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The VIMOS Ultra-Deep Survey: evidence for AGN feedback in galaxies with CIII]-1908Å~emission 10.8 to 12.5 Gyr ago
O. Le Fèvre, B. C. Lemaux, K. Nakajima +19
We analyze the CIII]-1908Åemission properties in a sample of 3899 star-forming galaxies (SFGs) at 2<z<3.8 from the VIMOS Ultra-Deep Survey (VUDS). We find a median EW(CIII])=2.0$\p…
Ly-Lyman Continuum connection in 3.5 < z < 4.3 star-forming galaxies from the VUDS survey
F. Marchi, L. Pentericci, L. Guaita +16
To identify the galaxies responsible for the reionization of the Universe, we must rely on the investigation of the Lyman Continuum (LyC) properties of z<5 star-forming galaxies, w…
The VIMOS Ultra Deep Survey: Nature, ISM properties, and ionizing spectra of CIII]1909 emitters at z=2-4
K. Nakajima, D. Schaerer, O. Le Fevre +12
Context: Ultraviolet (UV) emission-line spectra are used to spectroscopically confirm high-z galaxies and increasingly also to determine their physical properties. Aims: To interpr…
The VIMOS Ultra Deep Survey: The role of HI kinematics and HI column density on the escape of Lyalpha photons in star-forming galaxies at 2<z<4
L. Guaita, M. Talia, L. Pentericci +22
We selected a sample of 76 Lya emitting galaxies from the VIMOS Ultra Deep Survey (VUDS) at 2<z<4. We estimated the velocity of the neutral gas flowing out of the interstellar medi…
Reconstructing the galaxy density field with photometric redshifts: II. Environment-dependent galaxy evolution since
Nicola Malavasi, Lucia Pozzetti, Olga Cucciati +3
Although extensively investigated, the role of the environment in galaxy formation is still not well understood. In this context, the Galaxy Stellar Mass Function (GSMF) is a power…
The VIMOS Ultra Deep Survey: Emerging from the Dark, a Massive Proto-Cluster at z~4.57
B. C. Lemaux, O. Le Fèvre, O. Cucciati +20
Using spectroscopic observations taken for the VIMOS Ultra-Deep Survey (VUDS) we report here on the discovery of PCl J1001+0220, a massive proto-cluster located at $z_{spec}\sim4.5…