The VIMOS VLT deep survey (VVDS)

R. Pelló, O. Le Fèvre, C. Adami, M. Arnaboldi, S. Arnouts, S. Bardelli, M. Bolzonella, A. Bongiorno, M. Bondi, D. Bottini, G. Busarello, A. Cappi, S. Charlot, P. Ciliegi, T. Contini, S. Foucaud, P. Franzetti, B. Garilli, I. Gavignaud, L. GuzzoO. Ilbert, A. Iovino, F. Lamareille, V. Le Brun, D. Maccagni, B. Marano, C. Marinoni, G. Mathez, A. Mazure, H. J. McCracken, Y. Mellier, B. Meneux, P. Merluzzi, R. Merighi, S. Paltani, J. P. Picat, A. Pollo, L. Pozzetti, M. Radovich, V. Ripepi, D. Rizzo, R. Scaramella, M. Scodeggio, L. Tresse, G. Vettolani, A. Zanichelli, G. Zamorani, E. Zucca

Resultado de la investigación: Conference contribution

Resumen

This paper reviews the main results obtained so far by the VIRMOS VLT Deep Survey (VVDS) collaboration. The VVDS is one of the leading extragalactic surveys, started in 2002 using GTO awarded for the construction of VIMOS-VLT. Its aim is to study the evolution of galaxies, large-scale structures, and AGNs from a goal sample of ∼100,000 objects down to a magnitude I(AB)=24, with redshifts measured using VIMOS-VLT (typically in the range 0 < z < 5), and a wide wavelength coverage from different follow-up observations. Among the most important results achived by the VVDS so far are the redshift distributions for different galaxy populations, the evolution of the galaxy Luminosity Function in various filter bands (as a function of redshift, galaxy type, and environment), the evolution of the typedensity relation with redshfit, and the clustering properties from z ∼ 2. One of the most impressive findings of the VVDS using a pure magnitude-selected sample is the existence of an important population of bright galaxies at 1.6 < z < 5, 1.6 to 6.2 times larger than previous estimates based on color preselections (LBG technique).

Idioma originalEnglish
Título de la publicación alojadaHighlights of Spanish Astrophysics IV - Proceedings of the 7th Scientific Meeting of the Spanish Astronomical Society, SEA 2006
Páginas41-48
Número de páginas8
DOI
EstadoPublished - 1 dic 2007
Evento7th Scientific Meeting of the Spanish Astronomical Society, SEA 2006 - Barcelona, Spain
Duración: 12 sep 200615 sep 2006

Other

Other7th Scientific Meeting of the Spanish Astronomical Society, SEA 2006
PaísSpain
CiudadBarcelona
Período12/09/0615/09/06

