Table 4
Results of the K-S tests.
| Compared samples | N1, N2 | Prob. (%) |
|
|
||
| Type dependence | ||
| Passive vs. SF in the cluster | 846, 517 | < 0.01 |
| Passive vs. SF in Region 2 | 120,21 | < 0.01 |
| Passive vs. SF in Region 3 | 120,31 | < 0.01 |
| Passive vs. SF in Region 4 | 102,20 | < 0.01 |
| Passive vs. SF in Region (b) | 96,33 | 0.4 |
| Passive vs. SF in Region (c) | 199,54 | < 0.01 |
| Passive vs. SF in Region (d) | 328, 420 | < 0.01 |
| Environment dependence – SF galaxies | ||
| SF within and outside r200 | 78, 439 | > 10 |
| SF in Regions 2 and 3 | 31,31 | > 10 |
| SF in Regions 3 and 4 | 31,20 | > 10 |
| SF in Regions (b) and (c) | 33,54 | > 10 |
| SF in Regions (c) and (d) | 54, 422 | > 10 |
| Environment dependence – Passive galaxies | ||
| Passive within and outside r200 | 438, 408 | > 10 |
| Passive in Regions 1 and 2 | 120, 120 | 0.8 |
| Passive in Regions 2 and 3 | 120, 102 | > 10 |
| Passive in Regions 3 and 4 | 102,96 | > 10 |
| Passive in Regions (a) and (b) | 100,83 | 0.4 |
| Passive in Regions (b) and (c) | 83, 199 | > 10 |
| Passive in Regions (c) and (d) | 199, 328 | 2 |
Notes. N1 and N2 are the number of galaxies in the two compared samples. The listed probabilities (Prob., in %) are for the null hypothesis that two M⋆ distributions are drawn from the same parent population. Probabilities > 10% indicate statistically indistinguishable distributions. Only the distributions of samples with at least ten objects have been considered.
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