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Fig. A.3.
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Marginalised 1D and 2D posterior distributions for 68% (darker) and 95% (lighter) C.I. in the cosmological parameter space, comparing the results from the SDSS BAO and RSD (blue) likelihoods we introduce in Sect. 5.2 with the BOSS DR12 likelihood used in the main KiDS-1000 analysis (grey, Sánchez et al. 2017b).
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