Showing 21–40 of 49 results
/ Date/ Name
Jan 17, 2007Electron/pion separation with an Emulsion Cloud Chamber by using a Neural NetworkMar 30, 2018Final results of the search for $ν_μ \to ν_{e}$ oscillations with the OPERA detector in the CNGS beamJul 6, 2010PAMELA results on the cosmic-ray antiproton flux from 60 MeV to 180 GeV in kinetic energyDec 25, 2024Quality Assurance and Quality Control of the $26~\text{m}^2$ SiPM production for the DarkSide-20k dark matter experimentMar 15, 2011The cosmic-ray electron flux measured by the PAMELA experiment between 1 and 625 GeVNov 9, 2022Updated constraints on sterile neutrino mixing in the OPERA experiment using a new $ν_e$ identification methodMar 2, 2014Measurement of TeV atmospheric muon charge ratio with the full OPERA dataApr 4, 2020SiPM-matrix readout of two-phase argon detectors using electroluminescence in the visible and near infrared rangeApr 14, 2016NEWS: Nuclear Emulsions for WIMP SearchApr 6, 2006Hardware performance of a scanning system for high speed analysis of nuclear emulsionsAug 12, 2013New results on $ν_μ\to ν_τ$ appearance with the OPERA experiment in the CNGS beamJun 29, 2021Direct comparison of PEN and TPB wavelength shifters in a liquid argon detectorApr 13, 2018Final results of the OPERA experiment on $ν_τ$ appearance in the CNGS beamApr 29, 2024A new hybrid gadolinium nanoparticles-loaded polymeric material for neutron detection in rare event searchesJul 9, 2025Production, Quality Assurance and Quality Control of the SiPM Tiles for the DarkSide-20k Time Projection ChamberJul 28, 2023Directionality of nuclear recoils in a liquid argon time projection chamberNov 16, 2020Sensitivity of future liquid argon dark matter search experiments to core-collapse supernova neutrinosSep 2, 2022Sensitivity projections for a dual-phase argon TPC optimized for light dark matter searches through the ionization channelJul 25, 2011The discovery of geomagnetically trapped cosmic ray antiprotonsMar 16, 2013Search for $ν_μ\rightarrow ν_e$ oscillations with the OPERA experiment in the CNGS beam