Showing 1–20 of 69 results
/ Date/ Name
Apr 24, 2026Introducing Background Temperature to Characterise Hidden Randomness in Large Language ModelsApr 22, 2026Level crossings and superradiant quantum phase transition for a two-qutrit quantum Rabi modelApr 14, 2026Nemotron 3 Super: Open, Efficient Mixture-of-Experts Hybrid Mamba-Transformer Model for Agentic ReasoningMar 23, 2026The CYGNO experiment: a gaseous TPC with optical readout for rare events searchesMar 16, 2026Upgrade of the Trigger and Data Acquisition System for Continuous Imaging and Multi-Camera Operation in CYGNOMar 6, 2026First Optical Observation of Negative Ion Drift at Surface PressureJan 28, 2026Trigger Optimization and Event Classification for Dark Matter Searches in the CYGNO Experiment Using Machine LearningJan 4, 2026Simulation of the CYGNO Gaseous TPC Optical ReadoutDec 30, 2025Fast reconstruction-based ROI triggering via anomaly detection in the CYGNO optical TPCDec 22, 2025Ultra-high precision high voltage system for PTOLEMYDec 1, 2025Characterization of cutting-edge CMOS Active Pixel sensors within the CYGNO ExperimentNov 17, 2025Sensitivity to low-mass WIMPs with an improved liquid argon ionization response model within the DarkSide programmeOct 27, 2025Validation of field cage and cathode for low radioactivity operation with the CYGNO experimentMay 9, 2025Modeling the light response of an optically readout GEM based TPC for the CYGNO experimentDec 25, 2024Quality Assurance and Quality Control of the $26~\text{m}^2$ SiPM production for the DarkSide-20k dark matter experimentOct 23, 2024Neutrinoless Double Beta Decay Sensitivity of the XLZD Rare Event ObservatoryOct 22, 2024The XLZD Design Book: Towards the Next-Generation Liquid Xenon Observatory for Dark Matter and Neutrino PhysicsSep 1, 2024The GAPS Programme at TNG. LXI. Atmospheric parameters and elemental abundances of TESS young exoplanet host starsAug 10, 2024Mass determination of two Jupiter-sized planets orbiting slightly evolved stars: TOI-2420 b and TOI-2485 bJun 9, 2024Enhancing the light yield of He:CF$_4$ based gaseous detector