The VIMOS VLT deep survey (VVDS)

被引：0

作者：

Pello, R.

Le Fevre, O. ^{[1
]}

Adami, C. ^{[1
,2
]}

Arnaboldi, M.

Arnouts, S. ^{[1
]}

Bardelli, S.

Bolzonella, M. ^{[6
]}

Bongiorno, A. ^{[6
]}

Bondi, M. ^{[2
]}

Bottini, D. ^{[3
]}

Busarello, G.

Cappi, A.

Charlot, S. ^{[7
]}

Ciliegi, P.

Contini, T. ^{[8
]}

Foucaud, S. ^{[3
,9
]}

Franzetti, P.

Garilli, B. ^{[3
]}

Gavignaud, I. ^{[10
]}

Guzzo, L. ^{[11
]}

Ilbert, O. ^{[1
]}

Iovino, A. ^{[11
]}

Lamareille, F.

Le Brun, V. ^{[1
]}

Maccagni, D. ^{[3
]}

Marano, B. ^{[6
]}

Marinoni, C. ^{[1
,12
]}

Mathez, G.

Mazure, A.

McCracken, H. J. ^{[7
]}

Mellier, Y. ^{[7
]}

Meneux, B.

Merluzzi, P. ^{[5
]}

Merighi, R. ^{[2
]}

Paltani, S. ^{[13
,14
]}

Picat, J. P.

Pollo, A. ^{[8
,15
,16
]}

Pozzetti, L.

Radovich, M.

Ripepi, V.

Rizzo, D.

Scaramella, R. ^{[2
,4
]}

Scodeggio, M. ^{[3
]}

Tresse, L. ^{[1
]}

Vettolani, G. ^{[2
,5
]}

Zanichelli, A. ^{[5
]}

Zamorani, G. ^{[2
]}

Zucca, E. ^{[2
]}

机构：

[1] Univ Aix Marseille, LAM, CNRS, F-13012 Marseille, France

[2] INAF Osservatorio Astronom Bologna, I-40127 Bologna, Italy

[3] IASF INAF, I-20133 Milan, Italy

[4] INAF Osservatorio Astronom Roma, I-00040 Monte Porzio Catone, Italy

[5] INAF IRA, I-40129 Bologna, Italy

[6] Univ Bologna, Dipartimento Astron, I-40127 Bologna, Italy

[7] Univ Paris 06, CNRS, UMR 7095, Inst Astrophys Paris, F-75014 Paris, France

[8] Inst Recherche Astrophys & Planetol, F-31400 Toulouse, France

[9] Natl Taiwan Normal Univ, Dept Earth Sci, Taipei 11677, Taiwan

[10] Univ Andres Bello, Dept Ciencias Fis, Santiago, Chile

[11] INAF Osservatorio Astron Brera, Milan, Italy

[12] Aix Marseille Univ, CNRS, Ctr Phys Theor, F-13288 Marseille, France

[13] Integral Sci Data Ctr, Geneve, CH-1290 Versoix, Switzerland

[14] Observ Geneva, CH-1290 Sauverny, Switzerland

[15] Astron Observ Jagiellonian Univ, PL-30244 Krakow, Poland

[16] Natl Ctr Nuclear Res, PL-00681 Warsaw, Poland

来源：

HIGHLIGHTS OF SPANISH ASTROPHYSICS IV | 2007年

关键词：

D O I：

10.1007/978-1-4020-6000-7_4

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

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 similar to 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 type-density relation with redshift, and the clustering properties from z similar to 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).

引用

页码：41 / +

页数：3

共 50 条

[1] The VIMOS VLT Deep Survey
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Picat, J.P.
Scaramella, R.
Tresse, L.
Vettolani, G.
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Arnouts, S.
Bardelli, S.
Bolzonella, M.
Cappi, A.
Ciliegi, P.
Foucaud, S.
Gavignaud, I.
Ilbert, O.
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Marinoni, C.
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Radovich, M.
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Astronomy and Astrophysics, 2008, 487 (01): : 89 - 101
[2] The vimos VLT deep survey
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Cucciati, O.
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Ilbert, O.
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Pellò, R.
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[3] The VIMOS-VLT Deep Survey (VVDS) -: The dependence of clustering on galaxy stellar mass at z ∼ 1
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