\begin{table}%t2
\caption{\label{table:2}Synthesis results.}            
\small       
%\centerline
{          
\begin{tabular}{c c c c c c c c c}         
\hline\hline                 
LINERs & PL (\%) & I (\%) & II (\%) & III (\%) & IV (\%) & V (\%) & log age (yr) & Metallicity $(Z_\odot)$ \\
\hline    
NGC~315    &    7        &    2        & $<$1        & $<$1        & $<$1        &   92      &   9.79  &  1.29\\
NGC~1052   & $<$1        & $<$1        & $<$1        & $<$1        &   11        &   89      &  10.03  &  1.53\\
NGC~2768   & $<$1        & $<$1        & $<$1        & $<$1        &   37        &   63      &   9.79  &  2.07\\
NGC~2832   & $<$1        & $<$1        & $<$1        & $<$1        & $<$1        &   99      &  10.11  &  1.29\\
NGC~3193   &    9        & $<$1        & $<$1        & $<$1        & $<$1        &   91      &   9.72  &  1.12\\
NGC~3226   & $<$1        & $<$1        & $<$1        & $<$1        &   72        &   28      &   9.79  &  1.00\\
NGC~3379   & $<$1        & $<$1        & $<$1        & $<$1        & $<$1        &   99      &  10.11  &  1.68\\
NGC~3608   &    2        & $<$1        & $<$1        & $<$1        & $<$1        &   98      &  10.05  &  1.23\\
NGC~4261   & $<$1        & $<$1        & $<$1        & $<$1        &    5        &   95      &  10.06  &  1.49\\
NGC~4278   & $<$1        &    1        & $<$1        & $<$1        & $<$1        &   99      &  10.07  &  1.75\\
NGC~4374   & $<$1        & $<$1        &    2        & $<$1        &   90        &    8      &   9.18  &  2.46\\
NGC~4486   & $<$1        &    2        &    1        & $<$1        & $<$1        &   96      &   9.99  &  0.86\\
NGC~4494   & $<$1        & $<$1        &    7        & $<$1        &   11        &   83      &   9.80  &  1.25\\
NGC~4589   & $<$1        & $<$1        &   11        & $<$1        &    1        &   88      &   9.76  &  2.50\\
NGC~4636   & $<$1        & $<$1        & $<$1        & $<$1        & $<$1        &   99      &  10.04  &  1.00\\
NGC~5077   & $<$1        &    4        & $<$1        & $<$1        & $<$1        &   96      &   9.96  &  1.74\\
NGC~5322   & $<$1        & $<$1        &   12        & $<$1        & $<$1        &   88      &   9.75  &  2.50\\
NGC~5813   & $<$1        & $<$1        & $<$1        & $<$1        & $<$1        &   99      &  10.11  &  1.36\\
NGC~5982   &    1        & $<$1        & $<$1        & $<$1        & $<$1        &   98      &   9.98  &  0.99\\
NGC~7626   & $<$1        & $<$1        & $<$1        & $<$1        & $<$1        &   99      &  10.11  &  1.25\\
average    &    1.0      &    0.4      &    1.7      & $<$1        &   11        &   86      &   9.91  &  1.52\\
rms        &    2.5      &    1.0      &    3.6      & $<$1        &   25        &   24      &   0.22  &  0.51\\
\hline          
Inactive Es &   & I (\%) & II (\%) & III (\%) & IV (\%) & V (\%) & log age (yr)& Metallicity $(Z_\odot)$\\
\hline                        
NGC~221    &             &    1        & $<$1        &    4        &   94        & $<$1       & 9.33   &  1.88\\
NGC~821    &             & $<$1        & $<$1        & $<$1        & $<$1        &   99       & 10.10  &  1.18\\
NGC~2634   &             &    1        & $<$1        & $<$1        &    1        &   98       & 10.07  &  1.28\\
NGC~3348   &             & $<$1        &    4        & $<$1        & $<$1        &   96       & 10.01  &  2.50\\
NGC~3377   &             & $<$1        &    8        & $<$1        &   11        &   82       &  9.34  &  2.49\\
NGC~3610   &             & $<$1        &    7        & $<$1        &   56        &   37       &  9.36  &  2.40\\
NGC~3613   &             & $<$1        &    3        & $<$1        &   24        &   73       &  9.80  &  1.57\\
NGC~3640   &             & $<$1        & $<$1        & $<$1        &   30        &   70       &  9.82  &  1.45\\
NGC~4291   &             &    4        &    2        & $<$1        &   29        &   65       &  9.70  &  2.42\\
NGC~4339   &             & $<$1        &    3        & $<$1        &    1        &   95       &  9.96  &  1.59\\
NGC~4365   &             & $<$1        &   12        & $<$1        & $<$1        &   88       &  9.75  &  1.28\\
NGC~4406   &             &    2        & $<$1        & $<$1        & $<$1        &   98       & 10.04  &  0.94\\
NGC~4473   &             & $<$1        & $<$1        & $<$1        &   29        &   71       &  9.85  &  1.49\\
NGC~4478   &             & $<$1        & $<$1        & $<$1        &   99        & $<$1       &  9.66  &  0.90\\
NGC~4564   &             &    3        & $<$1        & $<$1        & $<$1        &   97       & 10.00  &  1.10\\
NGC~4621   &             &    2        & $<$1        & $<$1        & $<$1        &   98       & 10.03  &  1.18\\
NGC~4648   &             & $<$1        & $<$1        & $<$1        & $<$1        &   99       & 10.11  &  1.23\\
NGC~4649   &             & $<$1        & $<$1        & $<$1        &    3        &   96       & 10.03  &  0.95\\
NGC~4660   &             & $<$1        &    5        & $<$1        &   15        &   80       &  9.76  &  1.23\\
NGC~4914   &             & $<$1        &    8        & $<$5        &   87        & $<$1       &  9.45  &  2.43\\
NGC~5557   &             & $<$1        & $<$1        & $<$1        &    1        &   99       & 10.08  &  1.06\\
NGC~5576   &             &    2        &    6        & $<$1        &   25        &   66       &  9.62  &  1.52\\
NGC~5638   &             & $<$1        & $<$1        & $<$1        & $<$1        &   99       & 10.11  &  1.16\\
NGC~5831   &             & $<$1        & $<$1        & $<$1        & $<$1        &   99       & 10.11  &  1.22\\
NGC~7619   &             & $<$1        & $<$1        & $<$1        & $<$1        &   99       & 10.11  &  1.24\\
average    &             &    0.6      &    2.3      &    0.4      &   20        &   76       &  9.85  &  1.51\\
rms        &             &    1.1      &    3.4      &    1.3      &   31        &   32       &  0.26  &  0.53\\
\hline                          
\end{tabular}}
\smallskip
  Columns~(2)--(7) list the fractional
contribution to the total flux by the PL and by stellar populations I, II,
III, IV, and V, respectively. Contributions less than 1\% are listed as upper limits.
Column~(8) gives the mean stellar age, and Col. (9) gives the mean metallicity.
The last two rows show the average value and rms of each column. 
\end{table}