Showing 1–20 of 339 results
/ Date/ Name
Jun 29, 2022Euclid preparation: XXIII. Derivation of galaxy physical properties with deep machine learning using mock fluxes and H-band imagesMar 16, 2023Euclid: Validation of the MontePython forecasting toolsJul 20, 2022Euclid: Testing the Copernican principle with next-generation surveysSep 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 clustersSep 29, 2023Euclid: The search for primordial featuresApr 2, 2009Stellar and total baryon mass fractions in groups and clusters since redshift 1Jan 16, 2024Euclid: Improving the efficiency of weak lensing shear bias calibration. Pixel noise cancellation and the response method on trialOct 28, 2009A Weak Lensing Study of X-ray Groups in the COSMOS survey: Form and Evolution of the Mass-Luminosity RelationJun 3, 2022Euclid preparation: XX. The Complete Calibration of the Color-Redshift Relation survey: LBT observations and data releaseMar 26, 2013Evolution of Galaxies and their Environments at z = 0.1 to 3 in COSMOSMar 14, 2019An Ultra Deep Field survey with WFIRSTOct 23, 2019Euclid preparation: VI. Verifying the Performance of Cosmic Shear ExperimentsAug 13, 2020Paving the Way to Future Missions: the Roman Space Telescope Coronagraph Technology DemonstrationOct 21, 2019Euclid preparation: VII. Forecast validation for Euclid cosmological probesDec 8, 2020Euclid: Forecasts for $k$-cut $3 \times 2$ Point StatisticsJan 6, 2021Euclid preparation: XI. Mean redshift determination from galaxy redshift probabilities for cosmic shear tomographyFeb 17, 2021Euclid: Effect of sample covariance on the number counts of galaxy clusters