arXiv · astro-ph/0101034
The VIRMOS-VLT Deep Survey
Abstract
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.
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O. Le Fèvre, G. Vettolani, D. Maccagni, D. Mancini, A. Mazure, Y. Mellier, J. P. Picat, M. Arnaboldi, S. Bardelli, E. Bertin, G. Busarello, A. Cappi, S. Charlot, G. Chincarini, S. Colombi, B. Garilli, L. Guzzo, A. Iovino, V. Le Brun, M. Longhetti, G. Mathez, P. Merluzzi, H. J. McCracken, R. Pellò, L. Pozzetti, M. Radovich, V. Ripepi, P. Saracco, R. Scaramella, M. Scodeggio, L. Tresse, G. Zamorani, E. Zucca. 2001-01-03. The VIRMOS-VLT Deep Survey. https://doi.org/10.1007/10854354_65
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