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20112026
most citedThe VIMOS Ultra-Deep Survey: ~10,000 galaxies with spectroscopic redshifts to study galaxy assembly at early epochs 2<z<~6

353 citations · 6k across the 127 of their papers we have counts for

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Showing 2022Show all

10 papers · 1 filter

astro-ph.GA2022★ 13 cited

COSMOS-Web: An Overview of the JWST Cosmic Origins Survey

Caitlin M. Casey, Jeyhan S. Kartaltepe, Nicole E. Drakos +82

We present the survey design, implementation, and outlook for COSMOS-Web, a 255 hour treasury program conducted by the James Webb Space Telescope in its first cycle of observations…

astro-ph.GA2022★ 3 cited

The ALPINE-ALMA [CII] survey: The infrared-radio correlation and AGN fraction of star-forming galaxies at z 4.4-5.9

Lu Shen, Brian C. Lemaux, Lori M. Lubin +26

We present the radio properties of 66 spectroscopically-confirmed normal star-forming galaxies (SFGs) at in the COSMOS field that were [C II] detected in the Atacama La…

astro-ph.GA2022★ 18 cited

Properties of the interstellar medium in star-forming galaxies at redshifts 2 < z < 5 from the VANDELS survey

A. Calabrò, L. Pentericci, M. Talia +16

Gaseous flows inside and outside galaxies are key to understanding galaxy evolution, as they regulate their star formation activity across cosmic time. We study the ISM kinematics…

astro-ph.GA2022

The environmental dependence of the stellar and gas-phase mass-metallicity relation at 2 < z < 4

A. Calabro, L. Guaita, L. Pentericci +17

In the local universe, galaxies in clusters show different properties compared to more isolated systems. Understanding how this difference originates and whether it is already in p…

astro-ph.GA2022★ 13 cited

IR characteristic emission and dust properties of star-forming galaxies at 4.5 z 6.2

D. Burgarella, J. Bogdanoska, A. Nanni +31

The luminosity functions at z < 4 - 5 suggest that most galaxies have a relatively low stellar mass (logM_star = 10) and a low dust attenuation (A_FUV = 1.0). The physical properti…

astro-ph.GA2022★ 19 cited

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…