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