\begin{table}%t5 \caption{\label{tab:Mup}Mass-to-light ratios for selected ages in several photometric passbands from our {\em standard} model with different assumptions for~$M_{\rm up}$.} \small%\centering \par \begin{tabular}{lccccccc} \hline \hline & $M/L_V$ & $M/L_U$ & $M/L_B$ & $M/L_R$ & $M/L_I$ & $M/L_J$ & $M/L_K$\\ \hline $M_{\rm up}=5~M_{\odot}$ & & & & & & &\\ \hline $500~{\rm Myr}$ & $0.21 \pm 0.01$ & $0.126 \pm 0.003$ & $0.139 \pm 0.004$ & $0.25 \pm 0.02$ & $0.28 \pm 0.04$ & $0.28 \pm 0.06$ & $0.26 \pm 0.08$ \\ $800~{\rm Myr}$ &$ 0.28 \pm 0.02 $&$0.194 \pm 0.007 $&$0.210 \pm 0.008 $&$0.31 \pm 0.03 $&$0.31 \pm 0.04$&$0.29 \pm 0.05 $&$0.25 \pm 0.06 $\\ $3~{\rm Gyr}$ &$0.66 \pm 0.03 $&$0.55 \pm 0.01 $&$0.58 \pm 0.02 $&$0.67 \pm 0.03 $&$0.64 \pm 0.03$&$0.58 \pm 0.04 $&$0.50 \pm 0.04 $\\ $10~{\rm Gyr}$ &1.55$ \pm 0.04 $&$1.45 \pm 0.02 $&$1.58 \pm 0.03 $&$1.47 \pm 0.04 $&$1.33 \pm0.05 $&$1.15 \pm 0.05 $&$0.95 \pm 0.05 $\\ \hline $M_{\rm up}=6.5~M_{\odot}$ & & & & & & &\\ \hline $500~{\rm Myr}$ & 0.22 $\pm$ 0.01 & 0.127 $\pm$ 0.003 & 0.140 $\pm$ 0.004 & 0.26 $\pm$ 0.02 & 0.28 $\pm$ 0.03 & 0.29 $\pm$ 0.06 & 0.26 $\pm$ 0.08\\ $800~{\rm Myr}$ & 0.28 $\pm$ 0.01 & 0.191 $\pm$ 0.005 & 0.207 $\pm$ 0.006 & 0.30 $\pm$ 0.02 & 0.30 $\pm$ 0.03 & 0.28 $\pm$ 0.05 & 0.25 $\pm$ 0.06\\ $3~{\rm Gyr}$ & 0.66 $\pm$ 0.03 & 0.55 $\pm$ 0.01 & 0.58 $\pm$ 0.02 & 0.67 $\pm$ 0.03 & 0.64 $\pm$ 0.04 & 0.58 $\pm$ 0.04 & 0.49 $\pm$ 0.04\\ $10~{\rm Gyr}$ & 1.58 $\pm$ 0.05 & 1.47 $\pm$ 0.02 & 1.60 $\pm$ 0.03 & 1.49 $\pm$ 0.05 & 1.36 $\pm$ 0.06 & 1.17 $\pm$ 0.06 & 0.97 $\pm$ 0.06\\ \hline $M_{\rm up}=10~M_{\odot}$ & & & & & & &\\ \hline $500~{\rm Myr}$ &$0.22 \pm 0.01 $&$0.130 \pm 0.002 $&$0.143 \pm 0.003 $&$ 0.26 \pm 0.02 $&$0.28 \pm 0.04 $&$0.28 \pm 0.06 $&$0.26 \pm 0.08 $\\ $800~{\rm Myr}$ &$0.29 \pm 0.01 $&$0.199 \pm 0.005 $&$0.214 \pm 0.005 $&$ 0.31 \pm 0.02 $&$0.31 \pm 0.03 $&$0.29 \pm 0.05 $&$0.25 \pm 0.05 $\\ $3~{\rm Gyr}$ &$0.68 \pm 0.03 $&$0.56 \pm 0.01 $&$0.60 \pm 0.02 $&$ 0.69 \pm 0.04 $&$0.66 \pm 0.04 $&$ 0.60 \pm 0.04 $&$0.51 \pm 0.05 $\\ $10 ~{\rm Gyr}$ &$1.58 \pm 0.05 $&$1.48 \pm 0.02 $&$1.61 \pm 0.04 $&$1.49 \pm 0.06 $&$1.35 \pm 0.06 $&$1.16 \pm 0.06 $&$0.96 \pm 0.06 $\\ \hline \end{tabular} \end{table}