activity
19992026
most citedThe Galaxy Mass Function up to z=4 in the GOODS-MUSIC sample: into the epoch of formation of massive galaxies

415 citations · 2.2k across the 193 of their papers we have counts for

collaborators
Showing 2005 · astro-phShow all

6 papers · 2 filters

astro-ph2005

Dynamical and chemical evolution of NGC1569

S. Recchi, G. Hensler, L. Angeretti +1

Blue Compact Dwarf and Dwarf Irregular galaxies are generally believed to be unevolved objects, due to their blue colors, compact appearance and large gas fractions. Many of these…

astro-ph2005

Sulphur abundance in Galactic stars

E. Caffau, P. Bonifacio, R. Faraggiana +3

We investigate sulphur abundance in 74 Galactic stars by using high resolution spectra obtained at ESO VLT and NTT telescopes. For the first time the abundances are derived, where…

astro-ph2005

The metal abundance distribution of the oldest stellar component in the Sculptor dwarf spheroidal galaxy

G. Clementini, V. Ripepi, A. Bragaglia +3

(abridged): Low resolution spectroscopy obtained with FORS2 at the Very Large Telescope (VLT) has been used to measure individual metal abundances ([Fe/H]) for 107 RR Lyrae stars,…

astro-ph2005

A Supernova Factory in Mrk 273?

M. Bondi, M-A. Perez-Torres, D. Dallacasa +1

We report on 1.6 and 5.0 GHz observations of the ultraluminous infrared galaxy (ULIRG) Mrk 273, using the European VLBI Network (EVN) and the Multi-Element Radio-Linked Interferome…

astro-ph2005★ 2 cited

Cryogenic Filters for RFI Mitigation in Radioastronomy

G. Tuccari, A. Caddemi, S. Barbarino +4

RFI mitigation in Radioastronomy can be achieved adopting cryogenic filters in appropriate typologies. A study has been conducted in L, C and X band with the evaluation of the filt…

astro-ph2005

The s-process weak component: uncertainties due to convective overshooting

Vincenzo Costa, Maria Letizia Pumo, Alfio Bonanno +1

Using a new s-nucleosynthesis code, coupled with the stellar evolution code Star2003, we performed simulations to study the impact of the convection treatment on the s-process duri…