The VIMOS ultra-deep survey: 10 000 galaxies with spectroscopic redshifts to study galaxy assembly at early epochs 2 < z 6

被引：0

作者：

Le Fèvre, O. ^{[1
]}

Tasca, L.A.M. ^{[1
]}

Cassata, P. ^{[1
]}

Garilli, B. ^{[3
]}

Le Brun, V. ^{[1
]}

MacCagni, D. ^{[3
]}

Pentericci, L. ^{[4
]}

Thomas, R. ^{[1
]}

Vanzella, E. ^{[2
]}

Zamorani, G. ^{[2
]}

Zucca, E. ^{[2
]}

Amorin, R. ^{[4
]}

Bardelli, S. ^{[2
]}

Capak, P. ^{[12
]}

Cassarà, L. ^{[3
]}

Castellano, M. ^{[4
]}

Cimatti, A. ^{[5
]}

Cuby, J.G. ^{[1
]}

Cucciati, O. ^{[2
,5
]}

De La Torre, S. ^{[1
]}

Durkalec, A. ^{[1
]}

Fontana, A. ^{[4
]}

Giavalisco, M. ^{[13
]}

Grazian, A. ^{[4
]}

Hathi, N.P. ^{[1
]}

Ilbert, O. ^{[1
]}

Lemaux, B.C. ^{[1
]}

Moreau, C. ^{[1
]}

Paltani, S. ^{[9
]}

Ribeiro, B. ^{[1
]}

Salvato, M. ^{[14
]}

Schaerer, D. ^{[8
,10
]}

Scodeggio, M. ^{[3
]}

Sommariva, V. ^{[4
,5
]}

Talia, M. ^{[5
]}

Taniguchi, Y. ^{[15
]}

Tresse, L. ^{[1
]}

Vergani, D. ^{[2
,6
]}

Wang, P.W. ^{[1
]}

Charlot, S. ^{[7
]}

Contini, T. ^{[8
]}

Fotopoulou, S. ^{[9
]}

López-Sanjuan, C. ^{[11
]}

Mellier, Y. ^{[7
]}

Scoville, N. ^{[12
]}

机构：

[1] Aix-Marseille Université, CNRS, Laboratoire d'Astrophysique de Marseille, Marseille,13388, France

[2] INAF-Osservatorio Astronomico di Bologna, via Ranzani, 1, Bologna,40127, Italy

[3] INAF, IASF, via Bassini 15, Milano,20133, Italy

[4] INAF-Osservatorio Astronomico di Roma, via di Frascati 33, Monte Porzio Catone,00040, Italy

[5] University of Bologna, Department of Physics and Astronomy (DIFA), V.le Berti Pichat, 6/2, Bologna,40127, Italy

[6] INAF, IASF Bologna, via Gobetti 101, Bologna,40129, Italy

[7] Institut d'Astrophysique de Paris, CNRS, Université Pierre et Marie Curie, 98bis boulevard Arago, Paris,75014, France

[8] Institut de Recherche en Astrophysique et Planétologie-IRAP, CNRS, Université de Toulouse, 14 avenue E. Belin, Toulouse,31400, France

[9] Department of Astronomy, University of Geneva, Ch. d'Écogia 16, Versoix,1290, Switzerland

[10] Geneva Observatory, University of Geneva, Ch. des Maillettes 51, Versoix,1290, Switzerland

[11] Centro de Estudios de Física Del Cosmos de Aragón, Teruel,44001, Spain

[12] Department of Astronomy, California Institute of Technology, 1200 E. California Blvd., Pasadena,CA,91125, United States

[13] Astronomy Department, University of Massachusetts, Amherst,MA,01003, United States

[14] Max-Planck-Institut für Extraterrestrische Physik, Postfach 1312, Garching bei München,85741, Germany

[15] Research Center for Space and Cosmic Evolution, Ehime University, Bunkyo-cho 2-5, Matsuyama,790-8577, Japan

来源：

Astronomy and Astrophysics | 2015年 / 576卷

关键词：

We thank the ESO staff for their continuous support for the VUDS survey; particularly the Paranal staff; who conduct the observations; and Marina Rejkuba and the ESO user support group in Garching. This work is supported by funding from the European Research Council Advanced Grant ERC-2010-AdG-268107-EARLY and by INAF Grants PRIN 2010; PRIN 2012 and PICS 2013. A.C; O.C; M.T. and V.S. acknowledge the grant MIUR PRIN 2010–2011. D.M. gratefully acknowledges LAM hospitality during the initial phases of the project. This work is based on data products made available at the CESAM data center; Laboratoire d’Astrophysique de Marseille. This work partly uses observations obtained with MegaPrime/MegaCam; a joint project of CFHT and CEA/DAPNIA; at the Canada-France-Hawaii Telescope (CFHT) which is operated by the National Research Council (NRC) of Canada; the Institut National des Sciences de l’Univers of the Centre National de la Recherche Scientifique (CNRS) of France; and the University of Hawaii. This work is based in part on data products produced at TERAPIX and the Canadian Astronomy Data Centre as part of the Canada-France-Hawaii Telescope Legacy Survey; a collaborative project of NRC and CNRS;

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104

引用

共 23 条

[21] ALMA SPECTROSCOPIC SURVEY IN THE HUBBLE ULTRA DEEP FIELD: THE INFRARED EXCESS OF UV-SELECTED z=2-10 GALAXIES AS A FUNCTION OF UV-CONTINUUM SLOPE AND STELLAR MASS
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ASTROPHYSICAL JOURNAL, 2016, 833 (01):
[22] The evolution of the near-infrared galaxy luminosity function and colour bimodality up to z≃2 rom the UKIDSS Ultra Deep Survey Early Data Release
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[23] THE MASSIVE AND DISTANT CLUSTERS OF WISE SURVEY. II. INITIAL SPECTROSCOPIC CONFIRMATION OF z ∼ 1 GALAXY CLUSTERS SELECTED FROM 10,000 deg2
Stanford, S. A.
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