Table 3.
Number densities of observed Local Universe giants and general RGs relative to their cosmic means.
| Cluster | Filament | Sheet | Void | |
|---|---|---|---|---|
| environment | environment | environment | environment | |
| GRGs | 15 ± 2 | 2.4 ± 0.1 | 0.29 ± 0.04 | 0.06 ± 0.04 |
| RGs | 10.6 ± 0.6 | 2.41 ± 0.05 | 0.39 ± 0.02 | 0.08 ± 0.02 |
Notes. These numbers depend on environment class definitions and the scale to which the Cosmic Web density field is smoothed; in this case, we use the T-web classification scheme and a smoothing scale of 2.9 Mpc h−1. Clusters and filaments are (giant) radio galaxy overdense; sheets and voids are underdense.
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