\begin{table}%t7 \caption {\label{t5}Summary of the performance of the SVM regression models for predicting the input APs of the galaxy models.} %\centerline { \small \begin{tabular}{l c c c} \hline\hline Astrophysical parameter & mean(real-predicted)/mean(real) & sd(real-predicted)/mean(real) & SVs \\ \hline & Early-type galaxies & & \\ $p_{1}$ & --0.008 & 0.250 & 674 \\ $p_{2}$ & --0.001 & 0.076 & 646 \\ \hline & Spiral galaxies & & \\ $p_{1}$ & 0.018 & 0.384 & 2440 \\ $p_{2}$ & 0.010 & 0.451 & 1866 \\ infall timescale & 0.009 & 0.234 & 1786 \\ \hline & Irregular galaxies & & \\ $p_{1}$ & 0.004 & 0.174 & 647 \\ $p_{2}$ & 0.030 & 0.519 & 736 \\ infall timescale & 0.089 & 0.393 & 655 \\ \hline & Quenched star-forming galaxies & & \\ $p_{1}$ & 0.014 & 0.195 & 3116 \\ $p_{2}$ & 0.044 & 0.479 & 3127 \\ $p_{3}$ & 0.003 & 0.335 & 3077 \\ infall timescale & 0.038 & 0.524 & 3466 \\ \hline \end{tabular}} \par \medskip {\small \textsc{note.} The sample is for zero redshift and interstellar extinction ($A_{\rm v}$). The second and third columns list the mean and rms errors, respectively. The final column gives the number of support vectors in the SVM model.} \end{table}