Table 1.
Fraction of galaxies in each halo-mass bin for each large-scale environment classification.
| Color | LSS classifications | M200m ∈ 1011.5−12 M⊙ | M200m ∈ 1012−12.5 M⊙ | M200m ∈ 1012.5−13 M⊙ | M200m ∈ 1013−13.5 M⊙ | All M200m ∈ 1011.5−13.5 M⊙ |
|---|---|---|---|---|---|---|
| 28 492 halos | 11 094 halos | 3677 halos | 1113 halos | 44 310 halos | ||
| Cluster outskirts | 8% (2134) | 8% (826) | 8% (296) | 9% (102) | 8% (3358) | |
| Filaments | 12% (3291) | 10% (1090) | 12% (443) | 18% (203) | 11% (5027) | |
| Filament-void transition | 22% (6360) | 20% (2248) | 21% (758) | 20% (222) | 22% (9588) | |
| Voids and walls | 58% (16 646) | 62% (6926) | 59% (2180) | 53% (585) | 59% (26 337) |
Notes. For every halo-mass bin, we present the percentage of objects in cluster outskirts (orange), filaments (green), filament-void transition region (red), and voids and walls (purple) within LC-TNGX (detailed in Sect. ). The M200 m > 1013.5 M⊙ halos, of which there are 517, are defined as massive groups and clusters.
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