Internal kinematics of spiral galaxies in distant clusters - IV. Gas kinematics of spiral galaxies in intermediate redshift clusters and in the field

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Table 10:

K-S statistics comparing the kinematic (ir)regularity parameters of the galaxies in our sample classified as spiral or irregular/ peculiar using their photometry.
	D	P
$\sigma _{\rm PA}$	0.15	0.995
k_3,5/k₁	0.10	1.000
$\Delta \phi$	0.25	0.786

Notes. 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/k₁ 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. 3.8 for the rest.

Source LaTeX | All tables | In the text

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