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most citedWitnessing the build-up of the colour-density relation

2 citations · 2 across the 3 of their papers we have counts for

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Showing 2006 · astro-phShow all

7 papers · 2 filters

astro-ph2006

The VIRMOS-VLT Deep Survey: the last 10 billion years of evolution of galaxy clustering

A. Pollo, L. Guzzo, O. Le Fevre +46

We discuss the evolution of clustering of galaxies in the Universe from the present epoch back to z ~ 2, using the first-epoch data from the VIMOS-VLT Deep Survey (VVDS). We presen…

astro-ph20061k cited

zCOSMOS: A Large VLT/VIMOS redshift survey covering 0 < z < 3 in the COSMOS field

S. J. Lilly, O. Le Fevre, A. Renzini +42

zCOSMOS is a large redshift survey that is being undertaken in the COSMOS field using 600 hours of observation with the VIMOS spectrograph on the 8-m VLT. The survey is designed to…

astro-ph20062 cited

Witnessing the build-up of the colour-density relation

O. Cucciati, A. Iovino, C. Marinoni +50

We investigate the redshift and luminosity evolution of the galaxy colour-density relation using the data from the First Epoch VIMOS-VLT Deep Survey (VVDS) on scales of R=5 h^(-1)M…

astro-ph2006

Studying the Evolution of Multi-Wavelength Emissivities with the Vimos VLT Deep Survey

L. Tresse, O. Ilbert, E. Zucca +4

The VIMOS VLT Deep Survey is a unique I-selected spectroscopic sample to study galaxies all the way from z=5 to z=0. We recapitulate the first results about the evolution of the ga…

astro-ph200676 cited

The cosmic star formation rate evolution from z=5 to z=0 from the VIMOS VLT Deep Survey

L. Tresse, O. Ilbert, E. Zucca +45

We present the evolution of the comoving SFR density in the redshift range 0 < z < 5 using the first epoch data release of the VVDS, that is 11564 spectra selected at I_AB=24 over…

astro-ph200615 cited

The VIMOS VLT Deep Survey:The ultraviolet galaxy luminosity function and luminosity density at 3<z<4

S. Paltani, O. Le Fevre, O. Ilbert +46

We study the LF of the high-z galaxy population with 3<z<4 using a purely I-band magnitude-selected spectroscopic sample obtained in the framework of the VVDS. We determine the LF…