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19972026
most citedAccurate photometric redshifts for the CFHT Legacy Survey calibrated using the VIMOS VLT Deep Survey

1.7k citations · 15.4k across the 225 of their papers we have counts for

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Showing 2004Show all

13 papers · 1 filter

astro-ph2004★ 325 cited

The GALEX-VVDS Measurement of the Evolution of the Far-Ultraviolet Luminosity Density and the Cosmic Star Formation Rate

D. Schiminovich, O. Ilbert, S. Arnouts +10

In a companion paper (Arnouts et al. 2004) we presented new measurements of the galaxy luminosity function at 1500 Angstroms out to z~1 using GALEX-VVDS observations (1039 galaxies…

astro-ph2004★ 217 cited

The GALEX-VVDS Measurement of the Evolution of the 1500A Luminosity Function

S. Arnouts, D. Schiminovich, O. Ilbert +8

We present the first measurement of the galaxy luminosity function at 1500A between 0.2<z<1.2 based on GALEX-VVDS observations (1000 spectroscopic redshifts for galaxies with NUV<2…

astro-ph2004

A Virgo high-resolution Halpha kinematical survey

L. Chemin, C. Balkowski, V. Cayatte +9

We have completed a survey of 30 Virgo cluster galaxies in the Halpha emission-line using Fabry-Perot interferometry. The goal of the survey is to obtain a high angular resolution…

astro-ph2004

The VLT-VIMOS Mask Preparation Software

D. Bottini, B. Garilli, D. Maccagni +34

VIMOS (VIsible Multi-Object Spectrograph) is a multi-object imaging spectrograph installed at the VLT (Very large Telescope) at the ESO (European Southern Observatory) Paranal Obse…

astro-ph2004★ 191 cited

The VVDS data reduction pipeline: introducing VIPGI, the VIMOS Interactive Pipeline and Graphical Interface

M. Scodeggio, P. Franzetti, B. Garilli +36

The VIMOS VLT Deep Survey (VVDS), designed to measure 150,000 galaxy redshifts, requires a dedicated data reduction and analysis pipeline to process in a timely fashion the large a…

astro-ph2004★ 63 cited

Large scale diffuse light in the Coma cluster: a multi-scale approach

C. Adami, E. Slezak, F. Durret +7

We have obtained wide field images of the Coma cluster in the B, V, R and I bands with the CFH12K camera at CFHT. In order to search for large scale diffuse emission, we have appli…