Table 1.
Results of the binned DM fraction. For binning, the objects are first sorted into ascending stellar masses.
| Bin | NObj |  |
 |
 |
 |
 |
|---|---|---|---|---|---|---|
| No. | [dpts] | [M⊙] | ||||
| 1 | 50 | 9.59 |
0.84 |
0.79 |
0.73 |
0.71 |
| 2 | 50 | 9.89 |
0.84 |
0.76 |
0.70 |
0.75 |
| 3 | 50 | 10.12 |
0.84 |
0.73 |
0.66 |
0.66 |
| 4 | 50 | 10.35 |
0.86 |
0.65 |
0.65 |
0.62 |
| 5 | 27 | 10.59 |
0.90 |
0.43 |
0.30 |
0.40 |
Notes. Then affine binning is performed and 50 objects are allowed per bin. There are a total of 227 objects, so the final bin contains only 27 objects. To perform the binning, RMS statistics and the errors estimated from bootstrap iterations are used. Column 1: Bin number; Col. 2: number of objects (or data points) per bin; Col. 3: binned stellar masses and their errors showing the minimum and maximum boundaries of each bin, lower and upper bounds respectively; Col. 4: binned redshift; Cols. 5–7: binned DM fraction within Rout, Ropt, and Re, respectively. Here 1σ errors are given for each data point (except stellar masses). A catalogue of the individual quantities is published along with this table; see Table D.1.
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