Tracking the impact of environment on the Galaxy Stellar Mass Function
  up to z~1 in the 10k zCOSMOS sample
  We study the impact of the environment on the evolution of galaxies in the
zCOSMOS 10k sample in the redshift range 0.1<z<1.0 over an area of ~1.5 deg2.
The considered sample of secure spectroscopic redshifts contains about 8500
galaxies, with their stellar masses estimated by SED fitting of the
multiwavelength optical to NIR photometry. The evolution of the galaxy stellar
mass function (GSMF) in high and low density regions provides a tool to study
the mass assembly evolution in different environments; moreover, the
contributions to the GSMF from different galaxy types, as defined by their SEDs
and their morphologies, can be quantified. At redshift z~1, the GSMF is only
slightly dependent on environment, but at lower redshifts the shapes of the
GSMFs in high- and low-density environments become extremely different, with
high density regions exhibiting a marked bimodality. As a result, we infer that
galaxy evolution depends on both the stellar mass and the environment, the
latter setting the probability of a galaxy to have a given mass: all the galaxy
properties related to the stellar mass show a dependence on environment,
reflecting the difference observed in the mass functions. The shapes of the
GSMFs of early- and late-type galaxies are almost identical for the extremes of
the density contrast we consider. The evolution toward z=0 of the mass at which
the early- and late-type GSMFs match each other is more rapid in high density
environments. The comparison of the observed GSMFs to the same quantities
derived from a set of mock catalogues shows that blue galaxies in sparse
environments are overproduced in the semi-analytical models at intermediate and
high masses, because of a deficit of star formation suppression, while at z<0.5
an excess of red galaxies is present in dense environments at intermediate and
low masses, because of the overquenching of satellites. ABRIDGED
