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Fig. 15.

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Posterior distributions for the cosmological parameters from PR4 for HiLLiPoP (using different sky fractions labelled L, XL, and XXL) and CamSpec, as compared to Planck 2018 (Plik PR3). Likelihoods are considered for the combination of TT+TE+EE, with lowT and lolE used at low .

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