\begin{table}%T8
\caption{Classifications for all $54$ galaxies having a redshift measure.}
\label{t8}
%\centerline
{{
\begin{tabular}{rccccccccc}
\hline\hline
Gal id\#&{\it EW}[OII]&{\it EW} H$\delta$&{\it EW} H$\gamma$&{\it EW} H$\beta$&{\it EW} (H$\delta$+H$\gamma$)/2 &{\it EW} (H$\delta$+H$\gamma$+H$\beta$)/3 & Class &  Pos. &   Morph.\\   
\hline
\underline{\bf Cluster:}&&&&&&&&\\
35   &   23.4 &  8.2  &  1.3& $-$9.9&   4.75&    --&              EL&    p&   -- \\
37   &   12.3 &   4.7 &  4.1& $-$6.9&    4.40&      --  &            EL&    p  &   -- \\
102  &   7.0   &  4.6  &  2.0  &   0.0   &   3.3     &    --       &         N    &   it  &   sph  \\
128  &   1.2   &  6.0  & $-$   &  3.6   &   --    &     --       &         K+A   &  it  &	disk \\
184  &   0.0   &  1.5  &  0.0  &   1.6  &    0.75  &      1.0     &            N   &    it  &   sph \\
189  &  0.2  &   2.1  &  0.0  &   2.2   &   1.05  &      1.4    &             N    &   ct   &   sph \\
213  &   0.0  &   0.3  &  0.5  &   2.4   &   0.4    &     0.9     &            N   &    ct   &   sph \\
216  &    0.0  &   0.0   & 0.2  &   1.1   &   0.1   &      0.4     &            N    &   ct   &   sph \\
218  &   0.0  &   0.0  &  5.7  &   2.7    &  2.8    &     2.8    &             N    &   ct    &  sph \\
231  &    0.0  &   3.4   &  5.5  &   0.0  &    4.45  &      3.0    &             K+A  &   it  &   disk \\
235  &    0.9 &    1.0  &  1.1   &  2.7    &  1.05   &     1.6     &            N     &  ct    &  sph \\
296  &  19.7   &  4.6  &  2.8  & $-$4.6   &   3.7    &     --    &             EL  &    p   & $-$ \\
322  &    5.9  &   3.9 &   2.8  &   2.2   &   3.35   &     3.0     &            N   &    it  &   sph \\
343  &  19.0  &   2.1  &  0.5   & $-$10.3  &   1.3    &     0.9    &             EL   &   it  &   sph \\
391  &    9.4  &   4.9 &   6.9   & $-$   &   5.9   &      --     &            N   &    it   &  sph \\
396  &    9.1  &   3.7  &  0.0  &   0.0   &   1.8    &     1.2     &           N/K+A    &   p   &  disk \\
404  &  10.0  &   3.9  &  6.2  &   0.0   &   5.0   &      3.4    &             EL  &    p   &  disk \\
421  &    8.7  &   1.8  &  2.7  &   0.0   &   2.2    &     1.5    &             N   &    p &    sph \\
443  &   35.5  &   -- &   --  &   --   &   --   &      --    &             EL   &   p   &  -- \\
449  &   28.0  &   4.9 & $-$1.5  & $-$1.7   &   --    &     --     &            EL  &    p  &   -- \\
451  &    0.0  &   3.1  &  --   &  --  &    --   &      --     &            N    &   p  &   -- \\
452  &   34.4  &   1.9 & $-$4.2   &  --    &  --    &     --     &            EL   &   p  &   -- \\
902  &    2.8  &   2.2  &  0.9   &  0.0   &   1.5    &     1.0    &             N    &   p   &  sph \\
\hline
\underline{\bf Field:}&&&&&&&&&\\
44   &  -- &   3.8 &  1.3 & $-$0.8  &   2.5   &     --    &            EL    &     &  -- \\
58   &  10.7 &   6.9 &  1.8 &   --  &   4.4    &    --     &           EL     &     & $-$ \\
76   &  32.6 &   2.6 &  3.6  & $-$6.4  &   3.1    &    --     &           EL    &      & $-$ \\
121  &   9.4 &   3.1 &  2.2 & $-$0.8  &   2.6   &     --     &           N      &     & $-$ \\
161  &   4.9 &   4.2 &  7.0 &   --   &  5.6   &     --     &           K+A   &      & $-$ \\
