Showing 1–20 of 45 results
/ Date/ Name
Sep 6, 2004The VIMOS VLT Deep Survey - First epoch VVDS-Deep survey: 11564 spectra with 17.5<=IAB<=24, and the redshift distribution over 0< z <=5Sep 6, 2004The VIMOS VLT Deep Survey: Computing the two point correlation statistics and associated uncertaintiesMar 8, 2006The VIMOS VLT Deep Survey: The build-up of the colour-density relationJan 9, 2007Studying the evolution of large-scale structure with the VIMOS-VLT Deep SurveyJan 25, 2007VVDS-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 photometryApr 12, 2007The VIMOS VLT Deep Survey. The Assembly History of the Stellar Mass in Galaxies: from the Young to the Old UniverseFeb 2, 1996AGAPE, a microlensing search in the direction of M31: status ReportNov 27, 2008On the nature of faint Low Surface Brightness galaxies in the Coma clusterJun 19, 2006Deep and wide field imaging of the Coma cluster: the dataJul 25, 2006A deep wide survey of faint low surface brightness galaxies in the direction of the Coma cluster of galaxiesDec 5, 2006Witnessing the build-up of the colour-density relationOct 3, 2007Geometrical tests of cosmological models. III. The cosmology-evolution diagram at z=1Dec 17, 1998AgapeZ1: a Large Amplification Microlensing Event or an Odd Variable Star Towards the Inner Bulge of M31May 20, 2004Variable stars towards the bulge of M31: the AGAPE catalogueNov 20, 2003Early results from the VIMOS VLT Deep SurveyFeb 9, 2004VVDS: early results on LSS distribution to z~1.5Sep 10, 2004The VLT-VIMOS Mask Preparation SoftwareNov 22, 2005The VIMOS-VLT Deep Survey - The evolution of galaxy clustering per spectral type to z~1.5Jul 28, 2005The VIRMOS deep imaging survey IV: Near-infrared observationsJun 23, 2005The VIMOS VLT Deep Survey: Evolution of the non-linear galaxy bias up to z=1.5