\begin{table}%t8
\caption{Best-fitting ages, metallicity and abundance ratios.}
\label{stellarpopresult}
\small%\centerline
{
\begin{tabular}{c c c c c}
\hline
\hline
\noalign{\smallskip}
$r$ (arcsec) & Age (Gyr) & [Z/H] & [E/Fe] & $\chi^2$\\
\hline
Major axis &              &                &                &      \\
--5.5, --1.8  &  3.5 $\pm$ 1.4 &  0.22 $\pm$ 0.12 &  0.19 $\pm$ 0.05 & 0.30 \\
--1.8, --0.5  &  1.6 $\pm$ 0.3 &  0.70 $\pm$ 0.17 &  0.28 $\pm$ 0.05 & 1.67 \\
--0.5, +0.5  &  1.6 $\pm$ 0.3 &  0.79 $\pm$ 0.16 &  0.29 $\pm$ 0.05 & 1.73 \\
+0.5, +1.8  &  1.7 $\pm$ 0.3 &  0.69 $\pm$ 0.16 &  0.29 $\pm$ 0.05 & 1.93 \\
+1.8, +5.5  &  2.0 $\pm$ 0.5 &  0.50 $\pm$ 0.15 &  0.15 $\pm$ 0.05 & 1.74 \\
\hline
Minor axis &              &                &                &      \\
--5.8, --0.8  &  5.4 $\pm$ 2.3 &  0.05 $\pm$ 0.12 &  0.20 $\pm$ 0.05 & 0.04 \\
--0.8, +0.8  &  1.8 $\pm$ 0.3 &  0.55 $\pm$ 0.15 &  0.30 $\pm$ 0.05 & 0.38 \\
+0.8, +5.8  &  2.2 $\pm$ 0.6 &  0.50 $\pm$ 0.14 &  0.24 $\pm$ 0.05 & 0.83 \\
\hline
\end{tabular}}
\medskip
The upper part of the table corresponds to the optical major axis, the lower part to the minor axis.
\end{table}