\begin{table}%t7
\caption{\label{tab2}Parameters quantifying the (ir)regularity of the gas kinematics measured
for our sample.}
\par
%\centering
\par
\begin{tabular}{lccccc}
\hline \hline \noalign{\smallskip}
ID &  $R_{\rm max}$ &  $\sigma_{\rm PA}$    &   $\Delta \phi$    &  $ k_{3,5}/k_{1}$ & $V_{\rm asym}$ \\
$(1)$ & $(2)$ & $(3)$  &  $(4)$  & $(5)$ & $(6)$   \\
\hline
 1C7 &  13.8	     &  23 &  68 $\pm$ 26   & 0.32 $\pm$ 0.20  &  0.25  $\pm$  0.08  \\
 1C8 &  20.9	     &   2 &   9 $\pm$  6   & 0.06 $\pm$ 0.05  &  0.08  $\pm$  0.02  \\
 1C9 &	9.2	     &  19 &  66 $\pm$  20  & 0.10 $\pm$ 0.03  &  0.13  $\pm$  0.02   \\ 
 1C10 &  11.7	     &   9 &  14 $\pm$  9   & 0.26 $\pm$ 0.08  &  0.19  $\pm$  0.08  \\
 1F2 &  10.5	     &   2 &  35 $\pm$ 37   & 0.08 $\pm$ 0.02  &  0.08  $\pm$  0.02  \\
 1F3 &	10.0	     &   7 &  39 $\pm$  9   & 0.07 $\pm$ 0.05  &  0.05  $\pm$  0.02  \\
 1F4 &	5.5	     &  21 &  18 $\pm$  20  & 0.30 $\pm$ 0.19  &  0.21  $\pm$  0.10  \\
 1F5 &  11.3	     &   5 &  46 $\pm$  9   & 0.08 $\pm$ 0.03  &  0.09  $\pm$  0.03  \\ 
 1F6 &	4.4	     &  29 &  57 $\pm$ 44   & 0.27 $\pm$ 0.18  &  0.20  $\pm$  0.21  \\ 
 1F7 &  14.1  	     &   3 &   0 $\pm$ 11   & 0.05 $\pm$ 0.02  &  0.06  $\pm$  0.01  \\
 1F10 &	8.4	     &   8 &   1 $\pm$  7   & 0.25 $\pm$ 0.05  &  0.23  $\pm$  0.10  \\
 1F11 &  1\farcs7    &   5 &  18 $\pm$  5   & 0.05 $\pm$ 0.02  &  0.20  $\pm$  0.16  \\
 2C3	    &        9.7	  &  21	  &	47  $\pm$     60	  &   0.11	   $\pm$      0.04	&   0.10    $\pm$	0.04    \\
 2C5	    &        7.5	  &   5	  &	38  $\pm$     37	  &   0.06	   $\pm$      0.06	&   0.02    $\pm$	0.02    \\
 2C6	    &        8.8	  &  15	  &	84  $\pm$     14	  &   0.10	   $\pm$      0.03	&   0.12    $\pm$	0.04    \\
 2C7	    &        8.3	  &   6	  &	61  $\pm$     18	  &   0.09	   $\pm$      0.09	&   0.03    $\pm$	0.02    \\
 2C8	    &        7.6	  &   4	  &	77  $\pm$     17	  &   0.16	   $\pm$      0.08	&   0.11    $\pm$	0.05    \\
 2F1	    &        14.2	  &   6	  &	73  $\pm$      5	  &   0.06	   $\pm$      0.03	&   0.08    $\pm$	0.04    \\
 2F2	    &        4.2	  &   6	  &	72  $\pm$     34	  &   0.09	   $\pm$      0.08	&   0.12    $\pm$	0.14    \\
 2F3	    &        14.4	  &  17	  &	 1  $\pm$     34	  &   0.12	   $\pm$      0.05	&   0.17    $\pm$	0.08    \\
 2F4	    &        8.0	  &   7	  &	24  $\pm$     35	  &   0.06	   $\pm$      0.01	&   0.07    $\pm$	0.03    \\
 2F5	    &        11.3	  &  37	  &	 4  $\pm$     36	  &   0.06	   $\pm$      0.01	&   0.10    $\pm$	0.07    \\
 2F6	    &        4.6	  &   9	  &	62  $\pm$     13	  &   0.13	   $\pm$      0.08	&   0.11    $\pm$	0.06    \\
 2F9	    &        7.4	  &   8	  &	22  $\pm$      8	  &   0.18	   $\pm$      0.13	&   0.17    $\pm$	0.12    \\
 2F10	    &        11.6	  &   7	  &	37  $\pm$     10	  &   0.09	   $\pm$      0.04	&   0.11    $\pm$	0.03    \\
 2F11	    &        17.0	  &  43	  &	29  $\pm$     49	  &   0.83	   $\pm$      0.83	&   1.05    $\pm$	1.86    \\
 2F12	    &        11.4	  &   3	  &	30  $\pm$     36	  &   0.07	   $\pm$      0.02	&   0.05    $\pm$	0.02    \\
 2F15\&16    &        1\farcs9 	  &  19   &    --   		 	  &   0.77	   $\pm$      0.50	&   2.38    $\pm$	6.15    \\
