Showing 41–60 of 169 results
/ Date/ Name
Jan 27, 2025Euclid preparation. 3-dimensional galaxy clustering in configuration space. Part I. 2-point correlation function estimationSep 3, 2024Euclid preparation. L. Calibration of the linear halo bias in $Λ(ν)$CDM cosmologiesJul 29, 2024Euclid preparation. Exploring the properties of proto-clusters in the Simulated Euclid Wide SurveyMay 22, 2024Euclid preparation. LVIII. Detecting globular clusters in the Euclid surveyMay 22, 2024Euclid. III. The NISP InstrumentApr 18, 2024Euclid preparation. Improving cosmological constraints using a new multi-tracer method with the spectroscopic and photometric samplesMar 19, 2025Euclid preparation. Spatially resolved stellar populations of local galaxies with Euclid: a proof of concept using synthetic images with the TNG50 simulationJan 15, 2026Euclid: Galaxy SED reconstruction in the PHZ processing function: impact on the PSF and the role of medium-band filtersJan 12, 2026Euclid preparation. Testing analytic models of galaxy intrinsic alignments in the Euclid Flagship simulationNov 4, 2025Euclid Quick Data Release (Q1). Spectroscopic unveiling of highly ionised lines at z = 2.48-3.88Mar 19, 2025Euclid Quick Data Release (Q1) -- Characteristics and limitations of the spectroscopic measurementsNov 4, 2025Euclid Quick Data Release (Q1): Hunting for luminous z > 6 galaxies in the Euclid Deep Fields -- forecasts and first bright detectionsJul 21, 2025Euclid preparation: Expected constraints on initial conditionsApr 17, 2025Euclid preparation. Estimating galaxy physical properties using CatBoost chained regressors with attentionJun 10, 2025Euclid preparation: The NISP spectroscopy channel, on ground performance and calibrationApr 1, 2026Euclid preparation. Impact of redshift distribution uncertainties on the joint analysis of photometric galaxy clustering and weak gravitational lensingMar 30, 2026Euclid Quick Data Release (Q1). The Strong Lensing Discovery Engine F -- Bright and low-redshift strong lensesMar 13, 2026Euclid preparation. Simulated galaxy catalogues for non-standard cosmological modelsNov 11, 2025Euclid preparation: LXXXVII. Non-Gaussianity of 2-point statistics likelihood: Precise analysis of the matter power spectrum distributionMay 4, 2026Euclid preparation. CosmoPostProcess: A simulation calibrated framework for weak lensing selection bias in richness-selected galaxy clusters