DE component with increasing w: the DES-Y3 CPL model with w₀ = −0.95 and w_a = −0.4 (magenta) compared to ΛCDM (blue), both computed with our scheme. Panels on the left-hand column were computed using the early parametrization of H₀ = 67.56 km s⁻¹ Mpc⁻¹ using Planck Collaboration VI (2020), while panels on the right-hand column employ the local parametrization of H₀ = 73.04 km s⁻¹ Mpc⁻¹ from Riess et al. (2022). Top panels: expansion histories; for the vertical lines in red see Fig. 7. We note the deviations in the expansion histories from ΛCDM at late times (respective high scale factors) and the different run of these deviations (see gray curves in the bottom insets of the top panels). Middle panels: CMB temperature spectra. Bottom panels: matter power spectra. The results based on the CMB-determined H₀, shown in the left-hand column, display a clear deviation from ΛCDM, whereas the results based on the locally determined H₀ are in better agreement with ΛCDM.