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Table 2
Slopes of the linear fits plotted in the panels of Fig. 10.
| Mass range | 0.1 ≤ z ≤ 0.5 | 0.5 ≤ z ≤ 0.7 | 0.7 ≤ z ≤ 1.0 | |||
| Slope ± 1σ | Nvr/Ntot | Slope ± 1σ | Nvr/Ntot | Slope ± 1σ | Nvr/Ntot | |
|
|
||||||
| 10.25–10.45 | 0.26 ± 0.07 | 101/230 | – | – | – | – |
| 10.45–10.65 | 0.18 ± 0.07 | 101/187 | – | – | – | – |
| 10.65–10.85 | 0.17 ± 0.10 | 99/174 | 0.13 ± 0.10 | 65/131 | – | – |
| 10.85–11.05 | 0.03 ± 0.08 | 83/124 | −0.08 ± 0.12 | 50/109 | – | – |
| 11.05–11.25 | 0.41 ± 0.12 | 33/51 | −0.03 ± 0.16 | 33/59 | 0.06 ± 0.11 | 42/116 |
Notes. Different rows are for the different mass ranges, and the columns for the three redshift bins. Nvr is the number of “very red” galaxies, and Ntot the total number of galaxies in each panel.
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