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Fig. 8.
Posterior distribution of the parameters obtained by fitting the model in 3 to BB power spectra of S-PASS, Planck and WMAP in the multiple bin at ℓ ≃ 50 and for the isolatitude mask with |b| > 35°. The fit has been computed by applying a Gaussian prior on the synchrotron spectral index with βs = −3.13 ± 0.13.
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