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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

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Showing 2022Show all

14 papers · 1 filter

astro-ph.GA2022★ 28 cited

[CII] halos in ALPINE galaxies: smoking-gun of galactic outflows?

E. Pizzati, A. Ferrara, A. Pallottini +3

ALMA observations have revealed that many high redshift galaxies are surrounded by extended (10-15 kpc) [CII]-emitting halos which are not predicted by even the most advanced zoom-…

astro-ph.GA2022★ 18 cited

Interpreting ALMA non-detections of JWST super-early galaxies

M. Kohandel, A. Ferrara, A. Pallottini +3

Recent attempts to detect [OIII] 88m emission from super-early () galaxy candidates observed by JWST have been unsuccessful. By using zoom-in simulations, we show that the…

astro-ph.CO2022

CONCERTO: Simulating the CO, [CII], and [CI] line emission of galaxies in a 117 field and the impact of field-to-field variance

A. Gkogkou, M. Béthermin, G. Lagache +29

In the submm regime, spectral line scans and line intensity mapping (LIM) are new promising probes for the cold gas content and star formation rate of galaxies across cosmic time.…

astro-ph.GA2022★ 44 cited

A new look at the infrared properties of z 5 galaxies

L. Sommovigo, A. Ferrara, S. Carniani +6

Recent ALMA large surveys unveiled the presence of significant dust continuum emission in star-forming galaxies at . Unfortunately, such large programs -- i.e. ALPINE ($z\sim…

astro-ph.GA2022★ 40 cited

The ALMA REBELS Survey: The Cosmic HI Gas Mass Density in Galaxies at

K. E. Heintz, P. A. Oesch, M. Aravena +12

The neutral atomic gas content of individual galaxies at large cosmological distances has until recently been difficult to measure due to the weakness of the hyperfine HI 21-cm tra…

astro-ph.GA2022

The ALMA REBELS Survey: Average [CII] sizes of Star-Forming Galaxies from to

Y. Fudamoto, R. Smit, R. A. A. Bowler +36

We present the average [CII] emission line sizes of UV-bright star-forming galaxies at . Our results are derived from a stacking analysis of [CII] $158\,\rm{…