Marginalised posteriors distributions from the analysis of the WL and Recomb data sets. The Recomb data set is composed of data points for θ^*, A_s, and n_s which are inferred via marginalisation of the fiducial Planck posteriors (Planck Collaboration VI 2020) over the remaining cosmological parameters, as described in Section 3.4. Each panel shows the posterior resulting from a separate analysis of Recomb (green) and weak lensing (black) data sets as well as the combination of both data sets (red). Additionally, we show the Planck 2018 contours for reference (blue).