano, et al (MAGIC Collaboration), Nuovo Cimento C Geophysics Space Physics C 41(3), 107 (2018)
-
[34]
Q. N. Sun, F. R. Zhu, Y. Zhang et al., Nucl. Instrum. Meth. A 1057, 168759 (2023)
-
[35]
LHAASO Collaboration, Sci. Adv. 9(46), eadj2778 (2023)
-
[36]
F. Aharonian, A. Akhperjanian, M. Beilicke et al., Astrophys. J. 614(2), 897 (2004)
-
[37]
H. J. Völk and Konrad Bernlöhr, Exp. Astron. 25, 173 (2009)
-
[38]
S. Lee, S. Einecke, G. Rowell et al., Publications of the Astronomical Society of Australia 39, e041 (2022)