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Table 12:

Irregularity fraction.
  ${\rm frac}_{\sigma_{\rm PA}}$ ${\rm frac}_{\Delta \phi}$ ${\rm frac}_{k_{3,5}/k_{1}}$ ${\rm frac}_{\rm any}$ ${\rm frac}_{\rm all}$
  (1) (2) (3) (4) (5)
field & cluster 11 $\pm$ 5$\%$ 68 $\pm$ 7$\%$ 32 $\pm$ 7$\%$ 80 $\pm$ 6$\%$ 4 $\pm$ 3$\%$
only field 10 $\pm$ 6$\%$ 65 $\pm$ 9$\%$ 32 $\pm$ 9$\%$ 76 $\pm$ 8$\%$ 3 $\pm$ 3$\%$
only cluster 13 $\pm$ 8$\%$ 73 $\pm$ 11$\%$ 31 $\pm$ 12$\%$ 88 $\pm$ 8$\%$ 6 $\pm$ 6$\%$

Notes. Column (1): fraction of irregular velocity fields according to $\sigma _{\rm PA}$criterion; Col. (2): fraction of irregular velocity fields according to $\Delta \phi $ criterion; Col. (3): fraction of irregular velocity fields according to k3,5/k1 criterion; Col. (4): fraction of irregular velocity fields according to at least one of the three criteria; Col. (5): fraction of irregular velocity fields according to all the three criteria together.
Poisson errors are given for each fraction.
k3,5/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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