Huella dactilar

galaxies
luminosity
color
filters
estimates
wavelengths

ASJC Scopus subject areas

  • Astronomy and Astrophysics

Citar esto

Pelló, R., Fèvre, O. L., Adami, C., Arnaboldi, M., Arnouts, S., Bardelli, S., ... Zucca, E. (2007). The VIMOS VLT deep survey (VVDS). En Highlights of Spanish Astrophysics IV - Proceedings of the 7th Scientific Meeting of the Spanish Astronomical Society, SEA 2006 (pp. 41-48) https://doi.org/10.1007/978-1-4020-6000-7-4
Pelló, R. ; Fèvre, O. Le ; Adami, C. ; Arnaboldi, M. ; Arnouts, S. ; Bardelli, S. ; Bolzonella, M. ; Bongiorno, A. ; Bondi, M. ; Bottini, D. ; Busarello, G. ; Cappi, A. ; Charlot, S. ; Ciliegi, P. ; Contini, T. ; Foucaud, S. ; Franzetti, P. ; Garilli, B. ; Gavignaud, I. ; Guzzo, L. ; Ilbert, O. ; Iovino, A. ; Lamareille, F. ; Brun, V. Le ; Maccagni, D. ; Marano, B. ; Marinoni, C. ; Mathez, G. ; Mazure, A. ; McCracken, H. J. ; Mellier, Y. ; Meneux, B. ; Merluzzi, P. ; Merighi, R. ; Paltani, S. ; Picat, J. P. ; Pollo, A. ; Pozzetti, L. ; Radovich, M. ; Ripepi, V. ; Rizzo, D. ; Scaramella, R. ; Scodeggio, M. ; Tresse, L. ; Vettolani, G. ; Zanichelli, A. ; Zamorani, G. ; Zucca, E. / The VIMOS VLT deep survey (VVDS). Highlights of Spanish Astrophysics IV - Proceedings of the 7th Scientific Meeting of the Spanish Astronomical Society, SEA 2006. 2007. pp. 41-48
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title = "The VIMOS VLT deep survey (VVDS)",
abstract = "This paper reviews the main results obtained so far by the VIRMOS VLT Deep Survey (VVDS) collaboration. The VVDS is one of the leading extragalactic surveys, started in 2002 using GTO awarded for the construction of VIMOS-VLT. Its aim is to study the evolution of galaxies, large-scale structures, and AGNs from a goal sample of ∼100,000 objects down to a magnitude I(AB)=24, with redshifts measured using VIMOS-VLT (typically in the range 0 < z < 5), and a wide wavelength coverage from different follow-up observations. Among the most important results achived by the VVDS so far are the redshift distributions for different galaxy populations, the evolution of the galaxy Luminosity Function in various filter bands (as a function of redshift, galaxy type, and environment), the evolution of the typedensity relation with redshfit, and the clustering properties from z ∼ 2. One of the most impressive findings of the VVDS using a pure magnitude-selected sample is the existence of an important population of bright galaxies at 1.6 < z < 5, 1.6 to 6.2 times larger than previous estimates based on color preselections (LBG technique).",
author = "R. Pell{\'o} and F{\`e}vre, {O. Le} and C. Adami and M. Arnaboldi and S. Arnouts and S. Bardelli and M. Bolzonella and A. Bongiorno and M. Bondi and D. Bottini and G. Busarello and A. Cappi and S. Charlot and P. Ciliegi and T. Contini and S. Foucaud and P. Franzetti and B. Garilli and I. Gavignaud and L. Guzzo and O. Ilbert and A. Iovino and F. Lamareille and Brun, {V. Le} and D. Maccagni and B. Marano and C. Marinoni and G. Mathez and A. Mazure and McCracken, {H. J.} and Y. Mellier and B. Meneux and P. Merluzzi and R. Merighi and S. Paltani and Picat, {J. P.} and A. Pollo and L. Pozzetti and M. Radovich and V. Ripepi and D. Rizzo and R. Scaramella and M. Scodeggio and L. Tresse and G. Vettolani and A. Zanichelli and G. Zamorani and E. Zucca",
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Pelló, R, Fèvre, OL, Adami, C, Arnaboldi, M, Arnouts, S, Bardelli, S, Bolzonella, M, Bongiorno, A, Bondi, M, Bottini, D, Busarello, G, Cappi, A, Charlot, S, Ciliegi, P, Contini, T, Foucaud, S, Franzetti, P, Garilli, B, Gavignaud, I, Guzzo, L, Ilbert, O, Iovino, A, Lamareille, F, Brun, VL, Maccagni, D, Marano, B, Marinoni, C, Mathez, G, Mazure, A, McCracken, HJ, Mellier, Y, Meneux, B, Merluzzi, P, Merighi, R, Paltani, S, Picat, JP, Pollo, A, Pozzetti, L, Radovich, M, Ripepi, V, Rizzo, D, Scaramella, R, Scodeggio, M, Tresse, L, Vettolani, G, Zanichelli, A, Zamorani, G & Zucca, E 2007, The VIMOS VLT deep survey (VVDS). En Highlights of Spanish Astrophysics IV - Proceedings of the 7th Scientific Meeting of the Spanish Astronomical Society, SEA 2006. pp. 41-48, 7th Scientific Meeting of the Spanish Astronomical Society, SEA 2006, Barcelona, Spain, 12/09/06. https://doi.org/10.1007/978-1-4020-6000-7-4

The VIMOS VLT deep survey (VVDS). / Pelló, R.; Fèvre, O. Le; Adami, C.; Arnaboldi, M.; Arnouts, S.; Bardelli, S.; Bolzonella, M.; Bongiorno, A.; Bondi, M.; Bottini, D.; Busarello, G.; Cappi, A.; Charlot, S.; Ciliegi, P.; Contini, T.; Foucaud, S.; Franzetti, P.; Garilli, B.; Gavignaud, I.; Guzzo, L.; Ilbert, O.; Iovino, A.; Lamareille, F.; Brun, V. Le; Maccagni, D.; Marano, B.; Marinoni, C.; Mathez, G.; Mazure, A.; McCracken, H. J.; Mellier, Y.; Meneux, B.; Merluzzi, P.; Merighi, R.; Paltani, S.; Picat, J. P.; Pollo, A.; Pozzetti, L.; Radovich, M.; Ripepi, V.; Rizzo, D.; Scaramella, R.; Scodeggio, M.; Tresse, L.; Vettolani, G.; Zanichelli, A.; Zamorani, G.; Zucca, E.

