Studying the Evolution of Multi-Wavelength Emissivities with the Vimos VLT Deep Survey

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dc.creatorTresse, L.
dc.creatorIlbert, O.
dc.creatorZucca, E.
dc.creatorZamorani, G.
dc.creatorArnouts, S.
dc.creatorBardelli, S.
dc.creatorteam, the VVDS
dc.date2006-11-23
dc.date.accessioned2026-07-07T07:30:56Z
dc.date.available2026-07-07T07:30:56Z
dc.descriptionThe VIMOS VLT Deep Survey is a unique I-selected spectroscopic sample to study galaxies all the way from z=5 to z=0. We recapitulate the first results about the evolution of the galaxy populations as a function of type, morphology, environment and luminosity.
dc.description9 pages, 11 figures. To appear in the proceedings of the XLIst Rencontres de Moriond, XXVIth Astrophysics Moriond Meeting: "From dark halos to light", Eds. L.Tresse, S. Maurogordato and J. Tran Thanh Van (Editions Frontieres)
dc.identifierhttps://arxiv.org/abs/astro-ph/0611745
dc.identifierhttp://arxiv.org/abs/astro-ph/0611745
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/118575
dc.subjectAstrophysics
dc.titleStudying the Evolution of Multi-Wavelength Emissivities with the Vimos VLT Deep Survey
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