Table 2: Constraints on dark matter halos of galaxies modelled by NFW profiles for different lens samples and $r_{\rm max}=400h^{-1}~{\rm kpc}$. $N_{\rm d}$, $N_{\rm s}$ and $N_{\rm p}$ are the numbers of lenses, sources and pairs in each measurement. These numbers differ from those given in Table 1 because of the larger $r_{\rm max}$ used here. The virial radius $r_{\rm vir}^*$ and $\alpha $ are fitted quantities (see Fig. 4), the virial mass $M_{\rm vir}^*$ and the virial mass-to-light ratio $M_{\rm vir}^*/L^*$ are calculated from $r_{\rm vir}^*$. $\beta =3\alpha -1$ gives the scaling of $M_{\rm vir}/L$ with luminosity, $M_{\rm vir}/L\propto L^\beta $. All errors are 1-$\sigma $.

Lenses		 $N_{\rm d}$ $N_{\rm s}$ $N_{\rm p}$ $r_{\rm vir}^*$ $\alpha $ $\log(h\frac{M_{\rm vir}}{M_{\odot}})$ $M_{\rm vir}^*/L^*$ $\beta$
        [ $h^{-1}~{\rm kpc}$]     [ $h(M/L)_{\odot}$]  

all		 11 311 13 956 566 466 209+24-32 0.34+0.12-0.16 11.8+0.1-0.3 64+25-33 0.02+0.36-0.48
blue 9181 13 936 451 420 177+40-48 0.18+0.20-0.12 11.6+0.3-0.4 39+33-24 -0.46+0.60-0.36
red 2130 13 603 115 046 217+56-48 0.42+0.16-0.20 11.9+0.3-0.3 71+71-38 0.26+0.48-0.60


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