170 citations · 1.4k across the 19 of their papers we have counts for
40 papers
High [OIII]/[CII] surface brightness ratios trace early starburst galaxies
L. Vallini, A. Ferrara, A. Pallottini +2
We study the impact of deviations from the Kennicutt-Schmidt relation (quantified by the `burstiness' parameter ), gas metallicity (), and density () on the observed [OI…
The ALPINE-ALMA [CII] survey: Dust mass budget in the early Universe
F. Pozzi, F. Calura, Y. Fudamoto +32
The dust content of normal galaxies and the dust mass density (DMD) at high-z (z>4) are unconstrained given the source confusion and the sensitivity limitations of previous observa…
Dust temperature in ALMA $\hbox{[C $\scriptstyle\rm II $]}$-detected high- galaxies
L. Sommovigo, A. Ferrara, S. Carniani +4
At redshift the far-infrared (FIR) continuum spectra of main-sequence galaxies are sparsely sampled, often with a single data point. The dust temperature thu…
Velocity dispersion in the interstellar medium of early galaxies
M. Kohandel, A. Pallottini, A. Ferrara +5
We study the structure of spatially resolved, line-of-sight velocity dispersion for galaxies in the Epoch of Reionization (EoR) traced by [CII] line emission. Our labo…
The ALPINE-ALMA [C II] survey: the luminosity function of serendipitous [C II] line emitters at
Federica Loiacono, Roberto Decarli, Carlotta Gruppioni +32
We present the first [CII] 158 m luminosity function (LF) at from a sample of serendipitous lines detected in the ALMA Large Program to INvestigate [CII] at Early time…
Missing [CII] emission from early galaxies
S. Carniani, A. Ferrara, R. Maiolino +9
ALMA observations have revealed that [CII] 158m line emission in high-z galaxies is ~2-3 more extended than the UV continuum emission. Here we explore whether surface br…