Showing 21–40 of 257 results
/ Date/ Name
Mar 19, 2025Euclid Quick Data Release (Q1) First study of red quasars selectionSep 14, 2016Gaia Data Release 1: Astrometry - one billion positions, two million proper motions and parallaxesFeb 10, 2025Euclid: A complete Einstein ring in NGC 6505Aug 12, 2024Euclid: The Early Release Observations Lens Search ExperimentMar 27, 2023Euclid preparation. XXVII. A UV-NIR spectral atlas of compact planetary nebulae for wavelength calibrationMar 19, 2025Euclid Quick Data Release (Q1). Exploring galaxy morphology across cosmic time through Sersic fitsFeb 13, 2025Euclid: Finding strong gravitational lenses in the Early Release Observations using convolutional neural networksMay 22, 2024Euclid: Early Release Observations -- A preview of the Euclid era through a galaxy cluster magnifying lensOct 21, 2021Euclid: Forecast constraints on consistency tests of the $Λ$CDM modelSep 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 InstrumentMar 19, 2025Euclid Quick Data Release (Q1). Optical and near-infrared identification and classification of point-like X-ray selected sourcesOct 31, 2025Euclid: Systematic uncertainties from the halo mass conversion on galaxy cluster number count data analysesMar 20, 2025Euclid: Early Release Observations -- Interplay between dwarf galaxies and their globular clusters in the Perseus galaxy clusterJan 8, 2026Euclid preparation. Galaxy 2-point correlation function modelling in redshift spaceDec 5, 2025Euclid Quick Data Release (Q1). From simulations to sky: Advancing machine-learning lens detection with real Euclid dataNov 4, 2025Euclid Quick Data Release (Q1). Searching for giant gravitational arcs in galaxy clusters with mask region-based convolutional neural networks