activity
19972026
most citedDust-to-gas Ratio and Metal Abundance in Dwarf Galaxies

277 citations · 667 across the 14 of their papers we have counts for

collaborators

14 papers

astro-ph.GA2026

The gradual decline of Ly visibility in the CANDELS fields: evidence for the combined effects of galaxy evolution and reionization

L. Napolitano, L. Pentericci, A. Ferrara +35

We investigate the evolution of Ly visibility and the physical properties of Ly emitters (LAEs) across the five CANDELS fields using publicly available JWST/NIRSpec PRISM spe…

astro-ph.GA2025

Resolving dust and Lyα emission in a lensed galaxy at the epoch of reionization with JWST/CANUCS

V. Markov, M. Bradač, V. Estrada-Carpenter +20

Lyman emission is highly sensitive to dust and neutral hydrogen and is therefore expected to be strongly suppressed in dusty or gas-rich galaxies during the epoch of reionizati…

astro-ph.GA2025

Extreme equivalent width-selected low-mass starbursts at : insights into their role in cosmic reionization

M. Llerena, L. Pentericci, R. Amorín +22

We investigate the properties of extreme emission line galaxies (EELGs) at and their role in reionization. Compact, low-mass galaxies with intense optical emission lines ar…

astro-ph.GA2025★ 1 cited

Tentative rotation in a galaxy at z14 with ALMA

J. Scholtz, E. Parlanti, S. Carniani +20

We re-analysed ALMA observations of the [OIII]88m emission line in JADES-GS-z14.0, so far the most distant spectroscopically confirmed galaxy at z=14.18. Our analysis shows a…

astro-ph.GA2024★ 20 cited

The mass-metallicity relation as a ruler for galaxy evolution: insights from the James Webb Space Telescope

A. Pallottini, A. Ferrara, S. Gallerani +5

Galaxy evolution emerges from the balance between cosmic gas accretion, fueling star formation, and supernova (SN) feedback, regulating the metal enrichment. Hence, the stellar mas…

astro-ph.GA2024★ 51 cited

Gas-phase metallicity gradients in galaxies at

G. Venturi, S. Carniani, E. Parlanti +18

The study of gas-phase metallicity and its spatial distribution at high redshift is crucial to understand the processes that shaped the growth and evolution of galaxies in the earl…