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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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20 papers · 1 filter

astro-ph.CO2020★ 73 cited

Illuminating the dark side of cosmic star formation two billion years after the Big Bang

Margherita Talia, Andrea Cimatti, Marika Giulietti +5

How and when did galaxies form and assemble their stars and stellar mass? The answer to these questions, so crucial to astrophysics and cosmology, requires the full reconstruction…

astro-ph.GA2020★ 58 cited

The VANDELS survey: the relation between UV continuum slope and stellar metallicity in star-forming galaxies at z~3

A. Calabrò, M. Castellano, L. Pentericci +23

The estimate of stellar metallicities (Z*) of high-z galaxies are of paramount importance in order to understand the complexity of dust effects and the reciprocal interrelations am…

astro-ph.GA2020★ 70 cited

The VIMOS Ultra Deep Survey: The reversal of the star-formation rate density relation at

B. C. Lemaux, O. Cucciati, O. Le Fèvre +28

Utilizing spectroscopic observations taken for the VIMOS Ultra-Deep Survey (VUDS), new observations from Keck/DEIMOS, and publicly available observations of large samples of star-f…

astro-ph.GA2020★ 23 cited

The VANDELS survey: Discovery of massive overdensities of galaxies at z>2

L. Guaita, E. Pompei, M. Castellano +19

We want to investigate whether we can use Lyalpha emission to obtain information on the environment properties and whether Lyalpha emitters show different characteristics as a func…

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★ 6 cited

The VIMOS Ultra-Deep Survey: the Ly emission line morphology at

B. Ribeiro, O. Le Fèvre, A. Paulino-Afonso +20

The Lyman- (Ly) emission line has been ubiquitously used to confirm and study high redshift galaxies. We report on the line morphology as seen in the 2D spectra from the VIMO…