\begin{table}%t1
%\centering
\par
\caption{Comparison of the ZAHB levels, He core masses (in solar
mass units), HB evolutionary times (in Myr) and RGB evolutionary times
at brighter magnitudes than the ZAHB (in Myr) between the models used
in Zoccali et~al.~(\cite{Zoccali00}), in Paper~I, and the models by Cassisi et~al.~(\cite{Cassisi98}), for two selected metallicities
(see text for details).\label{compmodels}}
\begin{tabular}{lccccc} 
\hline \hline
            Zoccali et~al.~(\cite{Zoccali00})
            & $M_V\rm (ZAHB)$ 
            & $M_{\rm c}\rm (He)$
            & $t_{\rm HB}$
            & $t_{\rm RGB}$\\
\hline
%            \endhead
$Z=0.001$  & 0.54   & 0.499  & 102 & 63\\
$Z=0.006$  & 0.72   & 0.493  & 112 & 55\\
\hline
Cassisi et~al.~(\cite{Cassisi98}) & & & & \\
\hline
$Z=0.001$ & 0.49  & 0.500   & 85   & 58 \\
$Z=0.006$ & 0.68  & 0.493   & 94   & 47 \\
\hline
Paper~I & & & & \\
\hline
$Z=0.001$  & 0.58   & 0.495  &  88  & 65\\
$Z=0.006$  & 0.74   & 0.489  &  93  & 56\\
\hline 				
\end{tabular} 
\end{table}