Showing 1–20 of 26 results
/ Date/ Name
Apr 24, 2026Ultra-high-energy $γ$-ray imprints from PeV particles accelerated by supernova remnantsFeb 13, 2026LHAASO observation of Mrk 421 during 2021 March - 2024 March: a comprehensive VHE catalog of multi-timescale outbursts and its time average behaviorDec 18, 2025Cygnus X-3: A variable petaelectronvolt gamma-ray sourceNov 7, 2025Precise Measurement of the Cosmic Ray Helium Spectrum above 0.1 PeVOct 27, 2025First detection of ultra-high energy emission from gamma-ray binary LS I +61 303Oct 16, 2025Measurement of $C\!P$ asymmetry in $D^0 \to K^0_{\rm S} K^0_{\rm S}$ decays with Run 3 dataOct 14, 2025Energy calibration of LHAASO-KM2A using the cosmic ray Moon shadowApr 1, 2025Study of Ultra-High-Energy Gamma-Ray Source 1LHAASO J0056+6346u and Its Possible OriginsFeb 23, 2025Constraining the Cosmic-ray Energy Based on Observations of Nearby Galaxy Clusters by LHAASOOct 17, 2024Measurement of attenuation length of the muon content in extensive air showers from 0.3 to 30 PeV with LHAASOSep 14, 2024Deep view of Composite SNR CTA1 with LHAASO in $γ$-rays up to 300 TeVAug 19, 2024Observation of the $γ$-ray Emission from W43 with LHAASOJan 20, 2024Prompt and nonprompt $ψ(2S)$ production in $p$Pb collisions at $\sqrt{s_{NN}}=8.16$ TeVDec 14, 2023Amplitude analysis of the $B^{0}\to K^{*0}μ^+μ^-$ decayNov 17, 2023A model-independent measurement of the CKM angle $γ$ in partially reconstructed $B^{\pm} \to D^{*} h^{\pm}$ decays with $D \to K_{S}^{0} h^{+}h^{-}$ $(h=π, K)$Oct 19, 2023Observation of the Antimatter Hypernucleus $^4_{\barΛ}\overline{\hbox{H}}$Oct 6, 2023Measurement of the CKM angle $γ$ using the $B^{\pm}\rightarrow D^{*} h^{\pm}$ channelsSep 11, 2023Measurement of the CKM angle $γ$ in the $B^0 \to DK^{*0}$ channel using self-conjugate $D \to K_S^0 h^+ h^-$ decaysJul 23, 2023Characterizing non-Markovian Quantum Process by Fast Bayesian TomographyMar 12, 2023Measurement of electrons from open heavy-flavor hadron decays in Au+Au collisions at $\sqrt{s_{\rm NN}}=200$ GeV with the STAR detector