The VIRMOS-VLT Deep Survey

By O. Fèvre, G. Vettolani, D. Maccagni, Dario Mancini, A. Mazure, Y. Mellier, J. Picat, M. Arnaboldi, Sandro Bardelli, E. Bertin and 23 more. 2001

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The aim of the VIRMOS VLT Deep Survey (VVDS) is to study of the evolution of galaxies, large scale structures and AGNs from a sample of more than 150,000 galaxies with measured redshifts in the range 0<z<5+. The VVDS will rely on the VIMOS and NIRMOS wide field multi-object spectrographs, which the VIRMOS consortium is delivering to ESO. Together, they offer unprecedented multiplex capability in the wavelength range 0.37-1.8microns, allowing for large surveys to be carried out. The VVDS has several main aspects: (1) a deep multi-color imaging survey over 18deg^2 of more than one million galaxies, (2) a "wide" spectroscopic survey with more than 130,000 redshifts measured for objects brighter than IAB=22.5 over 18deg^2, (3) a "deep" survey with 50,000 redshifts measured to IAB=24, (4) ultra-deep" surveys with several thousand redshifts measured to IAB=25, (5) multi-wavelength observations with the VLA and XMM.

Subfields: Industrial and Manufacturing Engineering, Instrumentation, Media Technology

View Paper: https://www.semanticscholar.org/paper/d9f8a886532ad80f16a43be56e3f334834ec6cf8

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