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most citedA test of the nature of cosmic acceleration using galaxy redshift distortions

670 citations · 1.7k across the 26 of their papers we have counts for

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Showing 2006Show all

8 papers · 1 filter

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-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-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-ph200666 cited

The ATESP 5 GHz radio survey I. Source counts and spectral index properties of the faint radio population

I. Prandoni, P. Parma, M. H. Wieringa +5

[Abridged] The nature and evolutionary properties of the faint radio population, responsible for the steepening observed in the 1.4 GHz source counts below 1 milliJy, are not yet e…

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…

astro-ph2006109 cited

The VIMOS-VLT Deep Survey. Color bimodality and the mix of galaxy populations up to z~2

P. Franzetti, M. Scodeggio, B. Garilli +41

In this paper we discuss the mix of star-forming and passive galaxies up to z~2, based on the first epoch VIMOS-VLT Deep Survey (VVDS) data.In agreement with previous works we find…