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20162026
most citedEuclid. I. Overview of the Euclid mission

550 citations · 3.8k across the 99 of their papers we have counts for

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Showing 2020Show all

14 papers · 1 filter

astro-ph.GA2020★ 48 cited

Scaling relations and baryonic cycling in local star-forming galaxies: II. Gas content and star-formation efficiency

L. K. Hunt, C. Tortora, M. Ginolfi +1

Assessments of the cold-gas reservoir in galaxies are a cornerstone for understanding star-formation processes and the role of feedback and baryonic cycling in galaxy evolution. He…

astro-ph.GA2020★ 101 cited

The ALPINE-ALMA [CII] Survey: Obscured Star Formation Rate Density and Main Sequence of star-forming galaxies at z>4

Y. Khusanova, M. Béthermin, O. Le Fèvre +30

Star formation rate (SFR) measurements at z>4 have relied mostly on rest-frame far-ultraviolet (FUV) observations. The corrections for dust attenuation based on IRX- relation ar…

astro-ph.GA2020★ 11 cited

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…

astro-ph.GA2020★ 200 cited

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★ 38 cited

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…

astro-ph.GA2020★ 122 cited

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,…