\begin{table}%ta.1 %\centering \par \caption{\label{ta:1}Solar-scaled metallicity models from the ZAMS until the 1$^{{\rm st}}$ TP. } \small \begin{tabular}{ccccccccccccccc} \hline\hline \multicolumn{6}{c}{$Z = 0.02$ / solar} & & & \multicolumn{7}{c}{$Z = 0.008$ / solar} \\ \hline\noalign{\smallskip} $M_{{\rm ZAMS}}$ & $t_{{\rm MS}}$$^a$ & $t_{{\rm RGB}}$ & $t_{{\rm He-b}}$ & $t_{{\rm EAGB}}$ & $M_{{\rm tot}}$(1)$^b$ & $M_{\rm c}$(1)$^c$ & & $M_{{\rm ZAMS}}$ & $t_{{\rm MS}}$ & $t_{{\rm RGB}}$ & $t_{{\rm He-b}}$ & $t_{{\rm EAGB}}$ & $M_{{\rm tot}}$(1) & $M_{\rm c}$(1) \\ %\noalign{\smallskip} \hline %\noalign{\smallskip} 1.0 & 8616.2 & 3350.1 & 110.17 & 12.971 & 0.709 & 0.501 & & 1.0 & 6751.9 & 2521.0 & 104.48 & 10.369 & 0.742 & 0.513 \\ 1.2 & 4473.9 & 1555.6 & 106.47 & 12.368 & 0.981 & 0.509 & & 1.2 & 3600.5 & 1182.0 & 97.963 & 10.474 & 0.999 & 0.521 \\ 1.5 & 2560.8 & 242.28 & 108.73 & 11.645 & 1.353 & 0.511 & & 1.5 & 2097.9 & 193.39 & 99.367 & 9.8133 & 1.366 & 0.521 \\ 1.6 & 2091.5 & 172.58 & 110.80 & 12.243 & 1.476 & 0.508 & & 1.6 & 1725.1 & 137.98 & 100.87 & 11.363 & 1.490 & 0.516 \\ 1.8 & 1465.8 & 99.847 & 130.85 & 13.305 & 1.595 & 0.496 & & 1.8 & 1223.8 & 78.851 & 128.10 & 11.802 & 1.637 & 0.497 \\ 2.0 & 1075.0 & 58.364 & 177.34 & 15.417 & 1.895 & 0.478 & & 2.0 & 900.54 & 32.110 & 236.41 & 14.571 & 1.941 & 0.464 \\ 2.6 & 510.25 & 12.302 & 140.08 & 10.175 & 2.530 & 0.518 & & 2.6 & 448.03 & 9.9558 & 106.62 & 6.7430 & 2.506 & 0.569 \\ 3.0 & 344.35 & 7.1561 & 83.500 & 5.7529 & 2.900 & 0.596 & & 3.0 & 309.24 & 5.9283 & 60.199 & 3.7127 & 2.863 & 0.672 \\ 4.0 & 161.46 & 2.7018 & 28.711 & 1.8755 & 3.821 & 0.765 & & 4.0 & 152.27 & 2.3324 & 23.405 & 1.2466 & 3.812 & 0.801 \\ 5.0 & 92.624 & 1.3843 & 13.577 & 0.9122 & 4.800 & 0.830 & & 5.0 & 90.826 & 1.2398 & 12.184 & 0.6929 & 4.776 & 0.868 \\ 6.0 & 60.471 & 0.8147 & 8.1598 & 0.4890 & 5.767 & 0.928 & & 6.0 & 60.976 & 0.7491 & 7.7504 & 0.4100 & 5.711 & 0.991 \\ \hline\hline \multicolumn{6}{c}{$Z = 0.04$ / solar} & & & \multicolumn{7}{c}{$Z = 0.004$ / solar} \\ %\noalign{\smallskip} \hline %\noalign{\smallskip} $M_{{\rm ZAMS}}$ & $t_{{\rm MS}}$ & $t_{{\rm RGB}}$ & $t_{{\rm He-b}}$ & $t_{{\rm EAGB}}$ & $M_{{\rm tot}}$(1) & $M_{\rm c}$(1) & & $M_{{\rm ZAMS}}$ & $t_{{\rm MS}}$ & $t_{{\rm RGB}}$ & $t_{{\rm He-b}}$ & $t_{{\rm EAGB}}$ & $M_{{\rm tot}}$(1) & $M_{\rm c}$(1) \\ %\noalign{\smallskip} \hline %\noalign{\smallskip} 1.0 & 8648.4 & 3974.3 & 119.31 & 14.213 & 0.682 & 0.504 & & 1.0 & 5771.4 & 2050.5 & 92.852 & 10.965 & 0.776 & 0.517 \\ 1.2 & 4788.6 & 1527.4 & 119.81 & 12.305 & 0.963 & 0.513 & & 1.2 & 3141.2 & 966.74 & 94.451 & 9.3231 & 1.026 & 0.525 \\ 1.5 & 2697.1 & 231.58 & 122.80 & 12.425 & 1.349 & 0.513 & & 1.5 & 1847.2 & 164.02 & 94.336 & 9.2462 & 1.383 & 0.527 \\ 1.6 & 2196.0 & 167.42 & 124.74 & 14.042 & 1.476 & 0.510 & & 1.6 & 1525.1 & 117.01 & 103.22 & 9.0807 & 1.505 & 0.521 \\ 1.8 & 1527.7 & 96.664 & 158.38 & 13.966 & 1.611 & 0.496 & & 1.8 & 1088.4 & 65.247 & 131.73 & 11.283 & 1.672 & 0.499 \\ 2.0 & 1108.6 & 54.286 & 226.81 & 17.353 & 1.903 & 0.481 & & 2.0 & 812.67 & 27.464 & 199.22 & 11.361 & 1.935 & 0.488 \\ 2.6 & 509.95 & 13.146 & 140.91 & 10.013 & 2.518 & 0.528 & & 2.6 & 410.03 & 8.5853 & 82.059 & 4.0737 & 2.472 & 0.639 \\ 3.0 & 337.90 & 7.6362 & 83.253 & 6.2347 & 2.893 & 0.596 & & 3.0 & 286.74 & 5.2255 & 50.584 & 2.3417 & 2.834 & 0.744 \\ 4.0 & 151.95 & 2.8971 & 29.886 & 2.1740 & 3.826 & 0.750 & & 4.0 & 145.00 & 2.1178 & 20.483 & 1.1477 & 3.801 & 0.809 \\ 5.0 & 84.428 & 1.4122 & 13.929 & 1.0935 & 4.791 & 0.810 & & 5.0 & 88.228 & 1.1468 & 11.488 & 0.5852 & 4.775 & 0.894 \\ 6.0 & 53.949 & 0.8091 & 7.9334 & 0.5929 & 5.651 & 0.893 & & 6.0 & 60.070 & 0.7068 & 7.5367 & 0.3372 & 5.700 & 1.060 \\ \noalign{\smallskip} \hline \noalign{\medskip} \end{tabular} \end{table}