Table 1.
Properties of the superstructures found in the present study.
| Name | NCl | ⟨z⟩ | z-range | RA | Dec | length | Mest | ΔCl | ΔDM |
|---|---|---|---|---|---|---|---|---|---|
| 1. Quipu | 68 (63) | 0.043 | 0.027 – 0.065 | 27.7–119.4 | −69.8–51.7 | 428 | 2.4 | 1.4 | 0.5 |
| 2. Shapley | 23 (23) | 0.049 | 0.038 – 0.056 | 193.1–213.1 | −44.1–−27.2 | 90 | 0.8 | 3.8 | 1.3 |
| 3. Ser-CorBor | 34 (23) | 0.056 | 0.035 – 0.078 | 214.4–257.8 | −3.5–39.7 | 234 | 1.8 | 2.7 | 0.9 |
| 4. Hercules | 28 (19) | 0.032 | 0.024 – 0.046 | 234.9–279.0 | −1.8–68.1 | 154 | 0.6 | 0.7 | 0.3 |
| 5. Scu-Peg | 32 (27) | 0.047 | 0.037 – 0.065 | 345.3–30.6 | −31.6–20.3 | 216 | 1.3 | 2.1 | 0.7 |
Notes. NCl is the number of cluster members, the numbers in brackets give the number of members inside z = 0.03 − 0.06, ⟨z⟩ is the mean redshift, the length is in units of Megaparsec, Mest is the estimated supercluster mass in units of 1017 M⊙, ΔCl and ΔDM are the cluster and matter overdensity. The numbering that appears with the name of the superstructures is used for the labelling of the figures throughout the paper.
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