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.【doi.org/10.1016/j.xinn.2024.100695】
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】
LHAASO-KM2A detector simulation using Geant4
Radiation Detection Technology and Methods (2024) 8:1437–1447, 11 May, 2024,【DOI：10.1007/s41605-024-00467-8】