Notes. Columns in the table are as follows: (1) SCl_ID: the supercluster ID in the L10 catalogue; (2) the distance of the density maximum, d_peak; (3) the number of galaxies in the supercluster, N_gal; (4) the number of groups with at least 30 member galaxies in the supercluster, N₃₀; (5) the number of Abell clusters among groups with at least 30 member galaxies in the supercluster, N_Abell; (6) the maximum value of the fourth Minkowski functional, (V_3,max (clumpiness), for the supercluster; (7) classification: set – 1 for superclusters with the ratio of the shapefinders K₁/K₂ < 0.6 and 2 for superclusters with the ratio of the shapefinders K₁/K₂ ≥ 0.6); (8) morphology: S denotes spiders, mS – multispiders, F – filaments and mF – multibranching filaments; (9) notes. SGW denotes members of the Sloan Great Wall; F(L11) denotes a filamentary system according to (Luparello et al. 2011); T denotes superclusters for which at a certain mass fraction V₃ = 0, suggesting that these superclusters have tunnels through them (Appendix B, Einasto et al. 2011). Her-DSP denotes the superclusters located in a chain of superclusters that connects the Hercules supercluster with the dominant supercluster plane, and SGW chain denotes the superclusters in a chain in the foreground of the Sloan Great Wall.