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

670 citations · 1.8k across the 23 of their papers we have counts for

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astro-ph200846 cited

Physical properties of galaxies and their evolution in the VIMOS VLT Deep Survey. II. Extending the mass-metallicity relation to the range z=0.89-1.24

E. Perez-Montero, T. Contini, F. Lamareille +39

Aims. We present a continuation of our study about the relation between stellar mass and gas-phase metallicity in the VIMOS VLT Deep Survey (VVDS). In this work we extend the deter…

astro-ph200896 cited

Physical properties of galaxies and their evolution in the VIMOS VLT Deep Survey. I. The evolution of the mass-metallicity relation up to z~0.9

F. Lamareille, J. Brinchmann, T. Contini +43

We derive the mass-metallicity relation of star-forming galaxies up to , using data from the VIMOS VLT Deep Survey. Automatic measurement of emission-line fluxes and equi…

astro-ph200810 cited

The VVDS-VLA Deep Field - IV: Radio-optical properties

S. Bardelli, E. Zucca, M. Bolzonella +51

(abridged) We use the 1.4 GHz VIMOS-VLA Deep Survey and the optical VVDS and the CFHT-LS to compare the properties of radio loud galaxies with respect to the whole population of op…

astro-ph200835 cited

Eddington ratios of faint AGN at intermediate redshift: Evidence for a population of half-starved black holes

I. Gavignaud, L. Wisotzki, A. Bongiorno +51

We use one of the deepest spectroscopic samples of broad line active galactic nuclei (AGN) currently available, extracted from the VIMOS VLT Deep Survey (VVDS), to compute MgII and…

astro-ph200873 cited

The VVDS-SWIRE-GALEX-CFHTLS surveys: Physical properties of galaxies at z below 1.2 from photometric data

C. J. Walcher, F. Lamareille, D. Vergani +42

We intend to show that it is possible to derive the physical parameters of galaxies from their broad-band spectral energy distribution out to a redshift of 1.2. This method has the…

astro-ph2008162 cited

The Vimos VLT Deep Survey: Global properties of 20000 galaxies in the I_AB<=22.5 WIDE survey

B. Garilli, O. Le Fèvre, L. Guzzo +44

The VVDS-Wide survey has been designed with the general aim of tracing the large-scale distribution of galaxies at z~1 on comoving scales reaching ~100Mpc/h, while providing a good…