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Table 2.

Properties of the supercluster boxes and of the galaxy systems detected inside them using the GSyF algorithm.

SCl ID V N d = N/V dsurf = N/A dbas Ngal f NHC NFoG
 Rvir σv
(MSCC) [10 Mpc3] (DR13) [ Mpc−3] [deg−2] [deg−2] di >  dbas Nj ≥ 3 Nmem <  10 Nmem ≥ 10 [ Mpc] [km s−1]
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11) (12) (13)
55 0424.3 812 0.0019 77.6 8.3 468 27 57 011 005 1.1–2.4 245–806
72 0549.7 1941 0.0035 232.0 22.1 1341 18 228 030 022 0.9–2.4 184–689
75 0854.6 1607 0.0019 95.8 22.6 877 15 69 009 007 1.5–3.4 335–1144
76 2628.3 2617 0.0010 110.1 26.6 1536 27 204 014 011 1.3–3.6 214–1051
175 0577.4 2504 0.0043 116.3 25.8 1315 6 172 022 010 1.2–2.7 220–735
184 0692.9 2101 0.0030 70.5 20.7 1003 3 137 010 009 1.4–2.7 278–739
211 0814.7 1484 0.0018 28.6 11.5 654 6 53 002 003 1.9–2.1 406–496
219 0628.4 1913 0.0030 118.2 19.5 1273 6 175 013 010 1.4–3.7 292–1151
222 0955.9 1865 0.0020 97.3 20.3 885 3 123 010 008 1.3–4.1 245–1207
223 0777.0 776 0.0010 302.7 13.8 247 3 45 001 003 2.1–2.1 475–475
229 1352.4 1855 0.0014 45.2 22.3 745 3 106 006 002 2.2–2.2 498–498
236 0643.6 8636 0.0134 52.9 10.3 4733 3 309 093 073 0.5–1.8 105–703
238 3861.8 8328 0.0022 74.4 20.3 4860 6 832 038 074 0.7–4.0 112–1293
248 0690.1 1263 0.0018 72.4 17.4 564 3 75 005 002 1.7–2.8 366–730
264 0923.7 1704 0.0018 59.6 24.5 626 3 105 011 012 1.3–3.5 245–1026
266 0458.5 958 0.0021 49.5 28.8 318 3 55 006 003 1.6–3.1 320–823
272 0138.4 1379 0.0100 135.3 28.0 654 3 87 010 005 1.1–2.4 219–699
277 0905.3 2748 0.0030 76.0 20.2 1329 6 179 0017 009 1.4–2.5 278–675
278 0459.3 7920 0.0172 52.3 10.3 4116 6 222 080 035 0.5–1.9 112–711
283 1478.8 2320 0.0016 70.3 20.2 1379 12 239 010 017 1.5–3.4 295–907
295 0535.5 14 308 0.0267 48.5 7.2 7422 6 272 114 046 0.4–2.0 74–909
310 1558.8 12 286 0.0079 76.9 15.7 7529 6 1015 116 139 0.8–3.0 140–1182
311 0958.8 5270 0.0055 91.8 22.4 3050 6 416 048 040 0.8–2.4 131–704
314 0091.9 558 0.0061 135.2 27.0 289 3 49 010 004 1.2–2.3 254–659
317 0438.6 840 0.0019 104.2 38.2 433 6 76 010 005 1.8–3.3 366–929
323 1909.6 3330 0.0017 77.3 21.7 1764 6 304 017 021 1.5–3.7 295–1069
333 0445.5 1968 0.0044 65.1 22.6 793 3 135 014 027 1.1–2.9 221–949
335 0574.5 3099 0.0054 62.2 21.4 1285 3 211 029 038 0.8–3.0 144–973
343 0427.9 2679 0.0063 105.8 19.2 1526 6 196 023 025 0.8–2.4 131–675
360 0657.7 2199 0.0033 80.1 15.3 934 12 160 015 016 1.3–2.5 253–653
386 0535.9 3256 0.0061 54.9 17.2 1600 9 257 033 040 1.0–2.7 211–852
407 0800.0 1126 0.0014 48.9 22.8 481 12 79 005 005 1.5–4.0 280–1184
414 1245.9 10 902 0.0088 93.0 23.1 6366 6 1066 144 161 0.8–3.2 140–1191
419 0497.6 1723 0.0035 91.7 19.7 1103 6 196 025 020 1.2–3.3 211–976
422 0884.6 1065 0.0012 41.9 24.2 382 3 62 002 006 2.1–2.3 474–526
430 0437.0 1603 0.0037 88.6 22.9 871 3 121 020 009 1.3–2.4 281–647
440 1017.1 3442 0.0034 99.4 72.9 917 6 143 024 014 1.5–3.3 309–935
441 0516.1 1058 0.0021 60.8 20.9 425 6 59 002 003 3.0–3.0 796–796
454 0389.0 5704 0.0147 99.7 18.9 3231 6 524 084 106 0.7–1.9 142–610
457 0529.6 4072 0.0077 129.0 22.7 2605 6 443 058 044 1.0–3.1 187–1038
460 1041.1 3499 0.0034 108.4 27.3 1925 3 335 035 023 1.3–3.6 238–1073
463 0959.2 8466 0.0088 121.6 22.4 5278 3 898 113 113 0.6–3.1 103–1077
474 0343.8 7424 0.0216 109.2 15.3 4506 9 166 064 026 0.6–2.6 122–1115
484 0805.0 1319 0.0016 43.1 19.2 571 6 86 005 004 2.3–3.0 536–793
579 0658.9 1477 0.0022 142.9 1.2 1234 3 149 019 0023 0.6–1.9 128–659
586 0962.1 373 0.0004 18.3 13.6 72 3 8 000 000 −99.0 to −99.0 −99 to −99

Notes. The value −99 is set when GSyF does not detect systems. The columns in the table are as follows: (1) ID of the supercluster in MSCC; (2) supercluster box volume; (3) number of galaxies inside this volume; (4) mean volume number density inside the box; (5) mean surface (sky projected) number density of the box; (6) baseline density of the box; (7) number of galaxies with surface density above the baseline density; (8) used segmentation parameter f; (9) number of HC groups (see Sect. 3.2 for details); (10) remaining groups, after FoG correction, with richness between 5 and 9 galaxies; (11) remaining groups, after FoG correction, with richness higher or equal to 10 galaxies; (12) range of radii for the Nmem ≥ 10 FoG groups; (13) range of velocity dispersions for the Nmem ≥ 10 FoG groups.

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