The Second LHAASO Collaboration Conference in 2026 & The Academic Symposium for the 10th Anniversary of the LHAASO collaboration

We present a study of the γ-ray emission in the Kes 78 region using LHAASO observations. Our analysis reveals extended emission from LHAASO J1850−0004u, substantially larger than the supernova remnant, and identifies an additional point-like source, J1852−0003. Einstein Probe observations provide only an X-ray upper limit at the position of J1852−0003. Combining the LHAASO results with...

We report the first detection of TeV $\gamma$-ray emission from the region of the evolved supernova remnant (SNR) Simeis 147 (S147; G180.0$-$1.7) and its associated pulsar PSR J0538+2817, using 1484 days of LHAASO-WCDA observations and 1944 days of LHAASO-KM2A observations. The emission exhibits a clear energy-dependent morphology: the WCDA data favor a compact source plus an extended Gaussian...

Following our previous work on optimizing the analysis of LHAASO-KM2A full-array data at large zenith angles, we present preliminary results from a search for gamma-ray sources in the inner Galaxy, focusing on the W28, W30, and Galactic Center regions. These regions host various gamma-ray emission components, primarily associated with pulsar wind nebulae and interactions between high-energy...