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Comparison of the VIMOS-VLT Deep Survey with the Munich semi-analytical model - I. Magnitude counts, redshift distribution, colour bimodality, and galaxy clustering
S. de la Torre, B. Meneux, G. De Lucia +37
This paper presents a detailed comparison between high-redshift observations from the VIMOS-VLT Deep Survey (VVDS) and predictions from the Munich semi-analytical model of galaxy f…
The bimodality of the 10k zCOSMOS-bright galaxies up to z ~ 1: a new statistical and portable classification based on the optical galaxy properties
G. Coppa, M. Mignoli, G. Zamorani +56
Our goal is to develop a new and reliable statistical method to classify galaxies from large surveys. We probe the reliability of the method by comparing it with a three-dimensiona…
The zCOSMOS 10k-sample: the role of galaxy stellar mass in the colour-density relation up to z=1
O. Cucciati, A. Iovino, K. Kovac +53
[Abridged] With the first 10000 spectra of the flux limited zCOSMOS sample (I<=22.5) we study the evolution of environmental effects on galaxy properties since z=1.0, and disentang…
Understanding the shape of the galaxy two-point correlation function at z~1 in the COSMOS field
S. de la Torre, L. Guzzo, K. Kovac +59
We investigate how the shape of the galaxy two-point correlation function as measured in the zCOSMOS survey depends on local environment, quantified in terms of the density contras…
The XMM-Newton Wide-Field Survey in the COSMOS field (XMM-COSMOS): demography and multiwavelength properties of obscured and unobscured luminous AGN
M. Brusa, F. Civano, A. Comastri +64
We report the final optical identifications of the medium-depth (~60 ksec), contiguous (2 deg^2) XMM-Newton survey of the COSMOS field. XMM-Newton has detected ~800 X-ray sources d…
The VIMOS-VLT Deep Survey: Evolution in the Halo Occupation Number since z 1
U. Abbas, S. de la Torre, O. Le Fèvre +47
We model the evolution of the mean galaxy occupation of dark-matter halos over the range , using the data from the VIMOS-VLT Deep Survey (VVDS). The galaxy projected cor…