Notes. Uniformly distributed priors on the parameters used in our cosmological inferences. The priors given in Table 1 on the multiplicative shear m-bias and photometric redshift errors δ⟨z⟩ are used both for the real data analysis and for the mock data analysis, where for the latter the expectation values are set to zero. The δ⟨z⟩ for the sources follow a joint normal distribution with covariance matrix C_δ⟨z⟩ shown in Fig. 6 of H21. The m-bias follows an uncorrelated normal distribution. We increased the upper prior range on Ω_m to 0.75 for the real data analysis to have E_n posteriors that are not bound by the prior. The A_IA of the real data analysis are narrower to improve the emulator accuracy. The upper bound of A_ba is chosen arbitrarily and does play a role only for -only analysis.