Table 3.
Fitting results for the halo model, with the mean halo mass ⟨m⟩mle, the scatter in host halo mass σ log m, the mass scale where 50% of halos host a galaxy mth, the normalisation factor for the satellite galaxies m1 and its slope β, and the goodness-of-fit value 
with 12 degrees of freedom.
| Plot colour |
||||
|---|---|---|---|---|
| Blue | Red | Green | Magenta | |
| zd | 0.41 | 0.41 | 0.62 | 0.62 |
| αd | 0.67 | 0.67 | 1.57 | 1.57 |
| αs | 0.58 | 1.75 | 0.58 | 1.75 |
| ⟨m⟩mle in 1013 h−1 M⊙ | 2.45 | 2.46 | 2.58 | 2.60 |
| σ log m | 0.28 | 0.28 | 0.28 | 0.30 |
| mth in 1011 h−1 M⊙ | 2.24 | 2.26 | 4.15 | 4.19 |
| β | 1.08 | 1.09 | 1.06 | 1.05 |
| m1 in 1012 h−1 M⊙ | 7.70 | 7.68 | 11.54 | 11.92 |
 |
1.52 | 1.84 | 1.10 | 1.25 |
Notes. The lens and source redshifts, and local slopes αd, s are chosen as in Fig. 8, the source redshift zs is 0.99. The fit values for identical lens redshifts are expected to be very similar.
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