Table 1
Basic information on the main superclusters in the BGW supercluster system and the whole system.
| Supercluster | Richness | Diameter | Volume | Average density | Maximum density | log (M1) | log (M2) |
| Ngal | h-1 Mpc | (h-1 Mpc)3 | ⟨ ρL ⟩ | ⟨ ρL ⟩ | log (h-1 M⊙) | log (h-1 M⊙) | |
|
|
|||||||
| A | 255 | 186.1 | 67500 | 9.1 | 27.9 | 16.8 | 16.9 |
| B | 303 | 172.9 | 70848 | 9.3 | 29.6 | 16.6 | 16.9 |
| C | 73 | 63.8 | 19008 | 10.2 | 24.5 | 16.3 | 16.4 |
| D | 71 | 90.6 | 13635 | 9.3 | 21.2 | 16.0 | 16.2 |
|
|
|||||||
| Total | 830 | 271.1 | 241029 | 8.6 | 29.6 | 17.2 | 17.4 |
Notes. The line “Total” refers to the over-dense region found with the threshold of D> 5 mean densities. The individual superclusters in the BGW are found with the threshold D> 6. The two mass estimates are the mass derived from the stellar masses (log (M1)) and the mass derived from the critical density (log (M2)).
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