Table 1
Data of individual superclusters in the SGW.
(1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) | (11) | (12) |
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No. | Name | ID | N gal | N 1 |
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Dist. | Diam. | D8max | Vol. | L tot |
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1 | SCl 027 | 202-001+008 | 3222 | 706 | 381 | 50 | 255.6 | 107.0 | 14.0 | 25.9 | 51.6 |
2 | SCl 019 | 184+003+007 | 2060 | 456 | 274 | 33 | 230.4 | 56.4 | 15.0 | 14.4 | 29.2 |
3 | SCl 0499 | 168+002+007 | 408 | 60 | 26 | 7 | 227.7 | 34.1 | 7.5 | 2.0 | 4.77 |
4 | SCl 0319 | 159+004+006 | 245 | 30 | 23 | 3 | 206.2 | 21.4 | 7.5 | 1.4 | 2.16 |
5 | SCl 1109 | 157+003+007 | 120 | 4 | 5 | 3 | 219.2 | 12.1 | 5.2 | 0.2 | 1.49 |
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SGW | 6055 | 1256 | 709 | 96 | 43.9 | 89.22 |
Notes. Columns are as follows: (1) the order number of the supercluster; (2) the number of the supercluster in Liivamägi et al. (2012); (3) the supercluster ID AAA+BBB+ZZZ, where AAA is RA, +/–BBB is Dec, and ZZZ is 100z; (4) the number of galaxies in the supercluster, Ngal; (5) the number of single galaxies in the supercluster, N1; (6) the number of groups with 2 − 9 member galaxies, ; (7) the number of groups with ≥10 member galaxies,
; (8) the distance of the supercluster (the distance of the density maximum in the supercluster), in h-1 Mpc; (9) the supercluster diameter (the maximum distance between galaxies in the supercluster), Diam, in h-1 Mpc; (10) the highest value of the luminosity-density field calculated with the 8 h-1 Mpc smoothing kernel, D8max, in units of the mean luminosity density; (11) the volume of the supercluster (the number of connected 3D grid cells in the luminosity density field, multiplied by the cell volume, V), in 103 (h-1 Mpc)3; (12) the total luminosity of the supercluster, calculated as the weighted total luminosity of galaxies in the supercluster, Ltot, in 1012h-2L⊙.
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