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

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

doi:10.1051/0004-6361:20041960

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arXiv · astro-ph/0409133

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

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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 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

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O. Le Fevre, G. Vettolani, B. Garilli, L. Tresse, D. Bottini V. Le Brun, D. Maccagni, J. P. Picat, R. Scaramella, M. Scodeggio, A. Zanichelli, C. Adami, S. Bardelli, M. Bolzonella, A. Cappi, S. Charlot, T. Contini, S. Foucaud, P. Franzetti, I. Gavignaud, L. Guzzo, O. Ilbert, A. Iovino, H. J. McCracken, B. Marano, C. Marinoni, G. Mathez, A. Mazure, B. Meneux, R. Merighi, S. Paltani, R. Pellò, A. Pollo, L. Pozzetti, M. Radovich, G. Zamorani, E. Zucca, M. Bondi, A. Bongiorno, G. Busarello, P. Ciliegi, Y. Mellier, P. Merluzzi, V. Ripepi, D. Rizzo. 2005-07-02. 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. https://doi.org/10.1051/0004-6361%3A20041960

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