Table 2.
Fraction of galaxies with probability of being in a filament close to 0 or 1 and with different visit map thresholds (vmt).
| vmt | Probability threshold |
|||||
|---|---|---|---|---|---|---|
| 0.001 | 0.01 | 0.02 | 0.05 | 0.1 | 0.317 | |
| 0.03 | 0.19 0.38 0.19 | 0.23 0.46 0.23 | 0.26 0.51 0.25 | 0.30 0.58 0.28 | 0.35 0.67 0.32 | 0.48 0.88 0.40 |
| 0.05 | 0.20 0.38 0.18 | 0.25 0.47 0.22 | 0.28 0.52 0.24 | 0.33 0.60 0.27 | 0.38 0.68 0.30 | 0.51 0.89 0.38 |
| 0.08 | 0.26 0.44 0.18 | 0.30 0.51 0.21 | 0.33 0.56 0.23 | 0.37 0.63 0.26 | 0.43 0.72 0.29 | 0.54 0.90 0.36 |
| 0.12 | 0.30 0.47 0.17 | 0.36 0.56 0.20 | 0.38 0.60 0.22 | 0.43 0.67 0.24 | 0.48 0.75 0.27 | 0.57 0.91 0.34 |
Notes. Directional strength threshold was dst = 0.8 for every run, the visit map threshold for each is shown in the vmt column, the commonly used value is vmt = 0.05. The probability threshold shows the maximum difference, which is considered “close” to 0 or 1. These sizes correspond to a galaxy being classified the same in 99.9%, 99%, 98%, 95%, 90%, and 68.3% of runs. Each cell in the table first shows the fraction of galaxies with probability close to 0 (in small font), next the sum of the fractions with probabilities close to both 0 and 1, and then the fraction of galaxies with probability close to 1 (in small font). Majority of the galaxies have either a very low or very high probability being inside a filament.
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