**Table 1:** $D_{\rm n}$ 4000 median distribution.
	$\rm 10^{9{-}9.5}$ $M_\odot$	$\rm 10^{9.5{-}10}$ $M_\odot$	$\rm 10^{10{-}10.5}$ $M_\odot$	$\rm 10^{{10.5{-}11}}$ $M_\odot$	10^>11 $M_\odot$
z
$\sim$ 0	$1.24 \pm0.00$	$1.28 \pm0.00$	$1.46 \pm0.00$	$1.66 \pm0.00$	$1.81\pm0.00$
0.5-0.7	$1.18 \pm0.01$	$1.20 \pm0.01$	$1.27 \pm0.01$	$1.50 \pm0.02$	$1.69\pm0.02$
0.7-1.0	$1.13 \pm0.01$	$1.16 \pm0.01$	$1.21 \pm0.01$	$1.31 \pm0.01$	$1.55\pm0.02$
1.0-1.3	$1.07 \pm0.04$	$1.07 \pm0.02$	$1.09 \pm0.01$	$1.20 \pm0.02$	$1.37\pm0.02$

Notes: $D_{\rm n}$ 4000 median values in five intervals of stellar mass and three redshift bins for our VVDS-F02 sample. The error quoted in each interval represents the error on the median distribution using a statistical Jackknife technique. The median values of the $D_{\rm n}$ 4000 distribution in a nearby galaxy sample (SDSS DR4) are also listed.

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