Table 9
Comparison between AMIGA and HCG samples.
| Number of objects | p val. | |||
| p AMIGA | p HCG | |||
|
|
||||
| AGN | AMIGA | 44.2 ± 5.8 | 52.2 ± 6.0 | 52.2% |
| (Fig. 10c) | (Fig. 10e) | |||
| HCG | 56.5 ± 6.2 | 56.0 ± 6.4 | 46.0% | |
| (Fig. 10f) | (Fig. 10d) | |||
|
|
||||
| AGN + TO | AMIGA | 79.3 ± 6.9 | 108.2 ± 7.1 | 5.9% |
| HCG | 95.5 ± 7.2 | 100.9 ± 7.4 | 16.7% | |
|
|
||||
| SFN | AMIGA | 115.9 ± 7.1 | 98.1 ± 5.7 | 0.05% |
| HCG | 71.6 ± 5.7 | 43.6 ± 5.2 | 6.9 × 10-7% | |
Notes. The rows correspond to the distribution of galaxies (sample) and the columns to the probability of harbouring an AGN, an AGN + TO or a SFN. The numbers in italics are the cross-estimated, calculated using the presented method. The p-value is computed using a binomial test for a given probability and two different distributions.
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