Evidence for particle acceleration approaching PeV energies in the W51 complex

Science Bulletin, 30 September 2024.【doi.org/10.1016/j.scib.2024.07.017】

Monitoring the daily variation of Sun-Earth magnetic fields using galactic cosmic rays

The Innovation 5(6), 100695.

Data quality control system and long-term performance monitor of LHAASO-KM2A

Astroparticle Physics, January 2025【Doi：/10.1016/j.astropartphys.2024.103029】

Stringent Tests of Lorentz Invariance Violation from LHAASO Observations of GRB 221009A 

Phys. Rev. Lett. 2024.133, 071501【DOI:/10.1103/PhysRevLett.133.071501】

Discovery of Very High Energy Gamma-Ray Emissions from the Low-luminosity AGN NGC 4278 by LHAASO

The Astrophysical Journal Letters, Volume 971, Number 2【DOI 10.3847/2041-8213/ad5e6d】

Constraints on Ultraheavy Dark Matter Properties from Dwarf Spheroidal Galaxies with LHAASO Observations

  Phys. Rev. Lett. 2024,133, 061001 【DOI:/10.1103/PhysRevLett.133.061001】

 The First LHAASO Catalog of Gamma-Ray Sources

 The Astrophysical Journal Supplement Series, 2024,271,25【DOI:10.3847/1538-4365/acfd29】【arXiv:2305.17030】

  An ultrahigh-energy gamma-ray bubble powered by a super PeVatron

     Science Bulletin,26 February 2024,69(4): 449-457, 【DOI:10.1016/j.scib.2023.12.040】【arXiv:2310.10100】

  Does or Did the Supernova Remnant Cassiopeia A Operate as a PeVatron?

     The Astrophysical Journal Letters,961(2)【DOI:10.3847/2041-8213/ad1d62】【arXiv.2310.17082】

  Optimization of performance of the KM2A full array using the Crab Nebula

     Chinese Physics C, 29 February 2024,【DOI:10.1088/1674-1137/ad2e82】

  Measurements of all-particle energy spectrum and mean logarithmic mass of cosmic rays from 0.3 to 30PeV with LHAASO-KM2A

     Phys. Rev. Lett.,2024,132, 131002【Doi/10.1103/PhysRevLett.132.131002】【arXiv.2403.10010】