Table 2.
Kolmogorov–Smirnov-test p-values for the hypothesis that given two luminosity distributions are drawn from the same underlying luminosity function.
| Bin 1 | Bin 2 | Bin 3 | |
|---|---|---|---|
| Bin 2 | 0.83 | ||
| Bin 3 | 0.98 | 0.50 | |
| Bin 4 | 0.11 | 0.229 | 0.31 |
Notes. The bins correspond to different cluster-centric distances so that Bin 1 includes galaxies within R < 1.5 deg from NGC 1399, Bin 2: 1.5 deg < R < 2.5 deg, and Bin 3: R > 2.5 deg. Bin 4 includes the galaxies within one degree from the NGC 1399.
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