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Table 1.

Properties of the superclusters in the local Universe at z ≥ 0.03 constructed with a minimal linking length, l0 = 19 Mpc.

Name NCL wNCL Volume MCL tot Mest Length z zmin zmax nCL RCL RDM
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
A400 7 14.6 1.1 5.0 6.8 45.8 0.0202 0.0171 0.0243 1.4 1.9 1.6
Vir 5 5.0 0.5 2.4 2.5 18.4 0.0044 0.0031 0.0062 1.0 1.4 1.2
Cen 10 11.7 1.0 7.1 5.6 37.1 0.0131 0.0087 0.0160 1.2 1.6 1.4
Coma 13 37.8 2.3 18.9 16.8 78.0 0.0254 0.0202 0.0322 1.7 2.3 1.8
Comain 11 28.8 1.9 16.8 13.0 64.8 0.0242 0.0202 0.0280 1.5 2.1 1.7
Her 24 94.0 3.7 26.0 38.7 141.1 0.0297 0.0236 0.0349 2.6 3.6 2.6
Herin 10 30.6 1.7 6.7 13.4 71.1 0.0270 0.0236 0.0297 1.8 2.5 1.9
Sag 6 11.4 0.9 2.7 5.5 33.8 0.0204 0.0191 0.0246 1.2 1.7 1.4
Lac 6 9.7 0.6 4.4 4.3 19.9 0.0178 0.0169 0.0192 1.7 2.3 1.8

Notes. The superclusters are: PP = Perseus-Pisces SC, A400 = A400 SC, Coma = Coma SC, Vir = Local SC, Cen = Centaurus SC, Her = Hercules SC, Sag = Sagittarius SC, Lac = Lacerta SC. The suffix in designates that part of the supercluster which lies inside ≤0.03, otherwise the redshift constraint was relaxed in the SC construction. NCL is the number of SC members and wNCL the weighted number of members. The SC volume is in units of 105 Mpc3, MCL tot is the sum of the m200 cluster masses in units of 1014M, Mest is the estimated SC mass in units of 1015M and the length is in units of Mpc. The cluster density, nCL is in units of 10−4 Mpc−3 and the overdensity ratios RCL and RDM are defined in the text.

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