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The B-Band Luminosity Function of Red and Blue Galaxies up to z=3.5
E. Giallongo, S. Salimbeni, N. Menci +5
We have explored the redshift evolution of the luminosity function of red and blue galaxies up to . This was possible joining a deep I band composite galaxy sample, which in…
Obscured AGN and the X-ray, Optical and Far-Infrared Number Counts of AGN in the GOODS Fields
E. Treister, C. M. Urry, E. Chatzichristou +12
The deep X-ray, optical, and far-infrared fields that constitute GOODS are sensitive to obscured AGN (N_H>10^{22} cm^{-2}) at the quasar epoch (z~2-3), as well as to unobscured AGN…
Old Galaxies in the Young Universe
A. Cimatti, E. Daddi, A. Renzini +8
More than half of all stars in the local Universe are found in massive spheroidal galaxies, which are characterized by old stellar populations with little or no current star format…
The Great Observatories Origins Deep Survey - VLT/FORS2 Spectroscopy in the GOODS-South Field
E. Vanzella, S. Cristiani, M. Dickinson +14
We present the first results of the ESO/GOODS program of spectroscopy of faint galaxies in the Chandra Deep Field South (CDF-S). 399 spectra of 303 unique targets have been obtaine…
The Lyman-alpha forest according to LUQAS
M. Viel, M. Haehnelt, T. -S. Kim +6
We use the LUQAS sample of 27 high resolution, high signal-to-noise QSO absorption spectra (Kim et al. 2004) and the results from Croft et al. (2002) together with a suite of high-…
The K20 survey. VI. The Distribution of the Stellar Masses in Galaxies up to z~2
A. Fontana, L. Pozzetti, I. Donnarumma +14
We present a detailed analysis of the stellar mass content of galaxies up to z=2.5 in the K20 galaxy sample, that has a 92% spectroscopic completeness and a complete m…