\begin{table}%T5
%\centering
\par
\caption{Stellar populations for the cluster galaxies in terms of the
six stellar components defined (see text): main sequence (luminosity class~V)
young, intermediate and old populations; giant (luminosity class~III) young
and intermediate populations; young supergiant (luminosity class~I) 
populations.
All values are in percentage and give the contribution of each 
population component to the total light at $\lambda_{\rm ref} = 4200 $~\AA.
The distance~$D$, the number of features ($n_{\rm f}$) (see Sect.~\ref{metodo}) used 
for each solution found and the value of $E(B-V)$, when applicable, 
are also given. The relative position of each galaxy within the cluster (see Fig.~\ref{psg} is indicated in the second row ("ct'' stands for 
centre or core; "it'' denotes the intermediate region and "p'' identifies 
peripheral galaxies).  
}
\label{t5}
\begin{tabular}{rccccccc|rcc}
\noalign{\smallskip}
\hline\hline
\noalign{\smallskip}
CL0048&position&V young&V int.&V old&III young&III int.& I young&$D$&$n_{\rm f}$&$E(B-V)$\\
\noalign{\smallskip}
\hline
\noalign{\smallskip}
218&ct.&  &  &25&  &25&50&193&36&0.0\\
235&ct.&  &  &32&  &45&23&63 &33&0.0\\
189&ct.&  &11&40&  & 9&40&106&30&0.0\\
213&ct.&  &16&20&14&45& 5&75 &37&0.0\\
216&ct.&  &16&17& 4&53&10&125&43&0.0\\
231&it.&  &  &15& 1&17&67&50 &18&0.0\\
102&it.&  &  &  &  &42&58&582&33&0.0\\
128&it.&  &  &40&  & 7&53&96 &32&0.0\\
184&it.&  &17&17& 3&41&22&56 &35&0.0\\
322&it.&18&22&27&13&18& 2&36 &33&0.0\\
343&it.&  &11&27&  &26&36&117&41&0.0\\
391&it.&  &  &  &  &41&59&75 &19&0.0\\
396&p. &  &  &40&  &  &60&52 &19&0.0\\
404&p. &  &10&4 &21&49&16&60 &32&0.15\\
421&p. &  &  &12&  &  &88&164&26&0.0\\
443&p. & 6&  &13& 1&60&20&66 &28&0.0\\
451&p. &  &7 &29&  &43&21&280&31&0.0\\
902&p. &  &20&13&  &35&32&156&35&0.0\\
37 &p. & 6&  &  & 3&33&58&17 &19&0.0\\
\hline
\end{tabular}
\end{table}