Showing 1–20 of 23 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 ForecastsAug 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 6505Oct 14, 2024Spectroscopic confirmation of a dust-obscured, metal-rich dwarf galaxy at z~5Aug 29, 2024The MICADO first light imager for the ELT: overview and current StatusMay 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 EuclidMay 3, 2023HYPerluminous quasars at the Epoch of ReionizatION (HYPERION). A new regime for the X-ray nuclear properties of the first quasarsDec 24, 2022CUBES: a UV spectrograph for the futureAug 2, 2022CUBES, the Cassegrain U-Band Efficient SpectrographMar 1, 2017The Lyman Continuum escape fraction of faint galaxies at z~3.3 in the CANDELS/GOODS-North, EGS, and COSMOS fields with LBCSep 6, 2010The Great Observatories Origins Deep Survey: Constraints on the Lyman Continuum Escape Fraction Distribution of Lyman--Break Galaxies at 3.4<z<4.5