activity
20092026
most citedA CEERS Discovery of an Accreting Supermassive Black Hole 570 Myr after the Big Bang: Identifying a Progenitor of Massive z > 6 Quasars

365 citations · 1.7k across the 58 of their papers we have counts for

collaborators
Showing 2021Show all

6 papers · 1 filter

astro-ph.GA2021★ 21 cited

New insights on the nebular emission, ionizing radiation and low metallicity of Green Peas from advanced modelling

Vital Fernández, R. Amorín, E. Pérez-Montero +3

Low-metallicity, compact starburst galaxies referred to as Green Peas (GPs) provide a unique window to study galactic evolution across cosmic epochs. In this work, we present new d…

astro-ph.GA2021★ 69 cited

(Re)Solving Reionization with Lyα: How Bright Lyα Emitters account for the Cosmic Ionizing Background

Jorryt Matthee, Rohan P. Naidu, Gabriele Pezzulli +12

The cosmic ionizing emissivity from star-forming galaxies has long been anchored to UV luminosity functions. Here we introduce an emissivity framework based on Ly emitters (LAEs…

astro-ph.GA2021★ 58 cited

No strong dependence of Lyman continuum leakage on physical properties of star-forming galaxies at

A. Saxena, L. Pentericci, R. S. Ellis +15

We present Lyman continuum (LyC) radiation escape fraction measurements for 183 spectroscopically confirmed star-forming galaxies in the redshift range $3.11 < z < 3…

astro-ph.GA2021

The VANDELS survey: global properties of CIII]1908Å emitting star-forming galaxies at z3

M. Llerena, R. Amorín, F. Cullen +17

We study the mean properties of a large representative sample of 217 galaxies showing CIII] emission at , selected from a parent sample of 750 main-sequence star-formi…

astro-ph.GA2021★ 23 cited

Measuring Chemical Abundances with Infrared Nebular Lines: HII-Chi-mistry-IR

J. A. Fernández-Ontiveros, E. Pérez-Montero, J. M. Vílchez +2

We provide a new method to derive heavy element abundances based on the unique suite of nebular lines in the mid- to far-infrared (IR) range. Using grids of photo-ionisation models…

astro-ph.CO2021★ 8 cited

The less and the more IGM transmitted galaxies from z~2.7 to z~6 from VANDELS and VUDS

R. Thomas, L. Pentericci, O. Le Fèvre +22

Aim. Our aim is to analyse the variance of the Inter-Galactic Medium transmission (IGM) by studying this parameter in the rest-frame UV spectra of a large sample of high redshift g…