Table 1: Data on 2dFGRS and Millennium Run superclusters of various richness.
Name       2dF       Mill  
  Rich N 1st med 4th N 1st med 4th
1 2 3 4 5 6 7 8 9 10
$L_{\rm tot}$ P 365 5.157e11 8.302e11 1.347e12 1432 1.554e12 2.425e12 3.962e12
  M 151 1.526e12 2.583e12 4.267e12 283 6.028e12 1.028e13 1.720e13
  R 18 1.055e13 1.528e13 1.866e13 18 2.695e13 3.852e13 4.278e13
  E 9 2.024e13 4.320e13 4.975e13 1   1.048e14  
$M_{\rm m}$ P   -20.66 -20.94 -21.30   -22.14 -22.44 -22.77
  M   -20.73 -21.02 -21.34   -22.61 -22.87 -23.13
  R   -21.16 -21.45 -21.74   -23.00 -23.20 -23.42
  E   -21.09 -21.31 -21.57     -23.71  
$\delta_{\rm m}$ P   5.07 5.37 5.99   5.03 5.36 5.95
  M   5.42 5.89 6.46   5.57 6.14 6.88
  R   6.25 6.90 7.19   6.45 6.71 7.35
  E   6.91 7.26 7.87     7.35  
$\delta_{\rm p}$ P   5.140 5.780 7.330   5.200 5.930 7.533
  M   5.675 6.740 9.070   5.880 8.190 11.840
  R   8.643 10.400 12.460   10.26 11.72 16.81
  E   11.07 12.29 16.33   11.33 11.33 11.33
$D_{\max}$ P   13.93 17.49 21.95   14.07 18.22 23.69
  M   27.81 34.07 42.61   31.49 41.68 53.00
  R   75.61 84.56 90.48   73.80 85.32 106.30
  E   93.11 126.40 153.90     136.4  
$D_{\rm eff}$ P   7.51 9.58 11.70   7.71 9.87 12.20
  M   12.21 14.82 17.70   13.80 16.66 19.88
  R   24.90 27.10 28.49   23.30 25.96 27.24
  E   29.73 39.44 40.90     36.68  
$\Delta_{\rm o}$ P   2.39 3.41 4.33   1.57 2.55 4.06
  M   5.05 6.59 8.70   5.42 8.27 12.50
  R   13.2 15.2 23.5   13.6 23.49 27.89
  E   15.5 19.2 23.4     26.26  
$\epsilon_0$ P   1.02 1.06 1.12   1.02 1.06 1.15
  M   1.26 1.33 1.49   1.32 1.44 1.58
  R   1.65 1.77 1.83   1.79 1.96 2.13
  E   1.81 1.95 2.22     2.15  
Columns:
1 - Parameter: $L_{\rm tot}$ - supercluster total luminostity; $M_{\rm m}$ - main galaxy absolute magnitude (for 2dF in $b_{\rm j}$, for Mill in g); $\delta_{\rm m}$ and $\delta_{\rm p}$ - supercluster mean and maximum density (in units of the mean density); $D_{\max}$ and $D_{\rm eff}$ - supercluster maximum and effective diameter (in h-1Mpc); $\Delta_0$ - the distance between geometric and dynamic center (in h-1Mpc); $\epsilon_0$ - the ratio of mean to effective diameter; 2 - subcluster richness class: P - poor, M - medium, R - rich, E - extremely rich; 3 and 7 - the number of superclusters in subsamples of various richness for 2dF and Mill samples, respectively; 4, 6, 8 and 10 - 1st and 4th quantiles of distributions; 5 and 9 - median values of parameters.

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