Showing 1–20 of 34 results
/ Date/ Name
Nov 11, 2025Euclid preparation: LXXXVII. Non-Gaussianity of 2-point statistics likelihood: Precise analysis of the matter power spectrum distributionOct 20, 2025Euclid preparation: The flat-sky approximation for the clustering of Euclid's photometric galaxiesOct 10, 2025Euclid preparation. Cosmology Likelihood for Observables in Euclid (CLOE). 3. Inference and ForecastsAug 27, 2025Euclid: A machine-learning search for dual and lensed AGN at sub-arcsec separationsJul 10, 2025Euclid: Early Release Observations. Weak gravitational lensing analysis of Abell 2390Jun 10, 2025Euclid preparation: The NISP spectroscopy channel, on ground performance and calibrationMay 7, 2025Euclid preparation. The impact of redshift interlopers on the two-point correlation function analysisMar 19, 2025Euclid Quick Data Release (Q1), A first look at the fraction of bars in massive galaxies at $z<1$Mar 19, 2025Euclid Quick Data Release (Q1): First visual morphology catalogueFeb 10, 2025Euclid: A complete Einstein ring in NGC 6505May 22, 2024Euclid: Early Release Observations -- Programme overview and pipeline for compact- and diffuse-emission photometryDec 1, 2023Euclid preparation. XLI. Galaxy power spectrum modelling in real spaceOct 24, 2023Euclid preparation. LII. Forecast impact of super-sample covariance on 3x2pt analysis with EuclidNov 9, 2022Updated constraints on sterile neutrino mixing in the OPERA experiment using a new $ν_e$ identification methodDec 23, 2019First observation of a tau neutrino charged current interaction with charm production in the Opera experimentApr 11, 2019Final results on neutrino oscillation parameters from the OPERA experiment in the CNGS beamOct 31, 2018Latest results of the OPERA experiment on nu-tau appearance in the CNGS neutrino beamOct 25, 2018Measurement of the cosmic ray muon flux seasonal variation with the OPERA detectorApr 13, 2018Final results of the OPERA experiment on $ν_τ$ appearance in the CNGS beamMar 30, 2018Final results of the search for $ν_μ \to ν_{e}$ oscillations with the OPERA detector in the CNGS beam