activity
20032020
most citedzCOSMOS: A Large VLT/VIMOS redshift survey covering 0 < z < 3 in the COSMOS field

1k citations · 3.2k across the 14 of their papers we have counts for

collaborators

14 papers

astro-ph.GA2020★ 245 cited

The ALPINE-ALMA [CII] Survey: data processing, catalogs, and statistical source properties

M. Bethermin, Y. Fudamoto, M. Ginolfi +33

The ALPINE-ALMA large program targets the [CII] 158 m line and the far-infrared continuum in 118 spectroscopically confirmed star-forming galaxies between z=4.4 and z=5.9. It re…

astro-ph.IM2017★ 18 cited

The SPHERE data center: a reference for high contrast imaging processing

Ph. Delorme, N. Meunier, D. Albert +19

The objective of the SPHERE Data Center is to optimize the scientific return of SPHERE at the VLT, by providing optimized reduction procedures, services to users and publicly avail…

astro-ph.GA2016★ 119 cited

The VIMOS Ultra Deep Survey First Data Release: spectra and spectroscopic redshifts of 698 objects up to z~6 in CANDELS

L. A. M. Tasca, O. Le Fevre, B. Ribeiro +45

This paper describes the first data release (DR1) of the VIMOS Ultra Deep Survey (VUDS). The DR1 includes all low-resolution spectroscopic data obtained in 276.9 arcmin2 of the CAN…

astro-ph.CO2014★ 353 cited

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

O. Le Fevre, L. A. M. Tasca, P. Cassata +42

We present the VIMOS Ultra Deep Survey (VUDS), a spectroscopic redshift survey of ~10.000 very faint galaxies to study the major phase of galaxy assembly 2<z<~6. The survey covers…

astro-ph.CO2014★ 77 cited

VIMOS Ultra-Deep Survey (VUDS): Witnessing the Assembly of a Massive Cluster at z~3.3

B. C. Lemaux, O. Cucciati, L. A. M. Tasca +46

Using new spectroscopic observations obtained as part of the VIMOS Ultra-Deep Survey (VUDS), we perform a systematic search for overdense environments in the early universe ()…

astro-ph.GA2014★ 127 cited

The VIMOS Ultra-Deep Survey (VUDS): fast increase of the fraction of strong Lyman alpha emitters from z=2 to z=6

P. Cassata, L. A. M. Tasca, O. Le Fevre +42

Aims. The aim of this work is to constrain the evolution of the fraction of Lya emitters among UV selected star forming galaxies at 2<z<6, and to measure the stellar escape fractio…