activity
20042015
most citedThe VIMOS Public Extragalactic Redshift Survey (VIPERS). An unprecedented view of galaxies and large-scale structure at 0.5<z<1.2

350 citations · 2.5k across the 34 of their papers we have counts for

collaborators
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6 papers · 1 filter

astro-ph2008★ 162 cited

The Vimos VLT Deep Survey: Global properties of 20000 galaxies in the I_AB<=22.5 WIDE survey

B. Garilli, O. Le Fèvre, L. Guzzo +44

The VVDS-Wide survey has been designed with the general aim of tracing the large-scale distribution of galaxies at z~1 on comoving scales reaching ~100Mpc/h, while providing a good…

astro-ph2008★ 3 cited

GOSSIP, a new VO compliant tool for SED fitting

P. Franzetti, M. Scodeggio, B. Garilli +2

We present GOSSIP (Galaxy Observed-Simulated SED Interactive Program), a new tool developed to perform SED fitting in a simple, user friendly and efficient way. GOSSIP automaticall…

astro-ph2007★ 70 cited

The XMM-LSS catalogue: X-ray sources and associated optical data. Version I

M. Pierre, L. Chiappetti, F. Pacaud +34

Following the presentation of the XMM-LSS X-ray source detection package by Pacaud et al., we provide the source lists for the first 5.5 surveyed square degrees. The catalogues per…

astro-ph2005★ 77 cited

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…

astro-ph2005★ 54 cited

The XMM-LSS survey: The XMDS/VVDS 4 sigma catalogue

L. Chiappetti, M. Tajer, G. Trinchieri +15

We present a first catalogue of X-ray sources resulting from the central area of the XMM-LSS (Large Scale Structure survey). We describe the reduction procedures and the database t…

astro-ph2004

Data Reduction and Analysis Graphical Organizer

L. Paioro, B. M. Garilli, M. Scodeggio +1

Spectroscopic surveys are undergoing a rapid expansion in their data collecting capabilities, reaching the level of hundreds of spectra per pointing. An efficient use of such huge…