\begin{table}%t9
\caption{Clusters with both photometric and spectroscopic redshifts.
\label{tab:photspecred}}
%\centerline
{\begin{tabular}{cccl} 
\hline \hline
 Cluster    & PDCS & $\overline{z}_{\rm phot}$ & \multicolumn{1}{c}{$z_{{\rm spec}}$}   \\
\hline
%  V04       & P04  & --	  & $0.5505 \pm 0.0004$           \\
  V06       &  --  & 0.43 & $0.3658 \pm 0.0009$           \\
  V13      & P12 & 0.32 & $0.2630 \pm 0.0020$ $^{(1)}$  \\
  V17      &  --  & 0.32 & $0.3965 \pm 0.0002$ $^{(2)}$  \\
  V19      & P23 & 0.19 & $0.1290 \pm 0.0010$ $^{(1)}$  \\
  V23      & P20 & 0.34 & $0.3371 \pm 0.0002$ $^{(2)}$  \\
  V30      &  --  & 0.38 & $0.3979 \pm 0.0002$ $^{(2)}$  \\
  V36      & P11 & 0.36 & $0.3270 \pm 0.0030$ $^{(1)}$  \\
  V48      & P24 & 0.26 & $0.2674 \pm 0.0002$ $^{(2)}$  \\
  --        & P33 & 0.64 & $0.6400 \pm 0.0040$           \\
  --        & P36 & 0.18 & $0.2480 \pm 0.0020$           \\
  --        & P63 & 0.56 & $0.6863 \pm 0.0003$           \\
\hline
\end{tabular}}
\par
\smallskip
 $^{(1)}$  From Holden et~al. (\cite{Holden99}).\\
 $^{(2)}$  Redshift from SDSS data for a single galaxy that falls
into the brightest part of the ETS of the cluster.
\end{table}