Table 2: Galaxy contamination of the D1 field cross-identified with the VVDS field as a function of i' magnitude and r'-i' colour. The common area is $\sim$ 0.4 sq degree.
r'-i' i' < 20.0 i'< 21.0 i' < 22.0

total $3.2\% \pm 1.8$ $6.7\% \pm 1.9$ $13.1\% \pm 2.3$

<0.5 $3.2\% \pm 3.2$ $13.0\% \pm 4.3$ $23.5\% \pm 4.9$

>0.5 $3.1\% \pm 2.2$ $2.7\% \pm 1.5$ $6.5\% \pm 2.1$

>1.4 0% 0% $1.8\%\pm 1.8$

**Table 2:** Galaxy contamination of the D1 field cross-identified with the VVDS field as a function of i' magnitude and r'-i' colour. The common area is $\sim$ 0.4 sq degree.
r'-i'	i' < 20.0	i'< 21.0	i' < 22.0
total	$3.2\% \pm 1.8$	$6.7\% \pm 1.9$	$13.1\% \pm 2.3$
<0.5	$3.2\% \pm 3.2$	$13.0\% \pm 4.3$	$23.5\% \pm 4.9$
>0.5	$3.1\% \pm 2.2$	$2.7\% \pm 1.5$	$6.5\% \pm 2.1$
>1.4	0%	0%	$1.8\%\pm 1.8$

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