Open Access
Table D.3.
Galaxy environment.
| LTG | S0 | Elliptical | Merger | Uncertain | LTG | S0 | Elliptical | Merger | Uncertain | |
|---|---|---|---|---|---|---|---|---|---|---|
| Yang et al. (2007) DPS | NBCS | |||||||||
| isolated | 59.7 % | 68.6 % | 56.3 % | 54.0 % | 63.4 % | 65.7 % | 67.6 % | 47.8 % | 58.1 % | 67.9 % |
| poor group | 24.3 % | 16.6 % | 29.3 % | 25.0 % | 16.0 % | 21.0 % | 15.0 % | 25.4 % | 25.9 % | 13.3 % |
| rich group | 5.0 % | 2.4 % | 6.0 % | 3.6 % | 2.8 % | 4.6 % | 3.9 % | 11.2 % | 3.3 % | 3.4 % |
| cluster | 6.1 % | 2.4 % | 3.0 % | 4.2 % | 3.3 % | 4.5 % | 2.2 % | 10.4 % | 4.5 % | 3.4 % |
| unknown | 4.8 % | 10.1 % | 5.4 % | 13.2 % | 14.5 % | 4.2 % | 11.4 % | 5.2 % | 8.2 % | 12.0 % |
| Yang et al. (2007) (z < 0.11) DPS | NBCS | |||||||||
| isolated | 54.8 % | 65.2 % | 50.9 % | 43.6 % | 62.5 % | 62.8 % | 66.9 % | 39.1 % | 48.3 % | 65.1 % |
| poor group | 28.1 % | 23.0 % | 34.3 % | 33.3 % | 20.2 % | 22.4 % | 20.1 % | 28.7 % | 32.8 % | 15.1 % |
| rich group | 5.1 % | 2.8 % | 8.3 % | 6.7 % | 3.6 % | 5.8 % | 6.1 % | 14.9 % | 5.0 % | 6.0 % |
| cluster | 7.7 % | 4.6 % | 3.7 % | 9.3 % | 6.8 % | 6.2 % | 4.7 % | 13.8 % | 9.5 % | 6.6 % |
| unknown | 4.4 % | 4.4 % | 2.8 % | 7.1 % | 7.0 % | 2.9 % | 2.3 % | 3.4 % | 4.5 % | 7.2 % |
| Saulder et al. (2016) (z < 0.11) DPS | NBCS | |||||||||
| isolated | 38.2 % | 51.1 % | 35.2 % | 36.4 % | 44.0 % | 43.5 % | 48.8 % | 27.6 % | 33.3 % | 45.7 % |
| poor group | 37.0 % | 29.2 % | 38.0 % | 31.1 % | 33.0 % | 32.8 % | 31.7 % | 29.9 % | 38.8 % | 31.1 % |
| rich group | 12.7 % | 9.5 % | 11.1 % | 13.8 % | 9.5 % | 11.1 % | 10.5 % | 20.7 % | 11.4 % | 10.6 % |
| cluster | 10.7 % | 6.7 % | 12.0 % | 8.9 % | 10.0 % | 11.0 % | 8.1 % | 20.7 % | 11.9 % | 9.8 % |
| unknown | 1.5 % | 3.4 % | 3.7 % | 9.8 % | 3.6 % | 1.5 % | 0.9 % | 1.1 % | 4.5 % | 2.8 % |
Notes. Fraction of galaxies in different environments from Yang et al. (2007) and Saulder et al. (2016).
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