Posterior distributions of the cosmological parameters under the ΛDDM2 model, log₁₀Γ, log₁₀ε, S₈, σ₈, and Ω_m with 68% and 95% confidence interval contours obtained from our cosmological analysis, when only the Planck CMB data are used (gray) and the Planck CMB data are combined with the BAO + SNIa + SZ data (red). The latest result with the SZ power spectrum from T22 is shown in blue. We note that only Ω_m and σ₈ parameters are varied in T22, while the six ΛCDM cosmological parameters are varied in our analysis as shown in Table. 1.