Le Févre, O. et al. 2015, A&A, 576, 79
The VIMOS Ultra-Deep Survey: ~10,000 galaxies with spectroscopic redshifts to study galaxy assembly at early epochs 2 < z ≲ 6

Tasca, L. et al. 2014, A&A, 565, 10
Evidence for major mergers of galaxies at 2 ≲ z < 4 in the VVDS and VUDS surveys

Amorín, R. et al. 2014, A&A, 568, L8
Discovering extremely compact and metal-poor, star-forming dwarf galaxies out to z ~ 0.9 in the VIMOS Ultra-Deep Survey

Cucciati, O. et al. 2014, A&A, 570, 16
Discovery of a rich proto-cluster at z=2.9 and associated diffuse cold gas in the VIMOS Ultra-Deep Survey (VUDS)

Lemaux, B. et al. 2014, A&A, 572, 41
VIMOS Ultra-Deep Survey (VUDS): Witnessing the Assembly of a Massive Cluster at z~3.3

Cassata, P. et al. 2015, A&A 573, 24
The VIMOS Ultra-Deep Survey (VUDS): fast increase of the fraction of strong Lyman alpha emitters from z=2 to z=6

Durkalec, A. et al. 2015, A&A, 576, L7
The stellar mass - halo mass relation from galaxy clustering in VUDS: a high star formation efficiency at z~3

Tasca, L. et al. 2015, A&A, 581, 54
The evolving SFR-Mstar relation and sSFR since z~5 from the VUDS spectroscopic survey

Durkalec, A. et al. 2015, A&A, 583, 128
The evolution of clustering length, large-scale bias and host halo mass at 2 < z < 5 in the VIMOS Ultra Deep Survey

Hathi, N. et al. 2015, A&A, accepted
The VIMOS Ultra Deep Survey: Lyα Emission and Stellar Populations of Star-Forming Galaxies at 2< z < 2.5

Thomas, R. et al. 2014, arXiv:1411.5692
The VIMOS Ultra-Deep Survey (VUDS): IGM transmission towards galaxies with 2.5 < z < 5.5 and the colour selection of high redshift galaxies

Ribeiro, B. et al. 2016, arXiv:1602.01840
Size evolution of star-forming galaxies with 2 < z < 4.5 in the VIMOS Ultra-Deep Survey

Tasca, L. et al. 2016, arXiv:1602.01842
The VIMOS Ultra Deep Survey First Data Release: spectra and spectroscopic redshifts of 698 objects up to z~6 in CANDELS

Thomas, R. et al. 2016, arXiv:1602.01841
The extended epoch of galaxy formation: age dating of ~3600 galaxies with 2 < z < 6.5 in the VIMOS Ultra-Deep Survey