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Free access article
A&A 428, 1043-1049 (2004)
DOI: 10.1051/0004-6361:20048072
The VIMOS VLT Deep Survey
Public release of 1599 redshifts to I
across the Chandra Deep Field South
O. Le Fèvre1, G. Vettolani2, S. Paltani1, L. Tresse1, G. Zamorani3, V. Le Brun1, C. Moreau1, D. Bottini4, D. Maccagni4, J. P. Picat5, R. Scaramella2, M. Scodeggio4, A. Zanichelli2, C. Adami1, S. Arnouts1, S. Bardelli3, M. Bolzonella6, A. Cappi3, S. Charlot7, 8, T. Contini5, S. Foucaud4, P. Franzetti4, B. Garilli4, I. Gavignaud5, 9, L. Guzzo10, O. Ilbert1, A. Iovino10, H. J. McCracken7, 11, D. Mancini12, B. Marano6, C. Marinoni1, G. Mathez5, A. Mazure1, B. Meneux1, R. Merighi3, R. Pellò5, A. Pollo10, L. Pozzetti3, M. Radovich12, E. Zucca3, M. Arnaboldi12, M. Bondi2, A. Bongiorno6, G. Busarello12, P. Ciliegi3, L. Gregorini2, Y. Mellier7, 11, P. Merluzzi12, V. Ripepi12 and D. Rizzo5
1 Laboratoire d'Astrophysique de Marseille - UMR 6110, OAMP, Université de Provence, Traverse du Siphon-Les trois Lucs, BP 8, 13376 Marseille Cedex 12, France
e-mail: olivier.lefevre@oamp.fr
2 IRA-INAF, via Gobetti 101, 40129 Bologna, Italy
3 INAF - Osservatorio Astronomico di Bologna, via Ranzani 1, 40127 Bologna, Italy
4 IASF-INAF, via Bassini 15, 20133 Milano, Italy
5 Laboratoire d'Astrophysique de l'Observatoire Midi-Pyrénées - UMR 5572, 14 avenue E. Belin, 31400 Toulouse, France
6 Università di Bologna, Dipartimento di Astronomia, via Ranzani 1, 40127 Bologna, Italy
7 Institut d'Astrophysique de Paris - UMR 7095, 98bis bd Arago, 75014 Paris, France
8 Max Planck Institut für Astrophysik, Karl-Schwarzschild-Strasse 1, 85741 Garching, Germany
9 European Southern Observatory, Karl-Schwarzschild-Strasse 2, 85748 Garching, Germany
10 INAF - Osservatorio Astronomico di Brera, via Brera 28, 20121 Milano, Italy
11 Observatoire de Paris, LERMA - UMR 8112, 61 avenue de l'Observatoire, 75014 Paris, France
12 INAF - Osservatorio Astronomico di Capodimonte, Salita Moiariello 16, 80131 Napoli, Italy
(Received 10 April 2004 / Accepted 6 August 2004)
Abstract
This paper presents the VIMOS VLT Deep Survey
around the Chandra Deep Field South (CDFS). We have measured
1599 new redshifts with VIMOS on the European Observatory
Very Large Telescope - UT3,
in an area
arcmin
2, including 784
redshifts in the Hubble Space Telescope - Advanced Camera
for Surveys GOODS area. 30% of all objects with
IAB=24
have been observed independently of magnitude, indicating
that the sample is purely
magnitude limited. We have reached
an unprecedented completeness level of 84% in terms of
the ratio of secure measurements vs. observed objects,
while 95% of all objects have a redshift measurement.
A total of 1452 galaxies, 139 stars, 8 QSOs have a
redshift identification, 141 of these being unsecure
measurements. The redshift distribution down to
IAB=24
is peaked at a median redshift
z=0.73, with a significant
high redshift tail extending up to ~4. Several high
density peaks in the distribution of galaxies are
identified. In particular, the strong peak at
z=0.735
contains more than 130 galaxies in a velocity range
km s
-1 distributed all across the transverse
~20
h-1 Mpc of the survey. We are releasing all redshifts
to the community, along with the cross identification
with HST-ACS GOODS sources on the CENCOS database environment
http://cencosw.oamp.fr.
Key words: surveys -- galaxies: high-redshift -- galaxies: distances and redshifts -- cosmology: observations -- galaxies: evolution -- cosmology: large scale structure of Universe
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© ESO 2004



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