Open Access
Fig. 12.
One and two standard deviation constraints on H0 and Ωmh2 derived from BAO data used in Fig. 11 and from Big-Bang Nucleosynthesis. This figure assumes a flat universe and a Gaussian prior 100Ωbh2 = 2.260 ± 0.034 derived from the deuterium abundance measurement of Cooke et al. (2018).
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