\begin{table}%t7 \caption{\label{tab:Ages}Logarithmic production ratios $\log\left(\mbox{Th/x}\right)_0$ and corresponding decay ages in \object{CS~29491$-$069} and \object{HE~1219$-$0312} in Gyr.} \par %\centerline {\small \begin{tabular}{lrrrrrrrr}\hline\hline Pair & \multicolumn{2}{c}{Logarithmic production ratios} & \multicolumn{3}{c}{\object{CS~29491$-$069}} & \multicolumn{3}{c}{\object{HE~1219$-$0312}}\\ & Solar residuals & HEW $10\le S\le280$ & Residual age$^{1}$ & HEW age & Error$^{2,3}$ & Residual age$^{1}$ & HEW age & Error$^{2,3}$\\ \hline Th/Ba & $-1.39$ & $-0.96$ & $ 1.9$ & $17.1$ & $ 9.9$ (3.3) & $-6.5$ & $8.7$ & $5.9$ (4.2)\\ Th/La & $-0.65$ & $-0.22$ & $ 0.9$ & $16.5$ & $ 9.6$ (2.3) & $-5.7$ & $9.9$ & $5.0$ (2.8)\\ Th/Ce & $-0.88$ & $-0.62$ & $17.1$ & $24.6$ & $10.9$ (5.6) & $-0.6$ & $6.8$ & $9.4$ (8.4)\\ Th/Pr & $-0.36$ & $-0.20$ & $10.3$ & $13.2$ & $11.7$ (7.0) & $-6.5$ & $-3.6$ & $5.6$ (3.7)\\ Th/Nd & $-1.03$ & $-0.87$ & $10.5$ & $13.4$ & $10.2$ (4.2) & $-2.6$ & $ 0.4$ & $4.8$ (2.3)\\ Th/Sm & $-0.80$ & $-0.71$ & $12.0$ & $11.8$ & $11.1$ (6.1) & $-0.1$ & $-0.3$ & $6.6$ (5.1)\\ Th/Eu & $-0.43$ & $-0.32$ & $ 3.0$ & $ 3.8$ & $ 9.4$ (1.4) & $-4.9$ & $-4.1$ & $4.6$ (1.9)\\ Th/Gd & $-0.99$ & $-0.73$ & $13.5$ & $21.1$ & $ 9.6$ (2.3) & $-0.5$ & $7.1$ & $6.3$ (4.7)\\ Th/Dy & $-1.01$ & $-0.69$ & $14.0$ & $24.2$ & $ 9.9$ (3.3) & $ 1.8$ & $12.0$ & $5.3$ (3.3)\\ Th/Ho & $-0.41$ & $ 0.04$ & $ 4.4$ & $21.2$ & $12.6$ (8.4) & $-7.3$ & $9.5$ & $7.4$ (6.1)\\ Th/Er & $-0.79$ & $-0.48$ & $16.8$ & $26.4$ & $ 9.9$ (3.3) & $ 1.8$ & $11.5$ & $5.9$ (4.2)\\ Th/Tm & $ 0.12$ & $ 0.22$ & & & & $ 0.0$ & $0.1$ & $7.4$ (6.1)\\ Th/Hf & $-0.46$ & $ 0.20$ & & & & $-2.1$ & $[24.2]$ & $9.4$ (8.4)\\ Th/Os & $-0.78$ & $-0.93$ & [$<$36.5] & [$<$24.6] & & & &\\ \hline \multicolumn{3}{l}{Arithmetic mean} & $9.5\pm6.0$ & $17.6\pm6.8$ & & $-2.6\pm3.3$ & $4.8\pm5.9$ &\\ \hline \end{tabular}} \medskip \par $^1$ Assuming a solar age of 4.6~Gyr; $^2$ without $\sigma_{{\rm sys}}$, see Sect.~\ref{sec:ErrorBudget}; $^3$ values in parentheses without the Th abundance uncertainty. \end{table}