670 citations · 1.7k across the 26 of their papers we have counts for
6 papers · 1 filter
The ATESP 5 GHz radio survey. II. Physical properties of the faint radio population
A. Mignano, I. Prandoni, L. Gregorini +5
One of the most debated issues about sub-mJy radio sources, which are responsible for the steepening of the 1.4 GHz source counts, is the origin of their radio emission. Particular…
Geometrical tests of cosmological models. III. The cosmology-evolution diagram at z=1
C. Marinoni, A. Saintonge, T. Contini +22
The rotational velocity of distant galaxies, when interpreted as a size (luminosity) indicator, may be used as a tool to select high redshift standard rods (candles) and probe worl…
The VIMOS VLT Deep Survey: Tracing the galaxy stellar mass assembly history over the last 8Gyr
D. Vergani, M. Scodeggio, L. Pozzetti +46
We selected a mass-limited sample of 4048 objects from the VIMOS VLT Deep Survey in the redshift interval 0.5<z<1.3. We used the amplitude of the 4000 Balmer break (Dn4000) to sepa…
The VVDS type-1 AGN sample: The faint end of the luminosity function
A. Bongiorno, G. Zamorani, I. Gavignaud +51
In a previous paper (Gavignaud et al. 2006), we presented the type-1 Active Galactic Nuclei (AGN) sample obtained from the first epoch data of the VIMOS-VLT Deep Survey (VVDS). The…
Studying the evolution of large-scale structure with the VIMOS-VLT Deep Survey
L. Guzzo, O. Le Fevre, B. Meneux +16
The VIMOS-VLT Deep Survey (VVDS) currently offers a unique combination of depth, angular size and number of measured galaxies among surveys of the distant Universe: ~ 11,000 spectr…
VVDS-SWIRE: Clustering evolution from a spectroscopic sample of galaxies with redshift 0.2<z<2.1 selected from Spitzer IRAC 3.6 micron and 4.5 micron photometry
S. de la Torre, O. Le Fevre, S. Arnouts +53
By combining the VVDS with the SWIRE data, we have built the currently largest spectroscopic sample of galaxies selected in the rest-frame near-infrared. These allow us to investig…