Table 3.

Comparison assuming the ΛCDM cosmological model of the CMB measurement of the sound horizon rd and the direct measurement of the Hubble constant H0 with extrapolations from BAO and SN data. The * denotes the case where rd is a derived parameter depending on the densities of matter, baryon and radiation. In this case, we fix the baryon and radiation densities to their best-fitting Planck values.

Data setrd (Mpc)H0 (km s−1 Mpc−1)
Planck+WP147.49 ± 0.59
Riess73.0 ± 2.4
BAO+SN+H0137.0 ± 5.072.9 ± 2.4
BAO+SN+rd147.5 ± 0.667.7 ± 1.1
BAO+SN*145.5 ± 5.968.6 ± 2.2
BAO+H0132.1 ± 5.772.6 ± 2.4
BAO+rd147.5 ± 0.664.7 ± 2.2
SN+H0149 ± 1773.0 ± 2.4
SN+rd147.5 ± 0.669.9 ± 0.8
BAO*124 ± 1477.0 ± 6.6
SN*162 ± 27Unconstrained
Data setrd (Mpc)H0 (km s−1 Mpc−1)
Planck+WP147.49 ± 0.59
Riess73.0 ± 2.4
BAO+SN+H0137.0 ± 5.072.9 ± 2.4
BAO+SN+rd147.5 ± 0.667.7 ± 1.1
BAO+SN*145.5 ± 5.968.6 ± 2.2
BAO+H0132.1 ± 5.772.6 ± 2.4
BAO+rd147.5 ± 0.664.7 ± 2.2
SN+H0149 ± 1773.0 ± 2.4
SN+rd147.5 ± 0.669.9 ± 0.8
BAO*124 ± 1477.0 ± 6.6
SN*162 ± 27Unconstrained
Table 3.

Comparison assuming the ΛCDM cosmological model of the CMB measurement of the sound horizon rd and the direct measurement of the Hubble constant H0 with extrapolations from BAO and SN data. The * denotes the case where rd is a derived parameter depending on the densities of matter, baryon and radiation. In this case, we fix the baryon and radiation densities to their best-fitting Planck values.

Data setrd (Mpc)H0 (km s−1 Mpc−1)
Planck+WP147.49 ± 0.59
Riess73.0 ± 2.4
BAO+SN+H0137.0 ± 5.072.9 ± 2.4
BAO+SN+rd147.5 ± 0.667.7 ± 1.1
BAO+SN*145.5 ± 5.968.6 ± 2.2
BAO+H0132.1 ± 5.772.6 ± 2.4
BAO+rd147.5 ± 0.664.7 ± 2.2
SN+H0149 ± 1773.0 ± 2.4
SN+rd147.5 ± 0.669.9 ± 0.8
BAO*124 ± 1477.0 ± 6.6
SN*162 ± 27Unconstrained
Data setrd (Mpc)H0 (km s−1 Mpc−1)
Planck+WP147.49 ± 0.59
Riess73.0 ± 2.4
BAO+SN+H0137.0 ± 5.072.9 ± 2.4
BAO+SN+rd147.5 ± 0.667.7 ± 1.1
BAO+SN*145.5 ± 5.968.6 ± 2.2
BAO+H0132.1 ± 5.772.6 ± 2.4
BAO+rd147.5 ± 0.664.7 ± 2.2
SN+H0149 ± 1773.0 ± 2.4
SN+rd147.5 ± 0.669.9 ± 0.8
BAO*124 ± 1477.0 ± 6.6
SN*162 ± 27Unconstrained
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