2k citations · 28.1k across the 323 of their papers we have counts for
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The VIMOS-VLT Deep Survey: Luminosity dependence of clustering at z~1
A. Pollo, L. Guzzo, O. Le Fevre +2
We investigate the dependence of galaxy clustering on the galaxy intrinsic luminosity at high redshift, using the data from the First Epoch VIMOS-VLT Deep Survey (VVDS). The size (…
The VIMOS-VLT Deep Survey - The evolution of galaxy clustering per spectral type to z~1.5
B. Meneux, O. LeFevre, L. Guzzo +47
We measure the evolution of clustering for galaxies with different spectral types from 6495 galaxies with 17.5<=I_AB<=24 and measured spectroscopic redshift in the first epoch VIMO…
A large population of galaxies 9 to 12 billion years back in the history of the Universe
O. Le Fevre, S. Paltani, S. Arnouts +6
To understand the evolution of galaxies, we need to know as accurately as possible how many galaxies were present in the Universe at different epochs. Galaxies in the young Univers…
The VIMOS Integral Field Unit: data reduction methods and quality assessment
A. Zanichelli, B. Garilli, M. Scodeggio +38
With new generation spectrographs integral field spectroscopy is becoming a widely used observational technique. The Integral Field Unit of the VIsible Multi-Object Spectrograph on…
The Vimos VLT Deep Survey: Compact structures in the CDFS
C. Adami, A. Mazure, O. Ilbert +2
We have used the Vimos VLT Deep Survey in combination with other spectroscopic, photometric and X-ray surveys from literature to detect several galaxy structures in the Chandra Dee…
The VIRMOS deep imaging survey IV: Near-infrared observations
A. Iovino, H. J. McCracken, B. Garilli +49
In this paper we present a new deep, wide-field near-infrared imaging survey. Our J- and K-band observations in four separate fields complement optical BVRI, ultraviolet and spectr…
The VVDS-VLA Deep Field II. Optical and near infrared identifications of VLA S(1.4GHz)>80 microJy sources in the VIMOS VLT Deep Survey VVDS-02h field
P. Ciliegi, G. Zamorani, M. Bondi +46
In this paper we present the optical and near-infrared identifications of the 1054 radio sources detected in the 20cm deep radio survey down to a 5sigma flux limit of about 80 micr…
The VIMOS VLT Deep Survey: Evolution of the non-linear galaxy bias up to z=1.5
C. Marinoni, O. Le Fevre, B. Meneux +44
We present the first measurements of the Probability Distribution Function (PDF) of galaxy fluctuations in the VIMOS-VLT Deep Survey (VVDS) cone, covering 0.4x0.4 deg between 0.4<z…
The VIMOS VLT Deep Survey - Evolution of the luminosity functions by galaxy type up to z=1.5 from first epoch data
E. Zucca, O. Ilbert, S. Bardelli +47
From the first epoch observations of the VVDS up to z=1.5 we have derived luminosity functions (LF) of different spectral type galaxies. The VVDS data, covering ~70% of the life of…