Comparison of cosmological parameters estimated from the TT and EE spectra computed from the CMB maps and further accounting for foreground residuals through method-tailored templates derived from the FFP8 simulations. The sets of points correspond to various values of ℓ_max, and lets the four methods and Plik to be compared when the same scales are used. For comparison, we also show the corresponding parameters obtained with the Planck 2015 likelihood including multipoles up to ℓ_max = 2500 as the horizontal line surrounded by a grey band giving the uncertainties.