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Fig. 2.
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Posterior probability distributions from the Bayesian approach of H0, Ωm, Ωde, and w in an open-wCDM model, assuming a total, relative uncertainty of 5% for both cosmological probes (with fixed zd = 0.54, zs = 1.49, and zSNIa = 0.54). The colour-coding and shown statistical quantities are as in Fig. 1.
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