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Table 7:

Parameters quantifying the (ir)regularity of the gas kinematics measured for our sample.

ID 		$R_{\rm max}$ $\sigma _{\rm PA}$ $\Delta \phi $ k3,5/k1 $V_{\rm asym}$
(1) (2) (3) (4) (5) (6)
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 $.\!\!^{\prime\prime}$7 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 $.\!\!^{\prime\prime}$9 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

Notes. 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 Wright (2006); 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  k3,5/k1 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. 4.6. 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. k3,5/k1 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. 3.8 for the rest, therefore they are excluded from the analysis.


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