activity
19932022
most citedMass and environment as drivers of galaxy evolution in SDSS and zCOSMOS and the origin of the Schechter function

2k citations · 19.9k across the 179 of their papers we have counts for

collaborators

179 papers

astro-ph.GA2022★ 11 cited

Metal content of the circumgalactic medium around star-forming galaxies at z 2.6 as revealed by the VIMOS Ultra-Deep Survey

H. Méndez-Hernández, P. Cassata, E. Ibar +20

The circumgalactic medium (CGM) is the location where the interplay between large-scale outflows and accretion onto galaxies occurs. Metals in different ionization states flowing b…

astro-ph.GA2021★ 24 cited

The Type II AGN-host galaxy connection: insights from the VVDS and VIPERS surveys

G. Vietri, B. Garilli, M. Polletta +16

We present a study of optically-selected Type II AGN at 0.5 < z < 0.9 from the VIPERS and VVDS surveys, to investigate the connection between AGN activity and physical properties o…

astro-ph.GA2021★ 92 cited

The VANDELS ESO public spectroscopic survey: final Data Release of 2087 spectra and spectroscopic measurements

B. Garilli, R. McLure, L. Pentericci +94

VANDELS is an ESO Public Spectroscopic Survey designed to build a sample of high signal to noise, medium resolution spectra of galaxies at redshift between 1 and 6.5. Here we prese…

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★ 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…

astro-ph.GA2019★ 7 cited

The most massive, passive, and oldest galaxies at 0.5 < z < 2.1: Downsizing signature from galaxies selected from MgUV index

R. Thomas, O. Le Fèvre, G. Zamorani +10

Aims. We seek is to identify old and massive galaxies at 0.5<z<2.1 on the basis of the magnesium index MgUV and then study their physical properties. We computed the MgUV index bas…