188  &  69.0 &   0.0 &  4.5 & $-$24.0 &   --   &     --     &           EL    &      & $-$ \\
196  &  17.1  &  4.8 &  2.9 & $-$13.2 &   3.8   &     --     &           EL    &      & disk \\
199  &   9.2 &   0.6 &  0.0 &   3.6   &  0.3   &     1.4      &          N     &      & sph \\
203  &  23.0 &   6.0 &  3.7 & $-$2.4  &   4.8   &     --     &           EL    &      & $-$ \\
212  &  31.5 &   4.9 &  2.0 & $-$7.5  &   2.3    &    --     &           EL    &      & $-$ \\
217  &   0.0 &   0.0 &  0.1 &   1.1  &   0.05  &     0.4      &          N     &      & sph \\
244  &   2.0 &   0.0 &  1.6  &  3.7 &    0.8   &     1.8     &           N     &      & $-$ \\
245  &  10.8  &  7.9  & 4.7 &   --  &   6.3   &     --     &           EL     &     & $-$ \\
248  &  17.7 &   1.8 &  0.3 & $-$1.1  &   1.0   &     --     &           EL    &      & $-$ \\
265  &   0.0 &   2.3 &  2.4 &   2.5  &   2.35  &     2.4     &           N     &      & $-$ \\
266 &   14.0 &   4.9 &  5.5 &   --  &   5.2   &     --     &           EL    &      & $-$ \\
280  &   0.0  &  1.5 &  0.0 &   3.3  &   0.75  &     1.6    &            N      &     & $-$ \\
286  &   7.8 &   6.5 &  --  &  2.6  &   --   &     --      &          N     &      & disk \\
304  &  25.4 &   6.9  & 0.0 & $-$4.9  &   3.0   &     --    &            EL    &      & $-$ \\
346  &   0.0 &   1.6 &  0.9 &   2.8 &    1.2   &     1.8   &             N     &      & sph \\
399  &   5.4 &   -- &  -- &   --  &   --   &     --    &          N/K+A      &       & disk \\
400  &  27.4 &   5.1  & 2.0 & $-$0.5  &   3.6   &     --     &           EL     &     & sph \\
419  &  12.7 &   2.8 &  4.7 &   --  &   3.8   &     --     &           EL    &      & sph \\
424  &   0.0 & $-$2.7 &  0.0 &   --  &   --    &    --     &           N      &     & sph \\
428  &   3.1 &   0.7 &  4.3 &   1.3  &   2.5    &    2.1    &            N     &      & sph \\
439  &  17.9 &   4.4 &  2.5 &   --  &   3.4   &     --     &           EL    &      & disk \\
901  &  53.6 &  10.6 &  0.7 & $-$13.0 &   5.6   &     --     &           EL    &      & sph \\
903  &   7.8  &  3.3 &  3.5 & $-$0.2  &   3.4  &      --     &           N     &      & sph \\
906  &   5.6  &  3.9 &  -- &   --  &   --   &     --     &           N     &      & -- \\
907  &  30.7 &   2.9 &  0.0 & $-$9.2  &   1.4   &     --     &           EL    &      & sph \\
908  &   0.0 &   3.0 &  2.2 &   3.7  &   2.6    &    3.0     &          N/K+A     &      & $-$ \\
\hline
\end{tabular}}
}
\par
\medskip
Notes: All {\it EW} are given in \AA; Col. "Class'' gives the spectral 
classification. For three of the objects (\#396, \#399, \#908), since 
the  two methods  described (see Sects.~\ref{normais} 
and~\ref{alternativo}), 
do not give the same result, we display both of them.
Column "Pos.'' indicates the relative position of each 
cluster galaxy within the cluster as in Fig.~\ref{psg} ("ct'' stands for 
centre or core; "it'' denotes the intermediate region and "p'' identifies 
peripheral galaxies. Finally, Col.~"Morph.'' lists the morphological 
classification attributed by La~Barbera et~al. (2003): "sph'' (for spheroidal 
galaxies) and "disks''.
\end{table}