Showing 1–20 of 182 results
/ Date/ Name
Jun 29, 2022Euclid preparation: XXIII. Derivation of galaxy physical properties with deep machine learning using mock fluxes and H-band imagesSep 26, 2022Euclid preparation: XXII. Selection of Quiescent Galaxies from Mock Photometry using Machine LearningSep 26, 2022Euclid preparation. XXV. The Euclid Morphology Challenge -- Towards model-fitting photometry for billions of galaxiesAug 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 3, 2022Euclid preparation: XX. The Complete Calibration of the Color-Redshift Relation survey: LBT observations and data releaseOct 21, 2019Euclid preparation: VII. Forecast validation for Euclid cosmological probesJan 6, 2021Euclid preparation: XI. Mean redshift determination from galaxy redshift probabilities for cosmic shear tomographyOct 11, 2021Euclid preparation: XIX. Impact of magnification on photometric galaxy clusteringOct 23, 2023Euclid preparation. XXXI. The effect of the variations in photometric passbands on photometric-redshift accuracyJan 29, 2015Euclid Space Mission: building the sky surveyMar 19, 2025Euclid Quick Data Release (Q1). First Euclid statistical study of galaxy mergers and their connection to active galactic nucleiMar 19, 2025Euclid Quick Data Release (Q1): VIS processing and data productsNov 6, 2023Euclid Preparation. TBD. Impact of magnification on spectroscopic galaxy clusteringMay 9, 2024Euclid preparation. Sensitivity to neutrino parametersMar 19, 2025Euclid Quick Data Release (Q1). Photometric redshifts and physical properties of galaxies through the PHZ processing functionJan 14, 2025Euclid preparation LX. The use of HST images as input for weak-lensing image simulationsNov 29, 2024Euclid preparation: TBD. The impact of line-of-sight projections on the covariance between galaxy cluster multi-wavelength observable properties -- insights from hydrodynamic simulationsSep 11, 2024Euclid preparation. LXVII. Deep learning true galaxy morphologies for weak lensing shear bias calibrationSep 4, 2024Euclid preparation: Determining the weak lensing mass accuracy and precision for galaxy clusters