Showing 1–20 of 238 results
/ Date/ Name
Apr 24, 2026Ultra-high-energy $γ$-ray imprints from PeV particles accelerated by supernova remnantsApr 20, 2026Advances in photocathode development for PICOSEC Micromegas precise-timing detectorsApr 12, 2026First Observation of \boldmath{$D^+ \to a_0(980)ρ$ and $D^+ \to a_0(980)^+ f_0(500)$} in \boldmath{$D^+ \to π^+π^+π^-η$ and $D^+ \to π^+π^0π^0η$} DecaysApr 6, 2026Timing performance of large prototype based on $\upmu$RWELL- PICOSEC detector technology with $10 \times 10\ \mathrm{cm}^{2}$ active areaMar 19, 2026GRB 241030A: a bright afterglow challenging forward shock emissionMar 19, 2026Spatial resolution improvement of PICOSEC Micromegas precise timing detectorsMar 9, 2026Multi-epoch afterglow rebrightenings in GRB 250129A: Evidence for successive shock interactionsFeb 28, 2026First Amplitude Analysis of $D^0\rightarrow K^-π^0e^+ν_e$ and Observation of $D^0\rightarrow K^*_2(1430)^-e^+ν_e$Feb 17, 2026The COHERENT Experiment: 2026 UpdateFeb 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 sourceDec 17, 2025Measurements of the Absolute Branching Fraction of the Semileptonic Decay $\mathbf{Ξ^{-}\rightarrow Λe^- \barν_{e}}$ and the Axial Charge of the $\mathbfΞ^{-}$Dec 13, 2025Amplitude Analysis and Branching Fraction Measurement of $D^+ \to π^+π^0π^0$Dec 5, 2025Design and Performance of a 96-channel Resistive PICOSEC Micromegas Detector for ENUBETDec 4, 2025Performance Optimization and Characterization of 7-pad Resistive PICOSEC Micromegas DetectorsNov 17, 2025Measurement of Exclusive $π^+$--argon Interactions Using ProtoDUNE-SPNov 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 22, 2025Joint neutrino oscillation analysis from the T2K and NOvA experimentsOct 14, 2025Energy calibration of LHAASO-KM2A using the cosmic ray Moon shadow