Highlights of Spanish Astrophysics IV - Proceedings of the 7th Scientific Meeting of the Spanish Astronomical Society, SEA 2006. 2007. p. 41-48.

Resultado de la investigación: Conference contribution

TY - GEN

T1 - The VIMOS VLT deep survey (VVDS)

AU - Pelló, R.

AU - Fèvre, O. Le

AU - Adami, C.

AU - Arnaboldi, M.

AU - Arnouts, S.

AU - Bardelli, S.

AU - Bolzonella, M.

AU - Bongiorno, A.

AU - Bondi, M.

AU - Bottini, D.

AU - Busarello, G.

AU - Cappi, A.

AU - Charlot, S.

AU - Ciliegi, P.

AU - Contini, T.

AU - Foucaud, S.

AU - Franzetti, P.

AU - Garilli, B.

AU - Gavignaud, I.

AU - Guzzo, L.

AU - Ilbert, O.

AU - Iovino, A.

AU - Lamareille, F.

AU - Brun, V. Le

AU - Maccagni, D.

AU - Marano, B.

AU - Marinoni, C.

AU - Mathez, G.

AU - Mazure, A.

AU - McCracken, H. J.

AU - Mellier, Y.

AU - Meneux, B.

AU - Merluzzi, P.

AU - Merighi, R.

AU - Paltani, S.

AU - Picat, J. P.

AU - Pollo, A.

AU - Pozzetti, L.

AU - Radovich, M.

AU - Ripepi, V.

AU - Rizzo, D.

AU - Scaramella, R.

AU - Scodeggio, M.

AU - Tresse, L.

AU - Vettolani, G.

AU - Zanichelli, A.

AU - Zamorani, G.

AU - Zucca, E.

PY - 2007/12/1

Y1 - 2007/12/1

N2 - This paper reviews the main results obtained so far by the VIRMOS VLT Deep Survey (VVDS) collaboration. The VVDS is one of the leading extragalactic surveys, started in 2002 using GTO awarded for the construction of VIMOS-VLT. Its aim is to study the evolution of galaxies, large-scale structures, and AGNs from a goal sample of ∼100,000 objects down to a magnitude I(AB)=24, with redshifts measured using VIMOS-VLT (typically in the range 0 < z < 5), and a wide wavelength coverage from different follow-up observations. Among the most important results achived by the VVDS so far are the redshift distributions for different galaxy populations, the evolution of the galaxy Luminosity Function in various filter bands (as a function of redshift, galaxy type, and environment), the evolution of the typedensity relation with redshfit, and the clustering properties from z ∼ 2. One of the most impressive findings of the VVDS using a pure magnitude-selected sample is the existence of an important population of bright galaxies at 1.6 < z < 5, 1.6 to 6.2 times larger than previous estimates based on color preselections (LBG technique).

AB - This paper reviews the main results obtained so far by the VIRMOS VLT Deep Survey (VVDS) collaboration. The VVDS is one of the leading extragalactic surveys, started in 2002 using GTO awarded for the construction of VIMOS-VLT. Its aim is to study the evolution of galaxies, large-scale structures, and AGNs from a goal sample of ∼100,000 objects down to a magnitude I(AB)=24, with redshifts measured using VIMOS-VLT (typically in the range 0 < z < 5), and a wide wavelength coverage from different follow-up observations. Among the most important results achived by the VVDS so far are the redshift distributions for different galaxy populations, the evolution of the galaxy Luminosity Function in various filter bands (as a function of redshift, galaxy type, and environment), the evolution of the typedensity relation with redshfit, and the clustering properties from z ∼ 2. One of the most impressive findings of the VVDS using a pure magnitude-selected sample is the existence of an important population of bright galaxies at 1.6 < z < 5, 1.6 to 6.2 times larger than previous estimates based on color preselections (LBG technique).

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U2 - 10.1007/978-1-4020-6000-7-4

DO - 10.1007/978-1-4020-6000-7-4

M3 - Conference contribution

AN - SCOPUS:84890036354

SN - 9781402059995

SP - 41

EP - 48

BT - Highlights of Spanish Astrophysics IV - Proceedings of the 7th Scientific Meeting of the Spanish Astronomical Society, SEA 2006

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Pelló R, Fèvre OL, Adami C, Arnaboldi M, Arnouts S, Bardelli S y otros. The VIMOS VLT deep survey (VVDS). En Highlights of Spanish Astrophysics IV - Proceedings of the 7th Scientific Meeting of the Spanish Astronomical Society, SEA 2006. 2007. p. 41-48 https://doi.org/10.1007/978-1-4020-6000-7-4