Fig. 42
Marginal mean and 68% CL error bars on cosmological parameters estimated with different multipoles for the transition between the low-ℓ and the high-ℓ likelihood. Here we use only the TT power spectra and a Gaussian prior on the optical depth τ = 0.07 ± 0.02, within the base-ΛCDM model. “Plik TT+tauprior” refers to the case where we use the Plik high-ℓ likelihood only.
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