Showing 1–19 of 19 results
/ Date/ Name
Nov 11, 2025Euclid preparation: LXXXVII. Non-Gaussianity of 2-point statistics likelihood: Precise analysis of the matter power spectrum distributionOct 20, 2025Three decades of FCNC studies in 3-3-1 model with right-handed neutrinos: from $Z^\prime$-dominance to the alignment limitOct 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 catalogueMar 18, 2025Meson Mixing Bounds on $Z^{\prime}$ Mass in the Alignment Limit: Establishing the Phenomenological Viability of the 331 ModelFeb 10, 2025Euclid: A complete Einstein ring in NGC 6505Dec 19, 2024Leptoquark-induced radiative masses for active and sterile neutrinos within the framework of the 3-3-1 modelMay 22, 2024Euclid: Early Release Observations -- Programme overview and pipeline for compact- and diffuse-emission photometryMay 9, 2024Exploring solutions to the muon g-2 anomaly in a 3-3-1 model under flavor constraintsDec 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 EuclidJul 3, 2021Confronting the inverse seesaw mechanism with the recent muon g-2 resultMar 4, 2020Vacuum stability and spontaneous violation of the lepton number at low energy scale in a model for light sterile neutrinos