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20062026
most citedEarly structure formation in quintessence models and its implications for cosmic reionisation from first stars

59 citations · 75 across the 5 of their papers we have counts for

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7 papers · 1 filter

astro-ph.GA2026

The Baryon Budget of Galaxies across the First Billion Years

Umberto Maio, Céline Péroux

We provide a complete census of the baryons in early galaxies to investigate the phases in which gas and stars reside, their corresponding budgets, depletion times, and stellar ret…

astro-ph.GA20252 cited

High [OI] emission lines: ColdSIM simulations and ALMA observations

Massimiliano Parente, Manuela Bischetti, Umberto Maio +8

Neutral-oxygen [OI] far-infrared emission lines at m and m are powerful probes of the physical conditions in the interstellar medium, although they have not been fully e…

astro-ph.GA2024

Molecular gas and dust properties in quasar hosts

Francesco Salvestrini, Chiara Feruglio, Roberta Tripodi +12

Observational campaigns hunting the elusive reservoirs of cold gas in the host galaxies of quasars at the epoch of reionization (EoR) are crucial for studying the formation and evo…

astro-ph.GA2024

Atomic and molecular gas as traced by [C II] emission

Benedetta Casavecchia, Umberto Maio, Céline Péroux +1

The latest ALMA and JWST observations provide new information on the birth and evolution of galaxies in the early Universe, at the epoch of reionization. Of particular importance a…

astro-ph.GA202414 cited

ColdSIM predictions of [C II] emission in primordial galaxies

Benedetta Casavecchia, Umberto Maio, Céline Péroux +1

A powerful tool to probe the gas content at high redshift is the [C II] 158 m sub-millimeter emission line, which, due to its low excitation potential and luminous emission, is…

astro-ph.GA2024

Intertwined Formation of , Dust, and Stars in Cosmological Simulations

Cinthia Ragone-Figueroa, Gian Luigi Granato, Massimiliano Parente +4

Context: Molecular hydrogen () is crucial in galaxy formation and evolution, serving as the main fuel for star formation (SF). In metal-enriched environments,