Table 2
Results of the KS test (the pKS-values): comparison of the galaxy properties in filament- and spider-type superclusters of different overall shape and richness.
| (1) | (2) | (3) | (4) | (5) |
|
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| More elongated and less elongated superclusters | ||||
|
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| Filaments | Spiders | |||
|
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| flux-lim | vol-lim | flux-lim | vol-lim | |
| p KS | p KS | p KS | p KS | |
|
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| g − r | 0.515 | 0.735 | 0.331 | 0.107 |
| p l | 0.099 | 0.535 | 0.003 | 0.011 |
| log Ms | < 1e − 5 | 0.153 | 0.524 | 0.350 |
| SFR | 0.242 | 0.221 | 0.001 | 0.002 |
|
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| The richest superclusters | ||||
|
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| Filaments | Spiders | |||
| SCl 001, SCl 027 | SCl 019, SCl 099 | |||
|
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| flux-lim | vol-lim | flux-lim | vol-lim | |
| p KS | p KS | p KS | p KS | |
|
|
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| g − r | < 1e − 5 | < 1e − 5 | 0.824 | 0.804 |
| p l | < 1e − 5 | < 1e − 5 | 0.001 | 0.127 |
| log Ms | < 1e − 5 | 0.063 | 0.012 | < 1e − 5 |
| SFR | 0.001 | 0.003 | 0.003 | 0.079 |
| D 8 | < 1e − 5 | < 1e − 5 | < 1e − 5 | < 1e − 5 |
Notes. Columns are as follows: 1: Galaxy properties. g − r – colour index, pl – probability of being a late type, log Ms – log stellar mass, SFR – log SFR, D8 – environmental density at 8 h-1 Mpc scale smoothing scale; 2–5: the pKS-value of the test.
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