\begin{table}%t2
\caption{Parameters quantifying the irregularity of the gas kinematics measured
for our sample.}
\label{tab2}
\small%\centerline
 {
\begin{tabular}{ccccc}
\hline\hline
ID &  $R_{\rm max}$ &  $\sigma_{\rm PA}$    &   $\Delta \phi$    &  $ k_{3,5}/k_{1}$  \\
$(1)$ & $(2)$ & $(3)$  &  $(4)$  & $(5)$   \\
\hline
 C7 &  13.8	     &  23 &  68 $\pm$ 26   & 0.32 $\pm$ 0.20   \\
 C8 &  20.9	     &   2 &   9 $\pm$  6   & 0.06 $\pm$ 0.05   \\
 C9 &	9.2	     &  19 &  66 $\pm$  20   & 0.10 $\pm$ 0.03   \\ 
 C10 &  11.7	     &   9 &  14 $\pm$  9   & 0.26 $\pm$ 0.08   \\
 F2 &  10.5	     &   2 &  35 $\pm$ 37   & 0.08 $\pm$ 0.02   \\
 F3 &	10.0	     &   7 &  39 $\pm$  9   & 0.07 $\pm$ 0.05   \\
 F4 &	5.5	     &  21 &  18 $\pm$  20  & 0.30 $\pm$ 0.19   \\
 F5 &  11.3	     &   5 &  46 $\pm$  9   & 0.08 $\pm$ 0.03   \\ 
 F6 &	4.4	     &  29 &  57 $\pm$ 44   & 0.27 $\pm$ 0.18   \\ 
 F7 &  14.1  	     &   3 &   0 $\pm$ 11   & 0.05 $\pm$ 0.02   \\
 F10 &	8.4	     &   8 &   1 $\pm$  7   & 0.25 $\pm$ 0.05   \\
 F11 &  1\farcs7 &   5 &  18 $\pm$  5   & 0.05 $\pm$ 0.02   \\
\hline
\end{tabular}}
\medskip
Column (1): object ID; Col.~(2): maximum radius for which kinematic parameters could be calculated.  The conversion from arcsecond into kpc was done as explained in \citet{W06}; Col.~(3): standard deviation of the kinematic position angle~($\sigma_{\rm PA}$); Col.~(4): mean misalignment between the kinematic and photometric position angles~($\Delta \phi$); Col.~(5): mean $k_{3,5}/k_{1}$ of the analysis done while fixing the position angle and the ellipticity to their global values. \\
For galaxy F11, only the photometric redshift is available.  Since
photometric redshifts have big uncertainties, we give $R_{\rm max}$ of this galaxy in
arcseconds.  $k_{3,5}/k_{1}$ of galaxy~F5, $\Delta \phi$ of the galaxies that
have $\epsilon \leq 0.1$ (galaxy~F2) and all parameters for galaxy~F10 are
rather meaningless as explained in Sect.~4.1.  Therefore they are
excluded from the analysis.
\end{table}