\begin{table}%t4 \caption{\label{synthphot}Intrinsic color indices at quadrature computed by synthetic photometry.} %\centering \par \begin{tabular}{c c c } \hline\hline \noalign{\smallskip} Object & $(B-V)_0^{\rm q}$ & $(V-I)_0^{\rm q}$ \\ & (mag) & (mag) \\ \hline 4 110409 & $-0.243\pm 0.006$& $-0.252\pm 0.007$ \\ 4 113853 & $-0.196\pm 0.007$& $-0.206\pm 0.008$ \\ 4 117831 & $-0.179\pm 0.004$& $-0.192\pm 0.004$ \\ 4 121084 & $-0.271\pm 0.004$& $-0.294\pm 0.004$ \\ 4 121110 & $-0.248\pm 0.006$& $-0.269\pm 0.006$ \\ 4 121461 & $-0.207\pm 0.007$& $-0.228\pm 0.008$ \\ 4 159928 & $-0.247\pm 0.006$& $-0.263\pm 0.007$ \\ 4 160094 & $-0.238\pm 0.009$& $-0.260\pm 0.009$ \\ 4 163552 & $-0.232\pm 0.008$& $-0.246\pm 0.009$ \\ 4 175149 & $-0.271\pm 0.002$& $-0.288\pm 0.002$ \\ 4 175333 & $-0.191\pm 0.006$& $-0.211\pm 0.007$ \\ 5 016658 & $-0.203\pm 0.005$& $-0.218\pm 0.005$ \\ 5 026631 & $-0.242\pm 0.003$& $-0.257\pm 0.003$ \\ 5 032412 & $-0.283\pm 0.001$& $-0.303\pm 0.001$ \\ 5 038089 & $-0.273\pm 0.001$& $-0.292\pm 0.001$ \\ 5 095337 & $-0.242\pm 0.009$& $-0.261\pm 0.010$ \\ 5 095557 & $-0.216\pm 0.003$& $-0.233\pm 0.003$ \\ 5 100485 & $-0.215\pm 0.004$& $-0.232\pm 0.005$ \\ 5 100731 & $-0.217\pm 0.004$& $-0.233\pm 0.004$ \\ 5 106039 & $-0.204\pm 0.003$& $-0.210\pm 0.003$ \\ 5 111649 & $-0.169\pm 0.002$& $-0.168\pm 0.002$ \\ 5 123390 & $-0.254\pm 0.004$& $-0.274\pm 0.004$ \\ 5 180185 & $-0.182\pm 0.004$& $-0.188\pm 0.005$ \\ 5 180576 & $-0.221\pm 0.009$& $-0.237\pm 0.010$ \\ 5 185408 & $-0.222\pm 0.004$& $-0.239\pm 0.004$ \\ 5 196565 & $-0.200\pm 0.003$& $-0.209\pm 0.004$ \\ 5 261267 & $-0.253\pm 0.006$& $-0.266\pm 0.007$ \\ 5 265970 & $-0.214\pm 0.001$& $-0.226\pm 0.001$ \\ 5 266015 & $-0.265\pm 0.004$& $-0.280\pm 0.004$ \\ 5 266131 & $-0.239\pm 0.006$& $-0.258\pm 0.007$ \\ 5 266513 & $-0.194\pm 0.011$& $-0.208\pm 0.012$ \\ 5 277080 & $-0.244\pm 0.004$& $-0.256\pm 0.004$ \\ 5 283079 & $-0.234\pm 0.004$& $-0.252\pm 0.004$ \\ \hline \end{tabular} \tablefoot {Because the wavelength range provided in the OSTAR2002 grid is too short, $(V-I)_0$~values of systems with a component hotter than $30~000$~K were computed using Kurucz red fluxes (see~text).} \end{table}