Table 1.
Overview of the maximum-posterior cosmologies with the constraining power that we obtain for the original and calibrated model.
| Ωm | σ8 | S8 | |
|---|---|---|---|
| ad. original |
 |
 |
 |
| th. original |
 |
 |
 |
| ad. calibrated |
 |
 |
 |
| th. calibrated |
 |
 |
 |
Notes. For all results we marginalise over the biases b of the lenses. The input cosmology of the fiducial cosmo-SLICS is Ωm = 0.2905, σ8 = 0.8364 and thus 
. We fixed the time-independent equation-of-state parameter of dark energy w0 = −1.0 and Hubble parameter h = 0.6868 to their true values. We note that the parameter uncertainties increase slightly if we also vary parameters like w0, h, or the scalar spectral index ns.
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