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![]() |
(DR13) | [![]() |
[deg−2] | [deg−2] | di > dbas | Nj ≥ 3 | Nmem < 10 | Nmem ≥ 10 | [![]() |
[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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