| D | P | |
| distant galaxies: cluster versus field | ||
| M20 | 0.36 | 0.013 |
| Gini | 0.46 | 0.000 |
| A | 0.31 | 0.048 |
| C | 0.50 | 0.000 |
| field galaxies: distant versus local | ||
| M20 | 0.50 | 0.011 |
| Gini | 0.43 | 0.048 |
| A | 0.18 | 0.898 |
| C | 0.48 | 0.017 |
Notes. D: K-S statistics specifying the maximum deviation between the cumulative distribution of the morphological parameters for distant galaxies: cluster versus field and for field galaxies: distant versus local; P: significance level of the K-S statistics. In this analysis, only the galaxies for which spectroscopic redshifts are available (see Table 3 here and Table 1 in Paper III) and that are late morphological types (spiral/irregular) according to our eye-ball classification (see Tables 3 and 4) were used. Galaxy 2F19 was also excluded since it is not distant (z=0.0052).
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