Table 1.
Inference on the model parameters.
| Parameter | Truth | Prior | 100 time-delay | With prior | With H0 | Description |
|---|---|---|---|---|---|---|
| lenses | from Paper I | prior | ||||
| H0 | 70 | U(50, 90) |
 |
 |
 |
Hubble constant, in km s−1 Mpc−1 |
| μDM, 0 | 11.04 | U(10, 12) |
 |
 |
 |
Mean log MDM, 5 at log  = 11.4 and |
| average size | ||||||
| βDM | 0.57 | U(0, 3) |
 |
 |
 |
Dependence of log MDM, 5 on  |
| ξDM | −0.15 | U(−1, 1) |
 |
 |
 |
Dependence of log MDM, 5 on galaxy size |
| σDM | 0.05 | U(0.0, 0.5) |
 |
 |
 |
Intrinsic scatter in log MDM, 5 |
| μγ, 0 | 1.47 | U(0, 1) |
 |
 |
 |
Mean γDM at log  = 11.4 and |
| average size | ||||||
| βγ | −0.39 | U(−1, 1) |
 |
 |
 |
Dependence of γDM on log  |
| ξγ | −0.37 | U(−1, 1) |
 |
 |
 |
Dependence of γDM on galaxy size |
| σγ | 0.06 | U(0.0, 0.5) |
 |
 |
 |
Intrinsic scatter in γDM |
| log αsps | 0.10 | U(0.00, 0.25) |
 |
 |
 |
Log of the stellar population synthesis |
| mismatch parameter |
Notes. Column (2): true values of the population parameters. For the parameters relative to the dark matter component, these are defined by fitting the model directly to the distribution of MDM, 5 and γDM. Column (3): priors on the parameters. Columns (4)–(6): median, 16th, and 84th percentile of the marginal posterior probability distribution of each parameter obtained using the sample of 100 time-delay lenses on its own, in combination with a prior on the lens structural parameters from the analysis of Paper I, and in combination with a prior on H0 with 1% precision.
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