Showing 1–20 of 46 results
/ Date/ Name
Nov 11, 2025Euclid preparation: LXXXVII. Non-Gaussianity of 2-point statistics likelihood: Precise analysis of the matter power spectrum distributionOct 20, 2025Euclid preparation: The flat-sky approximation for the clustering of Euclid's photometric galaxiesOct 10, 2025Euclid preparation. Cosmology Likelihood for Observables in Euclid (CLOE). 3. Inference and ForecastsSep 8, 2025Active galactic nuclei-heated dust revealed in "little red dots"Aug 27, 2025Euclid: A machine-learning search for dual and lensed AGN at sub-arcsec separationsJul 10, 2025Euclid: Early Release Observations. Weak gravitational lensing analysis of Abell 2390Jun 10, 2025Euclid preparation: The NISP spectroscopy channel, on ground performance and calibrationMay 7, 2025Euclid preparation. The impact of redshift interlopers on the two-point correlation function analysisMar 19, 2025Euclid Quick Data Release (Q1), A first look at the fraction of bars in massive galaxies at $z<1$Mar 19, 2025Euclid Quick Data Release (Q1): First visual morphology catalogueFeb 10, 2025Euclid: A complete Einstein ring in NGC 6505May 22, 2024Euclid: Early Release Observations -- Programme overview and pipeline for compact- and diffuse-emission photometryDec 1, 2023Euclid preparation. XLI. Galaxy power spectrum modelling in real spaceOct 24, 2023Euclid preparation. LII. Forecast impact of super-sample covariance on 3x2pt analysis with EuclidJun 29, 2022Properties of the interstellar medium in star-forming galaxies at redshifts 2 < z < 5 from the VANDELS surveyFeb 8, 2022The VANDELS survey: a measurement of the average Lyman-continuum escape fraction of star-forming galaxies at z=3.5Sep 8, 2021No strong dependence of Lyman continuum leakage on physical properties of star-forming galaxies at $\mathbf{3.1 \lesssim z \lesssim 3.5}$Jul 1, 2021The VANDELS survey: global properties of CIII]$λ$1908Å emitting star-forming galaxies at z$\sim$3Sep 22, 2020FR-type radio sources at 3 GHz VLA-COSMOS: Relation to physical properties and large-scale environmentMar 30, 2020The deep Chandra survey in the SDSS J1030+0524 field