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http://hub.abes.fr/edp/periodical/aa/2015/volume_581/issue_2015/aa25379-14/authorship/30
http://hub.abes.fr/edp/periodical/aa/2015/volume_576/issue_2015/aa23829-14/authorship/35
http://hub.abes.fr/edp/periodical/aa/2015/volume_585/issue_2015/aa26396-15/authorship/33
http://hub.abes.fr/edp/periodical/aa/2014/volume_573/issue_2014/aa23824-14/authorship/35
http://hub.abes.fr/edp/periodical/aa/2015/volume_576/issue_2015/aa25532-14/authorship/32
http://hub.abes.fr/edp/periodical/aa/2014/volume_562/issue_2014/aa22193-13/authorship/1
http://hub.abes.fr/edp/periodical/aa/2014/volume_572/issue_2014/aa23828-14/authorship/35
http://hub.abes.fr/edp/periodical/aa/2015/volume_582/issue_2015/aa25430-14/authorship/1
http://hub.abes.fr/edp/periodical/aa/2023/volume_678/issue_2023/aa46293-23/authorship/1
http://hub.abes.fr/edp/periodical/aa/2018/volume_612/issue_2018/aa31935-17/authorship/5
http://hub.abes.fr/edp/periodical/aa/2018/volume_616/issue_2018/aa33047-18/authorship/36
http://hub.abes.fr/edp/periodical/aa/2018/volume_619/issue_2018/aa33655-18/authorship/21
http://hub.abes.fr/edp/periodical/aa/2019/volume_625/issue_2019/aa32197-17/authorship/5
http://hub.abes.fr/edp/periodical/aa/2019/volume_630/issue_2019/aa35813-19/authorship/12
http://hub.abes.fr/edp/periodical/aa/2012/volume_539/issue_2012/aa17683-11/authorship/1
http://hub.abes.fr/edp/periodical/aa/2015/volume_583/issue_2015/aa25343-14/authorship/32
http://hub.abes.fr/edp/periodical/aa/2014/volume_568/issue_2014/aa23816-14/authorship/35
http://hub.abes.fr/edp/periodical/aa/2016/volume_586/issue_2016/aa26782-15/authorship/4
http://hub.abes.fr/edp/periodical/aa/2014/volume_570/issue_2014/aa23811-14/authorship/35
http://hub.abes.fr/edp/periodical/aa/2016/volume_588/issue_2016/aa26012-15/authorship/33
http://hub.abes.fr/edp/periodical/aa/2016/volume_593/issue_2016/aa26505-15/authorship/30
http://hub.abes.fr/edp/periodical/aa/2019/volume_632/issue_2019/aa36550-19/authorship/27
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The VIMOS Ultra-Deep Survey (VUDS): fast increase in the fraction of strong Lyman- α emitters from z = 2 to z = 6
Evolution of clustering length, large-scale bias, and host halo mass at 2 <z< 5 in the VIMOS Ultra Deep Survey (VUDS)
The Lyman continuum escape fraction of galaxies at z = 3.3 in the VUDS-LBC/COSMOS field
Dust attenuation in z ~ 1 galaxies from Herschel and 3D-HST H α measurements
Listening to galaxies tuning at z ~ 2.5-3.0: The first strikes of the Hubble fork
VIMOS Ultra-Deep Survey (VUDS): Witnessing the assembly of a massive cluster at z ~ 3.3
The VIMOS Ultra-Deep Survey: ~10 000 galaxies with spectroscopic redshifts to study galaxy assembly at early epochs 2 < z ≃ 6
The evolving star formation rate: M⋆ relation and sSFR since z ≃ 5 from the VUDS spectroscopic survey
Effect of the star formation histories on the SFR- M∗ relation at z ≥ 2
Discovering extremely compact and metal-poor, star-forming dwarf galaxies out to z ~ 0.9 in the VIMOS Ultra-Deep Survey
The VIMOS Ultra Deep Survey: Ly α emission and stellar populations of star-forming galaxies at 2 <z< 2.5
The VANDELS ESO public spectroscopic survey: The spectroscopic measurements catalogue
GMASS ultradeep spectroscopy of galaxies at z ~ 2
Discovery of a rich proto-cluster at z = 2.9 and associated diffuse cold gas in the VIMOS Ultra-Deep Survey (VUDS)
Stellar mass to halo mass relation from galaxy clustering in VUDS: a high star formation efficiency at z ≃ 3
The star formation rate cookbook at 1 < z < 3: Extinction-corrected relations for UV and [OII] λ3727 luminosities
The VIMOS Ultra Deep Survey: Nature, ISM properties, and ionizing spectra of C III] λ1909 emitters at z = 2-4
The VANDELS ESO public spectroscopic survey: Observations and first data release
The progeny of a cosmic titan: a massive multi-component proto-supercluster in formation at z = 2.45 in VUDS
The VIMOS Ultra-Deep Survey: evidence for AGN feedback in galaxies with CIII]- λ1908 Å emission 10.8 to 12.5 Gyr ago
The most massive, passive, and oldest galaxies at 0.5 < z< 2.1: Downsizing signature from galaxies selected from Mg UV index
A few StePS forward in unveiling the complexity of galaxy evolution: light-weighted stellar ages of intermediate-redshift galaxies with WEAVE
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