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20052024
most citedThe lesser role of starbursts for star formation at z=2

867 citations · 19.7k across the 191 of their papers we have counts for

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19 papers · 1 filter

astro-ph.GA2023★ 20 cited

Early results from GLASS-JWST. XXVII. The mass-metallicity relation in lensed field galaxies at cosmic noon with NIRISS

Xianlong He, Xin Wang, Tucker Jones +20

We present a measurement of the mass-metallicity relation (MZR) at cosmic noon, using the JWST near-infrared wide-field slitless spectroscopy obtained by the GLASS-JWST Early Relea…

astro-ph.GA2023★ 5 cited

New insight on the nature of cosmic reionizers from the CEERS survey

S. Mascia, L. Pentericci, A. Calabrò +29

The Epoch of Reionization (EoR) began when galaxies grew in abundance and luminosity, so their escaping Lyman continuum (LyC) radiation started ionizing the surrounding neutral int…

astro-ph.GA2023★ 2 cited

The clustering properties of high-redshift passive galaxies

Manuela Magliocchetti, Paola Santini, Emiliano Merlin +1

We investigate the clustering properties of 3<z<5 candidate passive galaxies from the Merlin et al. (2019) sample residing in the GOODS-North (35 sources) and GOODS-South (33 sourc…

astro-ph.GA2023★ 6 cited

Identifying Lyα emitter candidates with Random Forest: learning from galaxies in CANDELS survey

L. Napolitano, L. Pentericci, A. Calabrò +8

The physical processes which make a galaxy a Lyman Alpha Emitter have been extensively studied for the past 25 years. However, the correlations between physical and morphological p…

astro-ph.GA2023★ 12 cited

Efficient NIRCam Selection of Quiescent Galaxies at 3 < z < 6 in CEERS

Arianna S. Long, Jacqueline Antwi-Danso, Erini L. Lambrides +30

Substantial populations of massive quiescent galaxies at challenge our understanding of rapid galaxy growth and quenching over short timescales. In order to piece together…

astro-ph.GA2023★ 34 cited

Near-infrared emission line diagnostics for AGN from the local Universe to redshift 3

Antonello Calabrò, Laura Pentericci, Anna Feltre +35

Optical rest-frame spectroscopic diagnostics are usually employed to distinguish between star formation and AGN-powered emission. However, this method is biased against dusty sourc…