Showing 1–20 of 102 results
/ Date/ Name
May 10, 2023On the degeneracies between baryons, massive neutrinos and f(R) gravity in Stage IV cosmic shear analysesNov 20, 2023Euclid preparation. Spectroscopy of active galactic nuclei with NISPFeb 15, 2024Euclid preparation. XLIII. Measuring detailed galaxy morphologies for Euclid with machine learningOct 24, 2023Euclid preparation. LII. Forecast impact of super-sample covariance on 3x2pt analysis with EuclidMar 19, 2025Euclid Quick Data Release (Q1). The first catalogue of strong-lensing galaxy clustersMar 19, 2025Euclid Quick Data Release (Q1). The Strong Lensing Discovery Engine D -- Double-source-plane lens candidatesMar 19, 2025Euclid Quick Data Release (Q1) First study of red quasars selectionSep 5, 2024Euclid preparation. Simulations and nonlinearities beyond $Λ$CDM. 1. Numerical methods and validationAug 9, 2024Euclid preparation. The Cosmic Dawn Survey (DAWN) of the Euclid Deep and Auxiliary FieldsJun 26, 2024Euclid preparation. Sensitivity to non-standard particle dark matter modelMay 28, 2024Euclid preparation. Observational expectations for redshift z<7 active galactic nuclei in the Euclid Wide and Deep surveysMay 22, 2024Euclid. II. The VIS InstrumentOct 10, 2025Euclid preparation. Cosmology Likelihood for Observables in Euclid (CLOE). 5. Extensions beyond the standard modelling of theoretical probes and systematic effectsJul 30, 2025Euclid: Forecasts on $Λ$CDM consistency tests with growth rate dataMar 30, 2026Euclid preparation. Galaxy power spectrum and bispectrum modellingAug 3, 2022Euclid preparation. XXIV. Calibration of the halo mass function in $Λ(ν)$CDM cosmologiesNov 23, 2022Euclid preparation. XXVII. Covariance model validation for the 2-point correlation function of galaxy clustersJun 7, 2021COSMOPOWER: emulating cosmological power spectra for accelerated Bayesian inference from next-generation surveysOct 23, 2023Euclid preparation. XXXI. The effect of the variations in photometric passbands on photometric-redshift accuracyMay 15, 2025Euclid: Photometric redshift calibration with the clustering redshifts technique