activity
20032005
collaborators

6 papers

astro-ph2005

The VIMOS-VLT Deep Survey - The evolution of galaxy clustering per spectral type to z~1.5

B. Meneux, O. LeFevre, L. Guzzo +47

We measure the evolution of clustering for galaxies with different spectral types from 6495 galaxies with 17.5<=I_AB<=24 and measured spectroscopic redshift in the first epoch VIMO…

astro-ph2005

The Vimos VLT Deep Survey: Compact structures in the CDFS

C. Adami, A. Mazure, O. Ilbert +2

We have used the Vimos VLT Deep Survey in combination with other spectroscopic, photometric and X-ray surveys from literature to detect several galaxy structures in the Chandra Dee…

astro-ph2005

The VIMOS VLT Deep Survey: Evolution of the non-linear galaxy bias up to z=1.5

C. Marinoni, O. Le Fevre, B. Meneux +44

We present the first measurements of the Probability Distribution Function (PDF) of galaxy fluctuations in the VIMOS-VLT Deep Survey (VVDS) cone, covering 0.4x0.4 deg between 0.4<z…

astro-ph2004

The VIMOS VLT Deep Survey - The evolution of galaxy clustering to z=2 from first epoch observations

O. Le Fevre, L. Guzzo, B. Meneux +44

This paper presents the evolution of the clustering of the main population of galaxies from z=2.1 to z=0.2, from the first epoch VIMOS VLT Deep Survey (VVDS), a magnitude limited s…

astro-ph2003

The Low Frequency Radio Counterpart of the XMM Large Scale Structure Survey

A. S. Cohen, H. J. A. Röttgering, N. E. Kassim +8

The XMM Large Scale Structure Survey (XMM-LSS) is a major project to map the large scale structure of the universe out to cosmological distances. An 8 degree by 8 degree region wil…

astro-ph2003

The VLA-VIRMOS Deep Field I. Radio observations probing the microJy source population

M. Bondi. P. Ciliegi, G. Zamorani, L. Gregorini +32

We have conducted a deep survey (r.m.s noise 17 microJy) with the Very Large Array (VLA) at 1.4 GHz, with a resolution of 6 arcsec, of a 1 square degree region included in the VIRM…