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Fig. 17.

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Degeneracies between the 2b-DDM parameter ε and four other cosmological parameters for the optimistic case, in the particular case where f ddm ini = 1 $ f_{\mathrm{ddm}}^{\mathrm{ini}} = 1 $. The addition of Planck data to 3 × 2pt data lifts these degeneracies.

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