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Table 3.
Number of X-ray AGNs and sources in the control sample for different morphologies and cosmic environments.
| Field | Filament | Cluster | ||||
|---|---|---|---|---|---|---|
| Morphology | BD | Non-BD | BD | Non-BD | BD | Non-BD |
| No. AGN | 12 (32%) | 21 (57%) | 4 (11%) | |||
| AGN | 6(50%) | 6(50%) | 3(14%) | 18(86%) | 0(0%) [0(0%)] | 4(100%) [13(100%)] |
| Dn4000, Hδ (AGN) | 1.58, 5.00 | 1.40, 4.54 | 1.63, 2.58 | 1.42, 3.43 | nan, nan | 1.47, 4.98 |
| No. galaxies | 494(41%) | 560(53%) | 72(7%) [218] | |||
| Galaxies | 87(19%) | 367(81%) | 121(22%) | 439(78%) | 20(28%) [62(28%)] | 52(72%) [156(72%)] |
| Dn4000, Hδ (galaxies) | 1.67, 1.23 | 1.32, 5.03 | 1.76, 0.64 | 1.38, 4.19 | 1.80, −0.04 | 1.40, 3.62 |
Notes. The median Dn4000 and Hδ values of each subset are also presented. The numbers in the square brackets show the number of AGNs when we classified sources using their overdensity values (see text for more details).
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