127 citations · 1k across the 25 of their papers we have counts for
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The ALPINE-ALMA [CII] Survey: the population of [CII]-undetected galaxies and their role in the -SFR relation
Michael Romano, L. Morselli, P. Cassata +22
The [CII] 158m emission line represents so far one of the most profitable tools for the investigation of the high-redshift galaxies in the early Universe. Being one of the brig…
The ALPINE-ALMA [CII] Survey: Investigation of 10 Galaxies at with [OII] and [CII] Line Emission ISM Properties and [OII]SFR Relation
Brittany N. Vanderhoof, A. L. Faisst, L. Shen +23
We present main-sequence ALPINE galaxies (log() = 9.2-11.1 and ) at with optical [OII] measurements from Ke…
The ALPINE-ALMA [CII] survey: The contribution of major mergers to the galaxy mass assembly at z~5
M. Romano, P. Cassata, L. Morselli +25
Galaxy mergers are thought to be one of the main mechanisms of the mass assembly of galaxies. Recently, many works have suggested a possible increase in the fraction of major merge…
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…
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…