All Tables

Table 1: Description of the 8 VVDS samples defined in the redshift range z=[0.5-1.2]
Table 2: Mean fraction of galaxies in the redshift range z=[0.5-1.2] for which $17.5\le I_{AB}\le 24$ among 40 mocks catalogues (serie S1) which are complete in stellar mass down to $10^9~M_\odot$ , built from the Millennium simulation with semi-analytical model of De Lucia & Blaizot (2007)
Table 3: Average systematic underestimate of the clustering length r₀ and the slope $\gamma$ of the correlation function introduced by the mass incompleteness. The values are computed for each parameter as $\epsilon(x)~=~\langle\delta x~/~x\rangle_{40}$ , where $\delta(x)~=~x_{\rm true}-x_{\rm observed}$ and the average is performed over 40 mock samples.
Table 4: Clustering length and slope of the correlation function $w_{\rm p}(r_{\rm p})$ for the different samples in the redshift range z=[0.5-1.2]. Values are derived for $0.2\le r_{\rm p}\le 21~h^{-1}$ Mpc. Associated errors have been extrapolated from the variance measured among 40 mocks catalogues for each stellar mass range. Values have not been corrected by underestimate due to stellar mass incompleteness.
Table 5: Measured values of the linear bias for the VVDS and SDSS samples, within 3 stellar mass ranges (see text).