 3C3	    &        12.2	  &   4	  &	 3  $\pm$      4	  &   0.17	   $\pm$      0.11	&   0.13    $\pm$	0.05    \\
 3C4	    &        12.7	  &   8	  &	 1  $\pm$      9	  &   0.15	   $\pm$      0.05	&   0.08    $\pm$	0.03    \\
 3C5	    &        7.5	  &   7	  &	84  $\pm$      7	  &   0.07	   $\pm$      0.03	&   0.11    $\pm$	0.10    \\
 3C6	    &        6.5	  &  11   &	52  $\pm$      8	  &   0.10	   $\pm$      0.07	&   0.18    $\pm$	0.11    \\
 3C7	    &        8.8	  &   3	  &	46  $\pm$      2	  &   0.09	   $\pm$      0.05	&   0.20    $\pm$	0.13    \\
 3F3	    &        3.7	  &   5	  &	48  $\pm$      5	  &   0.11	   $\pm$      0.02	&   0.10    $\pm$	0.07    \\
 3F6	    &        6.7	  &   3	  &	55  $\pm$      3	  &   0.16	   $\pm$      0.18	&   0.15    $\pm$	0.13    \\
 3F7	    &        4.8	  &   9	  &	97  $\pm$     25	  &   0.06	   $\pm$      0.04	&   0.06    $\pm$	0.03    \\
 3F8	    &        13.2	  &   4	  &	17  $\pm$     37	  &   0.20	   $\pm$      0.05	&   0.30    $\pm$	0.43    \\
 3F9	    &        7.7	  &   9	  &	46  $\pm$      9	  &   0.13	   $\pm$      0.02	&   0.13    $\pm$	0.11    \\
 4C2	    &        7.4	  &   3	  &	65  $\pm$      2	  &   0.08	   $\pm$      0.01	&   0.07    $\pm$	0.04    \\
 4C3	    &        8.9	  &  13	  &	63  $\pm$     12	  &   0.22	   $\pm$      0.14	&   0.14    $\pm$	0.03    \\
 4F3	    &        15.0	  &   9	  &	40  $\pm$     20	  &   0.07	   $\pm$      0.03	&   0.14    $\pm$	0.03    \\
 4F4	    &        10.8	  &   8	  &	60  $\pm$      9	  &   0.82	   $\pm$      1.21	&   0.57    $\pm$	0.64    \\
 4F5	    &        16.5	  &   9	  &	17  $\pm$     32	  &   0.07	   $\pm$      0.04	&   0.04    $\pm$	0.02    \\
 4F6	    &        10.7	  &   6	  &	28  $\pm$     31	  &   0.12	   $\pm$      0.05	&   0.09    $\pm$	0.04    \\
 4F7	    &        27.5	  &  29	  &	 7  $\pm$     53	  &   0.20	   $\pm$      0.06	&   0.17    $\pm$	0.05    \\
 4F8	    &        14.5	  &  18	  &	39  $\pm$     31	  &   0.18	   $\pm$      0.09	&   0.10    $\pm$	0.03    \\
 4F9	    &        8.7	  &   3	  &	55  $\pm$      3	  &   0.07	   $\pm$      0.05	&   0.05    $\pm$	0.02    \\
 4F12	    &        6.4  	  &  12	  &	24  $\pm$     18	  &   0.29	   $\pm$      0.16	&   0.17    $\pm$	0.07    \\
 4F13	    &        9.1	  &   2	  &	53  $\pm$      6	  &   0.10	   $\pm$      0.11	&   0.04    $\pm$	0.03    \\
\hline
\end{tabular}
\tablefoot{Column (1): object ID; Col.~(2): maximum radius for which the 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; Col.~(6): $V_{\rm asym}$~parameter of S08 measured as described in Sect.~\ref{shap}. The error is the standard deviation of the parameter in the range of observations. \\
For 1F11 and 2F15\&16, the spectroscopic redshifts are not available, therefore we give~$R_{\rm max}$ of these objects in arcseconds.  $k_{3,5}/k_{1}$~of galaxy~1F5, $\Delta \phi$~of the galaxies that have $\epsilon \leq 0.1$ (galaxies~1F2,~2F4, 2F12~and~4C3) and all parameters for galaxies~1F10,~2F5, 2F11~and~2F15\&16 are rather meaningless as explained in Paper~III for the MS~0451~sample and here, in~Sect.~\ref{special} for the rest, therefore they are excluded from the analysis.}
\end{table}