activity
20172022
most citedThe ALPINE-ALMA [CII] survey: Star-formation-driven outflows and circumgalactic enrichment in the early Universe

170 citations · 344 across the 6 of their papers we have counts for

collaborators

15 papers

astro-ph.GA202215 cited

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…

astro-ph.GA202159 cited

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…

astro-ph.GA202143 cited

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…

astro-ph.GA2021

The ALPINE-ALMA [CII] Survey: Kinematic Diversity & Rotation in Massive Star Forming Galaxies at z~4.4-5.9

G. C. Jones, D. Vergani, M. Romano +21

While the kinematics of galaxies up to z~3 have been characterized in detail, only a handful of galaxies at high redshift (z>4) have been examined in such a way. The Atacama Large…

astro-ph.GA2020

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…

astro-ph.GA2020

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,…