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Table 3.
Data points of the SMFs measured in this work.
| Cluster <1000 kpc | Cluster <500 kpc | Field | |||||||
|---|---|---|---|---|---|---|---|---|---|
| Φ [cluster−1 dex−1] |
Φ [cluster−1 dex−1] |
Φ [10−5 Mpc−3 dex−1] |
|||||||
| log[M⋆/M⊙] | All | Quiescent | Star-forming | All | Quiescent | Star-forming | All | Quiescent | Star-forming |
| 9.55 | − | − |
 |
− | − |
 |
478.4 ± 15.1 | 32.9 ± 4.1 | 445.4 ± 14.5 |
| 9.65 | − | − |
 |
− | − |
 |
452.6 ± 10.1 | 32.8 ± 2.8 | 419.8 ± 9.7 |
| 9.75 |
 |
 |
 |
 |
 |
 |
369.7 ± 8.1 | 32.1 ± 2.4 | 337.6 ± 7.7 |
| 9.85 |
 |
 |
 |
 |
 |
 |
379.3 ± 8.2 | 41.3 ± 2.7 | 338.0 ± 7.7 |
| 9.95 |
 |
 |
 |
 |
 |
 |
326.2 ± 7.6 | 53.3 ± 3.1 | 272.9 ± 6.9 |
| 10.05 |
 |
 |
 |
 |
 |
 |
282.2 ± 7.0 | 54.5 ± 3.1 | 227.7 ± 6.3 |
| 10.15 |
 |
 |
 |
 |
 |
 |
298.4 ± 7.2 | 68.0 ± 3.5 | 230.4 ± 6.3 |
| 10.25 |
 |
 |
 |
 |
 |
 |
249.4 ± 6.6 | 73.3 ± 3.6 | 176.0 ± 5.5 |
| 10.35 |
 |
 |
 |
 |
 |
 |
267.5 ± 6.8 | 86.2 ± 3.9 | 181.3 ± 5.6 |
| 10.45 |
 |
 |
 |
 |
 |
 |
222.8 ± 6.2 | 80.8 ± 3.7 | 142.0 ± 4.9 |
| 10.55 |
 |
 |
 |
 |
 |
 |
203.4 ± 5.9 | 83.4 ± 3.8 | 119.9 ± 4.5 |
| 10.65 |
 |
 |
 |
 |
 |
 |
202.4 ± 5.9 | 92.4 ± 4.0 | 110.0 ± 4.3 |
| 10.75 |
 |
 |
 |
 |
 |
 |
148.5 ± 5.0 | 77.2 ± 3.6 | 71.2 ± 3.5 |
| 10.85 |
 |
 |
 |
 |
 |
 |
128.3 ± 4.7 | 69.5 ± 3.4 | 58.8 ± 3.2 |
| 10.95 |
 |
 |
 |
 |
 |
 |
85.3 ± 3.8 | 53.4 ± 3.0 | 31.9 ± 2.3 |
| 11.05 |
 |
 |
 |
 |
 |
 |
57.2 ± 3.1 | 39.2 ± 2.6 | 18.0 ± 1.8 |
| 11.15 |
 |
 |
 |
 |
 |
 |
40.6 ± 2.6 | 29.4 ± 2.2 | 11.2 ± 1.4 |
| 11.25 |
 |
 |
 |
 |
 |
 |
16.8 ± 1.7 | 13.1 ± 1.5 | 3.7 ± 0.8 |
| 11.35 |
 |
 |
− |
 |
 |
− | 11.3 ± 1.4 | 10.0 ± 1.3 | 1.4 ± 0.5 |
| 11.45 |
 |
 |
 |
 |
 |
 |
3.9 ± 0.8 | 3.0 ± 0.7 | 0.8 ± 0.4 |
| 11.55 |
 |
 |
− |
 |
 |
− | 2.0 ± 0.6 | 2.0 ± 0.6 | − |
| 11.65 | − | − | − | − | − | − | 0.7 ± 0.3 | 0.5 ± 0.3 | 0.2 ± 0.2 |
| 11.75 | − | − | − | − | − | − | 0.2 ± 0.2 | 0.2 ± 0.2 | − |
Notes. Error bars for the cluster SMFs are based on bootstrap resamplings, where clusters are drawn with replacement as detailed in the text. The quiescent galaxies in the cluster environment are only reliably detected and characterised at stellar masses M⋆ ≥ 109.7 M⊙.
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