Highlights from the VIMOS VLT Deep Survey

O. Le Fèvre, B. Garilli, V. Le Brun, D. Maccagni, R. Scaramella, M. Scodeggio, L. Tresse, G. Vettolani, A. Zanichelli, C. Adami, S. Arnouts, S. Bardelli, M. Bolzonella, D. Bottini, A. Cappi, S. Charlot, P. Ciliegi, T. Contini, S. Foucaud, P. FranzettiI. Gavignaud, L. Guzzo, O. Ilbert, A. Iovino, F. Lamareille, H. J. McCracken, B. Marano, C. Marinoni, A. Mazure, B. Meneux, R. Merighi, S. Paltani, R. Pellò, A. Pollo, L. Pozzetti, M. Radovich, D. Vergani, G. Zamorani, E. Zucca, M. Bondi, A. Bongiorno, J. Brinchmann, O. Cucciati, S. De La Torre, L. De Ravel, L. Gregorini, E. Perez-Montero, Y. Mellier, P. Merluzzi, S. Temporin, C. J. Walcher

Research output: Contribution to journalReview articlepeer-review


Taking advantage of the efficient VIMOS multi-slit spectrograph on the VLT, we are conducting the VIMOS VLT Deep Survey (VVDS), aimed to trace the evolution of galaxies and large-scale structures over more than 90% of the life of the Universe. The VVDS is made of three magnitude selected surveys: the wide survey at IAB = 22.5, the deep survey at IAB = 24, and the ultra-deep survey at IAB = 24.75. To date, the VVDS has assembled more than 45000 redshifts in the range 0 < z ≤ 5. A number of results have been obtained, including a comprehensive view of the luminosity and stellar mass evolution as a function of galaxy type over 0 < z ≤ 2, a detailed look at the evolution of the clustering of galaxies as a function of type and environment, and a complete census of the actively star-forming galaxy population for 1.5 < z ≤ 5. This paper focuses on current highlights and on-going work from the VVDS.

Original languageEnglish
Pages (from-to)1115-1120
Number of pages6
JournalNuovo Cimento della Societa Italiana di Fisica B
Issue number9-11
Publication statusPublished - Sept 2007

ASJC Scopus subject areas

  • General Physics and Astronomy


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