Comparison of cosmological parameters estimated from the TT and EE spectra computed from the foreground-cleaned CMB maps. The labels on the horizontal axis give the spectrum and the ℓ_max used to obtain each set of results. The black points show the parameters obtained from the frequency map-based Plik likelihood using the same spectrum and ℓ_max. For comparison, we also show the values of the parameters obtained with the full Planck 2015 likelihood (including multipoles up to ℓ_max = 2500) as the horizontal line surrounded by a grey band giving the uncertainties. The foreground model used for the CMB maps is the method-tailored full-sky model from the FFP8 simulations in TT and a single D_ℓ ∝ ℓ² template in EE.