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Physical properties of galaxies and their evolution in the VIMOS VLT Deep Survey. I. The evolution of the mass-metallicity relation up to z~0.9
F. Lamareille, J. Brinchmann, T. Contini +43
We derive the mass-metallicity relation of star-forming galaxies up to , using data from the VIMOS VLT Deep Survey. Automatic measurement of emission-line fluxes and equi…
A weak lensing analysis of the Abell 2163 cluster
M. Radovich, E. Puddu, A. Romano +2
Weak lensing analysis is applied to a deep, one square degree r-band CFHT-Megacam image of the Abell 2163 field. The observed shear is fitted with Single Isothermal Sphere and Nava…
Rigorous luminosity function determination in presence of a background: theory and application to two intermediate redshift clusters
S. Andreon, G. Punzi, A. Grado
In this paper we present a rigorous derivation of the luminosity function (LF) in presence of a background. Our approach is free from the logical contradictions of assigning negati…
The Capodimonte Deep Field I - Presentation of the survey and first follow-up studies
J. M. Alcalá, M. Pannella, E. Puddu +16
We present the Capodimonte Deep Field (OACDF), a deep field covering an area of 0.5 square degrees in the B, V, R optical bands plus six medium-band filters in the wavelength range…
Data reduction and astrometry strategies for wide-field images: an application to the Capodimonte Deep Field
J. M. Alcala', M. Radovich, R. Silvotti +4
The Capodimonte Deep Field (OACDF) is a multi-colour imaging survey on two 0.5x0.5 square degree fields performed in the BVRI bands and in six medium-band filters (700 - 900 nm) wi…