Table 4.
FRs and COM AGN in different environments.
Radio class | Cluster | Filament | Field |
---|---|---|---|
FRII | 10 (46%) | 6 (27%) | 6 (27%) |
FRI/FRII | 4 (36%) | 4 (36%) | 3 (28%) |
FRI | 4 (27%) | 8 (53%) | 3 (20%) |
COM AGN | 84 (23.2%) | 132 (36.5%) | 146 (40.3%) |
Notes. Cross-correlation of the FR and COM AGN samples with Darvish et al. (2015) in respect to different environments (cluster, filament, field). In the parentheses we give the percentage over the total cross-matched number of objects with the same type (within the Darvish environments).
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