activity
20052025
most citedFragmentation of star-forming clouds enriched with the first dust

302 citations · 2.4k across the 42 of their papers we have counts for

collaborators
Showing 2023Show all

8 papers · 1 filter

astro-ph.GA2023★ 2 cited

The ALMA Reionization Era Bright Emission Line Survey (REBELS): The molecular gas content of galaxies at z~7

M. Aravena, K. E. Heintz, M. Dessauges-Zavadsky +18

A key to understanding the formation of the first galaxies is to quantify the content of the molecular gas as the fuel for star formation activity through the epoch of reionization…

astro-ph.GA2023★ 2 cited

The ALMA REBELS survey: obscured star formation in massive Lyman-break galaxies at z = 4-8 revealed by the IRX- and relations

R. A. A. Bowler, H. Inami, L. Sommovigo +23

We investigate the degree of dust obscured star formation in 49 massive () Lyman-break galaxies (LBGs) at - observed as par…

astro-ph.GA2023★ 109 cited

Stochastic star formation in early galaxies: JWST implications

A. Pallottini, A. Ferrara

The star formation rate (SFR) in high redshift galaxies is expected to be time-variable due to competing physical processes. Such stochastic variability might boost the luminosity…

astro-ph.GA2023★ 80 cited

XQR-30: the ultimate XSHOOTER quasar sample at the reionization epoch

Valentina D'Odorico, E. Banados, G. D. Becker +46

The final phase of the reionization process can be probed by rest-frame UV absorption spectra of quasars at z>6, shedding light on the properties of the diffuse intergalactic mediu…

astro-ph.CO2023★ 11 cited

CONCERTO: Extracting the power spectrum of the [C II ] emission line

M. Van Cuyck, N. Ponthieu, G. Lagache +21

CONCERTO is the first experiment to perform a [CII] line intensity mapping survey to target . Measuring the [CII] power spectrum allows us to study the role of dusty star-fo…

astro-ph.GA2023★ 38 cited

Dust attenuation law in JWST galaxies at z = 7-8

V. Markov, S. Gallerani, A. Pallottini +5

Attenuation curves in galaxies depend on dust chemical composition, content, and grain size distribution. Such parameters are related to intrinsic galaxy properties such as metalli…