\begin{table}%t10
\caption{\label{tabks}K-S statistics comparing the kinematic (ir)regularity parameters of the galaxies in our sample classified as spiral or irregular/ peculiar using their photometry.}
\par
%\centering
\par
\begin{tabular}{lcccc}
\hline \hline \noalign{\smallskip}
&$D$ & $P$ 	\\
\hline
${\sigma_{\rm PA}}$ & 0.15 & 0.995 \\
${k_{3,5}/k_{1}}$ & 0.10 & 1.000  \\
${\Delta \phi}$ & 0.25 & 0.786 \\
\hline
\end{tabular}
\tablefoot {$D$: K-S statistics specifying the maximum deviation between the cumulative distribution of the given parameter for spiral and irregular galaxies in our sample; $P$: significance level of the K-S statistics. \\ 
$k_{3,5}/k_{1}$ of galaxy~1F5, $\Delta \phi$ of the galaxies that have $\epsilon \leq 0.1$ (1F2, 2F4, 2F12 and~4C3) and all parameters for 1F10, 2F5, 2F11 and 2F15\&16 have been excluded from the calculations as explained in Paper~III for the MS~0451 sample and here, in Sect.~\ref{special} for the~rest.}
\end{table}