\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}