\begin{table}%t6
\caption{\label{tab_ksmorph}K-S statistics of the morphological parameters of our sample and the local sample.}
%\centering
\par
\begin{tabular}{lcccc}
\hline \hline \noalign{\smallskip}
&$D$ & $P$ 	\\
&distant galaxies: cluster versus field & \\
\hline
$M_{20}$ & 0.36 & 0.013 \\
Gini & 0.46 & 0.000 \\
$A$ & 0.31 & 0.048 \\
$C$ & 0.50 & 0.000 \\
\hline
&field galaxies: distant versus local & \\
$M_{20}$ & 0.50 & 0.011 \\
Gini & 0.43 & 0.048 \\
$A$ & 0.18 & 0.898 \\
$C$ & 0.48 & 0.017 \\
\hline
\end{tabular}
\tablefoot {$D$: K-S statistics specifying the maximum deviation between the cumulative distribution of the morphological parameters for distant galaxies: cluster versus field and for field galaxies: distant versus local; $P$:~significance level of the K-S~statistics.  In~this analysis, only the galaxies for which spectroscopic redshifts are available (see Table~\ref{centdist} here and Table~\ref{cltable} in Paper~III) and that are late morphological types (spiral/irregular) according to our eye-ball classification (see~Tables~\ref{centdist} and~\ref{eyeball}) were used.  Galaxy~2F19 was also excluded since it is not distant ($z=0.0052$).}
\end{table}