Showing 1–20 of 190 results
/ Date/ Name
Apr 23, 2026Attention-based multiple instance learning for predominant growth pattern prediction in lung adenocarcinoma wsi using foundation modelsApr 21, 2026Radon-induced backgrounds in the NEXT-100 experimentApr 17, 2026Electroluminescence Yield Measurements in Xenon Gas with the NEXT-DEMO++ DetectorMar 26, 2026Searches for Continuous Gravitational Waves from Supernova Remnants in the first part of the LIGO-Virgo-KAGRA Fourth Observing runMar 19, 2026GWTC-4.0: Tests of General Relativity. I. Overview and General TestsDec 22, 2025Nuclear Physics Mid Term Plan at LNGSNov 23, 2025Optimizing the potential of KM3NeT in detecting core-collapse supernovaeNov 20, 2025Deep Learning Framework for Enhanced Neutrino Reconstruction of Single-line Events in the ANTARES TelescopeNov 11, 2025Euclid preparation: LXXXVII. Non-Gaussianity of 2-point statistics likelihood: Precise analysis of the matter power spectrum distributionNov 10, 2025Search for steady and flaring neutrino emission from cosmic sources using the complete ANTARES datasetNov 4, 2025Demonstration of Sub-Percent Energy Resolution in the NEXT-100 DetectorNov 3, 2025First results of the NEXT-100 detector using $^{83m}$Kr decaysOct 22, 2025Joint neutrino oscillation analysis from the T2K and NOvA experimentsOct 20, 2025Euclid preparation: The flat-sky approximation for the clustering of Euclid's photometric galaxiesOct 16, 2025Measurement of $C\!P$ asymmetry in $D^0 \to K^0_{\rm S} K^0_{\rm S}$ decays with Run 3 dataOct 10, 2025Euclid preparation. Cosmology Likelihood for Observables in Euclid (CLOE). 3. Inference and ForecastsSep 17, 2025Coherent Control of Quantum-Dot Spins with Cyclic Optical TransitionsSep 10, 2025Time-Dependent Modeling of the Sub-Hour Spectral Evolution During the 2013 Outburst of Mrk 421Sep 9, 2025Measurement of muon neutrino induced charged current interactions without charged pions in the final state using a new T2K off-axis near detector WAGASCI-BabyMINDSep 4, 2025GWTC-4.0: Constraints on the Cosmic Expansion Rate and Modified Gravitational-wave Propagation