All Figures

$\begin{figure} \par\includegraphics[width=7.3cm,clip]{1962fig1.ps} \end{figure}$ Figure 1: The redshift distribution in the VVDS-02h field. The filled histogram contains 6137 galaxies with quality flag $\geq$ 2, and another 1093 galaxies with quality $\rm flag =1$ (open dashed histogram), in the redshift range z=[0.2, 2.1].
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In the text

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{1962fig2.ps} \end{figure}$ Figure 2: The rest frame B-I_AB color ( left) and absolute magnitude M_{B_AB} ( right) from the VVDS-02h data up to $z\sim 2$ .
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In the text

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{1962fig3.ps} \end{figure}$ Figure 3: The correlation function from the VVDS-02h data up to ${z\simeq 2}$ : ( left) ${w}{_{\rm p}}({r}{_{\rm p}})$ measured in 6 redshift bins, the number of galaxies in each bin is indicated on the top right of each panel, ( right) the correlation length r₀(z) and correlation function slope $\gamma$ measured from fitting ${w}{_{\rm p}}({r}{_{\rm p}})$ assuming a power law form $\xi (r) = (r/r_0)^{-\gamma }$ . 68%, 90% and 95% likelihood contours are drawn.
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In the text

$\begin{figure} \par\includegraphics[width=8cm,clip]{1962fig4.ps} \end{figure}$ Figure 4: The correlation function ${w}{_{\rm p}}({r}{_{\rm p}})$ for the VVDS-CDFS data in three redshift bins from z=0.4 to to z=1.5. The slope has been fixed to $\gamma =1.72$ , i.e. the mean measured in the VVDS-02h field in the range z=[0.2, 1.1].
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In the text

$\begin{figure} \par\includegraphics[width=8.3cm,clip]{1962fig5.ps} \end{figure}$ Figure 5: Correlation function computed from the VVDS sample, applying the same color-magnitude selection function as for the DEEP2 survey (Coil et al. 2004): ( bottom) the full sample in the redshift range [0.7, 1.35], ( top two panels) the lower [0.7, 0.9] and higher [0.9, 1.35] redshift samples. The slope has been fixed to the same slope as measured in the DEEP2 to ease r₀ comparison.
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In the text

$\begin{figure} \par\includegraphics[width=8.2cm,clip]{1962fig6.ps} \end{figure}$ Figure 6: Comparison of the correlation length r₀(z) (comoving) measured in the VVDS-Deep survey applying a color-color and magnitude selection as in the DEEP2 survey, and the DEEP2 survey measurements (Coil et al. 2004): VVDS-02h, with $\gamma =1.66$ fixed to the DEEP2 value: filled circles; r₀ and $\gamma$ fitted simultaneously: open-dot circles, DEEP2 measurements: open stars. Data points have been shifted slightly along the redshift axis to avoid overlap.
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In the text

$\begin{figure} \par\includegraphics[width=8.5cm,clip]{1962fig7.ps} \end{figure}$ Figure 7: Evolution of the correlation length r₀(z) (comoving) from the VVDS. Black circles are for the VVDS-02h data, open squares are for the VVDS-CDFS data. The doted points indicate the measurements when setting the slope to the mean $\gamma =1.76$ measured in the range z=[0.2, 1.3]. Associated errors have been computed from the fitting of ${w}{_{\rm p}}({r}{_{\rm p}})$ and associated errors drived from 50 mock galaxy samples from Galics (see text). The VVDS-CDFS measurements are slightly higher than in the VVDS-02h, but remain compatible within the measurement errors. The VVDS-CDFS measurement at z=0.7 include a strong over-density of more than 130 galaxies (see Le Fèvre et al. 2004b), making the correlation function higher in this bin.
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In the text

$\begin{figure} \par\includegraphics[width=7.3cm,clip]{1962fig1.ps} \end{figure}$	Figure 1: The redshift distribution in the VVDS-02h field. The filled histogram contains 6137 galaxies with quality flag $\geq$ 2, and another 1093 galaxies with quality $\rm flag =1$ (open dashed histogram), in the redshift range z=[0.2, 2.1].
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$\begin{figure} \par\includegraphics[width=8.8cm,clip]{1962fig2.ps} \end{figure}$	Figure 2: The rest frame B-I_AB color ( left) and absolute magnitude M_{B_AB} ( right) from the VVDS-02h data up to $z\sim 2$ .
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$\begin{figure} \par\includegraphics[width=8cm,clip]{1962fig4.ps} \end{figure}$	Figure 4: The correlation function ${w}{_{\rm p}}({r}{_{\rm p}})$ for the VVDS-CDFS data in three redshift bins from z=0.4 to to z=1.5. The slope has been fixed to $\gamma =1.72$ , i.e. the mean measured in the VVDS-02h field in the range z=[0.2, 1.1].
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