Showing 1–20 of 33 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 20, 2025The radio flare and multi-wavelength afterglow of the short GRB 231117A: energy injection from a violent shell collisionJul 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 catalogueDec 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 EuclidNov 9, 2022SN 2022ann: A type Icn supernova from a dwarf galaxy that reveals helium in its circumstellar environmentNov 20, 2020The luminous red nova variety: AT 2020hat and AT 2020kogFeb 5, 2020Observational constraints on the optical and near-infrared emission from the neutron star-black hole binary merger S190814bvAug 4, 2017Hydrogen-Poor Superluminous Supernovae from the Pan-STARRS1 Medium Deep SurveyMay 17, 2016PS1-14bj: A Hydrogen-Poor Superluminous Supernova With a Long Rise and Slow DecayApr 26, 2016Supplement: Localization and broadband follow-up of the gravitational-wave transient GW150914Feb 26, 2016Localization and broadband follow-up of the gravitational-wave transient GW150914Jan 3, 2015The Nature and Orbit of the Ophiuchus StreamNov 4, 2014Zooming In on the Progenitors of Superluminous Supernovae With the HST