Table 3.
Properties of the Perseus-Pisces SC and the SGW constructed with a minimum linking length of 19 Mpc.
| Name | NCL | wNCL | Volume | Cl. mass | Est. mass | Length | ⟨z⟩ | zmin | zmax | Density | RCL | RDM |
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| (105 Mpc3) | (1014 M⊙) | (1015 M⊙) | (Mpc) | (10−4 Mpc−3) | ||||||||
| PP | 22 | 58.3 | 2.9 | 35.8 | 24.9 | 115.7 | 0.0205 | 0.0147 | 0.0314 | 2.0 | 2.8 | 2.1 |
| PPin | 20 | 49.0 | 2.8 | 31.6 | 21.5 | 115.7 | 0.0195 | 0.0147 | 0.0300 | 1.8 | 2.4 | 1.9 |
| PPcore | 13 | 30.4 | 1.5 | 27.8 | 12.9 | 63.4 | 0.0176 | 0.0147 | 0.0210 | 2.1 | 2.9 | 2.2 |
| SGW | 7 | 14.6 | 1.1 | 5.0 | 6.8 | 45.8 | 0.0202 | 0.0171 | 0.0243 | 1.4 | 1.9 | 1.6 |
Notes. For the Perseus-Pisces SC we provide values for three different extensions: PP = full SC, PPin = structure at z ≤ 0.03, and PPcore = core region. The columns give (from left to right) NCL and wNCL (the number of members and the weighted number of members, respectively); the SC volume; cl. mass (the sum of the estimated masses of the member clusters); est. mass and length (the estimated SC mass and its extent); ⟨z⟩, zmin, and zmax (the mean, minimum, and maximum redshift); the number density of clusters in the SC; RCL and RDM (the overdensity ratio of the cluster number density and matter density in the SC compared to the cosmic mean, respectively).
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