The VIMOS VLT Deep Survey - First epoch VVDS-Deep survey: 11564 spectra with 17.5<=IAB<=24, and the redshift distribution over 0< z <=5

Abstract

This paper presents the ``First Epoch'' sample from the VIMOS VLT Deep Survey (VVDS). The VVDS goals, observations, data reduction with VIPGI, and redshift measurement with KBRED are discussed. Data have been obtained with the VIsible Multi Object Spectrograph (VIMOS) on the ESO-VLT UT3, allowing to observe ~600 slits simultaneously at R~230. A total of 11564 objects have been observed in the VVDS-02h and VVDS-CDFS Deep fields over a total area of 0.61deg^2, selected solely on the basis of apparent magnitude 17.5 <=I_{AB} <=24. The VVDS covers the redshift range 0 < z <= 5. It is successfully going through the ``redshift desert'' 1.5<z<2.2, while the range 2.2<z<2.7 remains of difficult access because of the VVDS wavelength coverage.A total of 9677 galaxies have a redshift measurement, 836 are stars, 90 are AGNs, and a redshift could not be measured for 961 objects. There are 1065 galaxies with a measured redshift z>1.4. The survey reaches a redshift measurement completeness of 78% overall (93% including less reliable objects), with a spatial sampling of the population of galaxies of 25% and ~30% in the VVDS-02h and VVDS-CDFS. The redshift accuracy measured from repeated observations with VIMOS and comparison to other surveys is ~276km/s. From this sample we present for the first time the redshift distribution of a magnitude limited spectroscopic sample down to IAB=24. The redshift distribution has a median of z=0.62, z=0.65, z=0.70, and z=0.76, for magnitude limited samples with IAB<=22.5, 23, 23.5, and 24. A high redshift tail above redshift 2 and up to redshift 5 becomes readily apparent for IAB>23.5, probing the bright star forming population of galaxies. This sample provides an unprecedented dataset to study galaxy evolution over 90% of the life of the universe

30 pages, accepted 22-Feb-05 in A&A

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• Photo-z Quality Cuts and their Effect on the Measured Galaxy Clustering
• COLDz: Karl G. Jansky Very Large Array discovery of a gas-rich galaxy in COSMOS
• The Grism Lens-Amplified Survey from Space (GLASS). XIII. G800L optical spectra from the parallel fields
• HerMES: Disentangling active galactic nuclei and star formation in the radio source population
• Optimizing high redshift galaxy surveys for environmental information
• PRIMUS: The Effect of Physical Scale on the Luminosity-Dependence of Galaxy Clustering via Cross-Correlations
• Optimising Spectroscopic and Photometric Galaxy Surveys: Efficient Target Selection and Survey Strategy
• Stellar properties of z ~ 1 Lyman-break galaxies from ACS slitless grism spectra
• Astrophysics in 2005
• The VIMOS Public Extragalactic Redshift Survey (VIPERS): PCA-based automatic cleaning and reconstruction of survey spectra
• Spitzer's View of the Candidate Cluster and Protocluster Catalog (CCPC)
• The many flavours of photometric redshifts
• Searching for low-redshift faint galaxies with MMT/Hectospec
• A Generalized Method for Measuring Weak Lensing Magnification With Weighted Number Counts
• Variability and transient search in the SUDARE-VOICE field: a new method to extract the light curves
• The Metallicity Distribution of Distant F and G type stars in the CFHT Legacy Survey Deep Field
• Evolution of the real-space correlation function from next generation cluster surveys
• Sky surveys and deep fields of ground-based and space telescopes
• Integral field spectroscopy with SINFONI of VVDS galaxies. I. Galaxy dynamics and mass assembly at 1.2 < z < 1.6
• Learn from every mistake! Hierarchical information combination in astronomy
• 3D spectroscopic surveys: Exploring galaxy evolution mechanisms
• Panchromatic properties of galaxies in wide-field optical spectroscopic and photometric surveys
• The VIMOS VLT Deep Survey. The different assembly history of passive and star-forming L_B >= L*_B galaxies in the group environment at z < 1
• The intriguing life of star-forming galaxies in the redshift range 1 < z < 2 using MASSIV
• Integral field spectroscopy with SINFONI of VVDS galaxies. II. The mass-metallicity relation at 1.2 < z < 1.6