Marginal posterior distributions for a subset of the cosmological, nuisance, and derived parameters used in our cosmological model. Coloured lines represent the marginal distributions from various samples. Dashed lines show the priors for all non-derived parameters. There is a clear difference between the marginal distributions of the gold and full-sample (‘KV450-DIR’) analyses. We note in particular that the previously observed preference within KV450 for small values of the matter density parameter Ω_m is removed in our gold analyses. The gold analyses also prefer a lower value of A_IA, consistent with 0 in all cases.