What were the main difference of the wants between H0 and Bao​

Wthat these components provide significantly different constraints and could provide strong diagnostics for model selection, also in view of more precise data to arrive. For instance, in the  model we find a mild tension of  for the Ωm estimates obtained using DV and AP separately. Considering both Ωk and w as free parameters, we find that the concordance model is in tension with the best-fit values provided by the BAO data alone a. We complemented the BAO data with the Supernovae Ia () and Observational Hubble datasets to perform a joint analysis on th model and its standard ex- tensions. By assuming M scenario, we find that these data provide H0 7 km/s Mpc−1 as the best-fit value for the present expansion rate. In the kΛCDM scenario we find that the evidence for acceleration using the BAO data alone is more than ∼ 5.8σ, which increases to 8.4σ in our joint analysis. sorry if this dosent help

Explanation:

“a committee reviews the bill and marks it up to make it more viable and to reflect interests