Showing 1–20 of 49 results
/ Date/ Name
Jan 12, 2022Very large SiPM arrays with aggregated outputJul 22, 2011Observations of the December 13 and 14, 2006, Solar Particle Events in the 80 MeV/n - 3 GeV/n range from space with PAMELA detectorJul 13, 2014Observation of nu_tau appearance in the CNGS beam with the OPERA experimentJan 9, 2014Evidence for $ν_μ\to ν_τ$ appearance in the CNGS neutrino beam with the OPERA experimentMay 22, 2007Track reconstruction in the emulsion-lead target of the OPERA experiment using the ESS microscopeMar 11, 2025Flow and thermal modelling of the argon volume in the DarkSide-20k TPCJan 20, 2010A statistical procedure for the identification of positrons in the PAMELA experimentOct 31, 2018Latest results of the OPERA experiment on nu-tau appearance in the CNGS neutrino beamJan 21, 2021Separating $^{39}$Ar from $^{40}$Ar by cryogenic distillation with Aria for dark matter searchesApr 11, 2019Final results on neutrino oscillation parameters from the OPERA experiment in the CNGS beamApr 23, 2014Determination of the muon charge sign with the dipolar spectrometers of the OPERA experimentJul 13, 2015Intrinsic neutron background of nuclear emulsions for directional Dark Matter searchesJun 28, 2012Gamma Ray Bursts Scaling Relations to test cosmological modelsMar 6, 2015Limits on muon-neutrino to tau-neutrino oscillations induced by a sterile neutrino state obtained by OPERA at the CNGS beamAug 26, 2024Benchmarking the design of the cryogenics system for the underground argon in DarkSide-20kDec 23, 2019First observation of a tau neutrino charged current interaction with charm production in the Opera experimentJan 22, 2020Design and construction of a new detector to measure ultra-low radioactive-isotope contamination of argonMar 21, 2011PAMELA Measurements of Cosmic-ray Proton and Helium SpectraApr 16, 2014Procedure for short-lived particle detection in the OPERA experiment and its application to charm decaysOct 23, 2011The missing matter problem: from the dark matter search to alternative hypotheses