245 citations · 5.8k across the 91 of their papers we have counts for
14 papers · 1 filter
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…
The ALPINE-ALMA [CII] Survey: The nature, luminosity function and star formation history of dusty galaxies up to z~6
C. Gruppioni, M. Bethermin, F. Loiacono +30
We present the detailed characterisation of a sample of 56 sources serendipitously detected in ALMA band 7, as part of the ALMA Large Program to INvestigate CII at Early Times (ALP…
The ALPINE-ALMA [C II] Survey: [C II]158micron Emission Line Luminosity Functions at
Lin Yan, A. Sajina, F. Loiacono +28
We present the [CII]158m line luminosity functions (LFs) at using the ALMA observations of 118 sources, which are selected to have UV luminosity and…
The ALPINE-ALMA [CII] survey: Molecular gas budget in the Early Universe as traced by [CII]
M. Dessauges-Zavadsky, M. Ginolfi, F. Pozzi +32
The molecular gas content of normal galaxies at z>4 is poorly constrained, because the commonly used molecular gas tracers become hard to detect. We use the [CII]158um luminosity,…
The ALPINE-ALMA [CII] survey: Dust attenuation properties and obscured star formation at z~4.4-5.8
Yoshinobu Fudamoto, P. A. Oesch, A. Faisst +34
We present dust attenuation properties of spectroscopically confirmed star forming galaxies on the main sequence at a redshift of ~4.4-5.8. Our analyses are based on the far infrar…
Predicting FIR lines from simulated galaxies
Alessandro Lupi, Andrea Pallottini, Andrea Ferrara +3
Far-infrared (FIR) emission lines are a powerful tool to investigate the properties of the interstellar medium, especially in high-redshift galaxies, where ALMA observations have p…
Star formation law in the EoR from [CII] and CIII] lines
L. Vallini, A. Ferrara, A. Pallottini +2
We present a novel method to simultaneously characterise the star formation law and the interstellar medium properties of galaxies in the Epoch of Reionization (EoR) through the co…
The ALPINE-ALMA [CII] Survey: Size of Individual Star-Forming Galaxies at z=4-6 and their Extended Halo Structure
S. Fujimoto, J. D. Silverman, Matthieu Bethermin +31
We present the physical extent of [CII] 158um line-emitting gas from 46 star-forming galaxies at z=4-6 from the ALMA Large Program to INvestigate CII at Early Times (ALPINE). Using…
The ALPINE-ALMA [CII] Survey: On the nature of an extremely obscured serendipitous galaxy
Michael Romano, P. Cassata, L. Morselli +31
We report the serendipitous discovery of a bright galaxy (Gal-A) observed as part of the ALMA Large Program to INvestigate [CII] at Early times (ALPINE). While this galaxy is detec…
The ALPINE-ALMA [CII] survey. Little to no evolution in the [CII]-SFR relation over the last 13 Gyr
D. Schaerer, M. Ginolfi, M. Bethermin +34
The [CII] 158 micron line is one of the strongest IR emission lines, which has been shown to trace the star-formation rate (SFR) of galaxies in the nearby Universe and up to $z \si…
The ALPINE-ALMA [CII] Survey: data processing, catalogs, and statistical source properties
M. Bethermin, Y. Fudamoto, M. Ginolfi +33
The ALPINE-ALMA large program targets the [CII] 158 m line and the far-infrared continuum in 118 spectroscopically confirmed star-forming galaxies between z=4.4 and z=5.9. It re…
Outflows and extended [CII] halos in high redshift galaxies
Elia Pizzati, Andrea Ferrara, Andrea Pallottini +4
Recent stacked ALMA observations have revealed that normal, star-forming galaxies at are surrounded by extended () [CII] emitting halos which…