Table 4: Linear Pearson correlation coefficients.
  $\sigma_{\rm PA}-k_{3,5}/k_{1}$ $\Delta \phi-\sigma_{\rm PA}$ $k_{3,5}/k_{1}-\Delta \phi$
this sample 0.5 0.7 0.2
local sample 0.7 0.1 0.7
  $R_{\rm d}-k_{3,5}/k_{1}$ $R_{\rm d}-\sigma_{\rm PA}$ $R_{\rm d}-\Delta \phi$
this sample -0.3 -0.4 -0.3
local sample 0.0 0.1 0.0
  MB-k3,5/k1 $M_{B}-\sigma_{\rm PA}$ $M_{B}-\Delta \phi$
this sample 0.5 0.4 0.4
local sample 0.1 -0.2 0.1
  A-k3,5/k1 $A-\sigma_{\rm PA}$ $A-\Delta \phi$
this sample 0.0 -0.3 0.0
  C-k3,5/k1 $C-\sigma_{\rm PA}$ $C-\Delta \phi$
this sample 0.1 0.2 0.1
  $F_{\rm em}-k_{3,5}/k_{1}$ $F_{\rm em}-\sigma_{\rm PA}$ $F_{\rm em}-\Delta \phi$
this sample -0.5 -0.4 -0.7
  $F_{\rm em}/L_{B}-k_{3,5}/k_{1}$ $F_{\rm em}/L_{B}-\sigma_{\rm PA}$ $F_{\rm em}/L_{B}-\Delta \phi$
this sample -0.4 -0.5 -0.7
  z-k3,5/k1 $z-\sigma_{\rm PA}$ $z-\Delta \phi$
both samples -0.1 -0.2 0.4
$\Delta \phi $ of the galaxies that have $\epsilon \leq 0.1$ (galaxy F2 in ``this sample'', NGC 628, NGC 3184, NGC 3938 and NGC 5713 in the local sample), k3,5/k1 of galaxy F5 (this sample) and all parameters for galaxy F10 (this sample) are doubtful as explained in Sect. 4.1. Therefore they are excluded while calculating the correlation coefficients. For the calculation of the correlations with the redshift, only field galaxies were used. So the results do not have the bias of the environment. Including the cluster galaxies does not change the result.

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