Showing 1–20 of 24 results
/ Date/ Name
Mar 6, 2026The Collective Voice of Ly$α$ Emitters: Insights from JWST Stacked SpectroscopyFeb 20, 2026Investigating the role of mergers in galaxy assembly in the early Universe (z > 5)Dec 18, 2025The AGN nature of strong CIII emitters in the Early Universe with JWSTNov 11, 2025Euclid preparation: LXXXVII. Non-Gaussianity of 2-point statistics likelihood: Precise analysis of the matter power spectrum distributionOct 29, 2025Extreme equivalent width-selected low-mass starbursts at $z=4-9$: insights into their role in cosmic reionizationOct 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 ForecastsJun 10, 2025Euclid preparation: The NISP spectroscopy channel, on ground performance and calibrationMay 15, 2025Redshift evolution of Lyman continuum escape fraction after JWSTMay 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 2, 2024The ionizing photon production efficiency of star-forming galaxies at $z\sim 4-10$Oct 14, 2024Seven wonders of Cosmic Dawn: JWST confirms a high abundance of galaxies and AGNs at z $\simeq$ 9-11 in the GLASS fieldOct 14, 2024Spectroscopic confirmation of a dust-obscured, metal-rich dwarf galaxy at z~5Feb 17, 2024Peering into cosmic reionization: the Ly$α$ visibility evolution from galaxies at $z$ = 4.5-8.5 with JWSTMar 2, 2023Ionized gas kinematics and chemical abundances of low-mass star-forming galaxies at $z\sim 3$Jan 23, 2023Insights into the reionization epoch from cosmic-noon-CIV emitters in the VANDELS surveyJun 29, 2022Properties of the interstellar medium in star-forming galaxies at redshifts 2 < z < 5 from the VANDELS surveyJun 13, 2022Strong C IV emission from star-forming galaxies: a case for high Lyman continuum photon escape