Table 2.

68 per cent and 95 per cent confidence level parameter constraints from the MCMC analysis of SN+OHD+BAO data for the fourth-order Taylor, (2,2) Padé and (2,1) rational Chebyshev polynomial approximations of the luminosity distance. H0 values are given in units of km s−1 Mpc−1, while rd values in units of Mpc.

ParameterTaylorPadéRational Chebyshev
MeanMeanMean
H065.80|$^{+2.09}_{-2.11}$||$^{+4.22}_{-4.00}$|64.94|$^{+2.11}_{-2.02}$||$^{+4.12}_{-4.13}$|64.95|$^{+1.89}_{-1.94}$||$^{+3.77}_{-3.77}$|
q0−0.276|$^{+0.043}_{-0.049}$||$^{+0.093}_{-0.091}$|−0.285|$^{+0.040}_{-0.046}$||$^{+0.087}_{-0.084}$|−0.278|$^{+0.021}_{-0.021}$||$^{+0.041}_{-0.042}$|
j0−0.023|$^{+0.317}_{-0.397}$||$^{+0.748}_{-0.685}$|0.545|$^{+0.463}_{-0.652}$||$^{+1.135}_{-1.025}$|1.585|$^{+0.497}_{-0.914}$||$^{+1.594}_{-1.453}$|
s0−0.745|$^{+0.196}_{-0.284}$||$^{+0.564}_{-0.487}$|0.118|$^{+0.451}_{-1.600}$||$^{+3.422}_{-1.921}$|1.041|$^{+1.183}_{-1.784}$||$^{+3.388}_{-3.087}$|
M−19.16|$^{+0.07}_{-0.07}$||$^{+0.14}_{-0.14}$|−19.03|$^{+0.02}_{-0.02}$||$^{+0.05}_{-0.05}$|−19.17|$^{+0.07}_{-0.07}$||$^{+0.13}_{-0.13}$|
ΔM−0.054|$^{+0.023}_{-0.022}$||$^{+0.044}_{-0.045}$|−0.054|$^{+0.022}_{-0.023}$||$^{+0.045}_{-0.045}$|−0.050|$^{+0.022}_{-0.022}$||$^{+0.044}_{-0.045}$|
α0.127|$^{+0.006}_{-0.006}$||$^{+0.012}_{-0.012}$|0.127|$^{+0.006}_{-0.006}$||$^{+0.012}_{-0.012}$|0.130|$^{+0.006}_{-0.006}$||$^{+0.012}_{-0.012}$|
β2.624|$^{+0.071}_{-0.068}$||$^{+0.136}_{-0.140}$|2.625|$^{+0.065}_{-0.069}$||$^{+0.137}_{-0.135}$|2.667|$^{+0.068}_{-0.069}$||$^{+0.137}_{-0.135}$|
rd149.2|$^{+3.7}_{-4.1}$||$^{+7.7}_{-7.5}$|148.6|$^{+3.5}_{-3.8}$||$^{+7.5}_{-7.1}$|147.2|$^{+3.7}_{-4.0}$||$^{+7.8}_{-7.5}$|
ParameterTaylorPadéRational Chebyshev
MeanMeanMean
H065.80|$^{+2.09}_{-2.11}$||$^{+4.22}_{-4.00}$|64.94|$^{+2.11}_{-2.02}$||$^{+4.12}_{-4.13}$|64.95|$^{+1.89}_{-1.94}$||$^{+3.77}_{-3.77}$|
q0−0.276|$^{+0.043}_{-0.049}$||$^{+0.093}_{-0.091}$|−0.285|$^{+0.040}_{-0.046}$||$^{+0.087}_{-0.084}$|−0.278|$^{+0.021}_{-0.021}$||$^{+0.041}_{-0.042}$|
j0−0.023|$^{+0.317}_{-0.397}$||$^{+0.748}_{-0.685}$|0.545|$^{+0.463}_{-0.652}$||$^{+1.135}_{-1.025}$|1.585|$^{+0.497}_{-0.914}$||$^{+1.594}_{-1.453}$|
s0−0.745|$^{+0.196}_{-0.284}$||$^{+0.564}_{-0.487}$|0.118|$^{+0.451}_{-1.600}$||$^{+3.422}_{-1.921}$|1.041|$^{+1.183}_{-1.784}$||$^{+3.388}_{-3.087}$|
M−19.16|$^{+0.07}_{-0.07}$||$^{+0.14}_{-0.14}$|−19.03|$^{+0.02}_{-0.02}$||$^{+0.05}_{-0.05}$|−19.17|$^{+0.07}_{-0.07}$||$^{+0.13}_{-0.13}$|
ΔM−0.054|$^{+0.023}_{-0.022}$||$^{+0.044}_{-0.045}$|−0.054|$^{+0.022}_{-0.023}$||$^{+0.045}_{-0.045}$|−0.050|$^{+0.022}_{-0.022}$||$^{+0.044}_{-0.045}$|
α0.127|$^{+0.006}_{-0.006}$||$^{+0.012}_{-0.012}$|0.127|$^{+0.006}_{-0.006}$||$^{+0.012}_{-0.012}$|0.130|$^{+0.006}_{-0.006}$||$^{+0.012}_{-0.012}$|
β2.624|$^{+0.071}_{-0.068}$||$^{+0.136}_{-0.140}$|2.625|$^{+0.065}_{-0.069}$||$^{+0.137}_{-0.135}$|2.667|$^{+0.068}_{-0.069}$||$^{+0.137}_{-0.135}$|
rd149.2|$^{+3.7}_{-4.1}$||$^{+7.7}_{-7.5}$|148.6|$^{+3.5}_{-3.8}$||$^{+7.5}_{-7.1}$|147.2|$^{+3.7}_{-4.0}$||$^{+7.8}_{-7.5}$|
Table 2.

68 per cent and 95 per cent confidence level parameter constraints from the MCMC analysis of SN+OHD+BAO data for the fourth-order Taylor, (2,2) Padé and (2,1) rational Chebyshev polynomial approximations of the luminosity distance. H0 values are given in units of km s−1 Mpc−1, while rd values in units of Mpc.

ParameterTaylorPadéRational Chebyshev
MeanMeanMean
H065.80|$^{+2.09}_{-2.11}$||$^{+4.22}_{-4.00}$|64.94|$^{+2.11}_{-2.02}$||$^{+4.12}_{-4.13}$|64.95|$^{+1.89}_{-1.94}$||$^{+3.77}_{-3.77}$|
q0−0.276|$^{+0.043}_{-0.049}$||$^{+0.093}_{-0.091}$|−0.285|$^{+0.040}_{-0.046}$||$^{+0.087}_{-0.084}$|−0.278|$^{+0.021}_{-0.021}$||$^{+0.041}_{-0.042}$|
j0−0.023|$^{+0.317}_{-0.397}$||$^{+0.748}_{-0.685}$|0.545|$^{+0.463}_{-0.652}$||$^{+1.135}_{-1.025}$|1.585|$^{+0.497}_{-0.914}$||$^{+1.594}_{-1.453}$|
s0−0.745|$^{+0.196}_{-0.284}$||$^{+0.564}_{-0.487}$|0.118|$^{+0.451}_{-1.600}$||$^{+3.422}_{-1.921}$|1.041|$^{+1.183}_{-1.784}$||$^{+3.388}_{-3.087}$|
M−19.16|$^{+0.07}_{-0.07}$||$^{+0.14}_{-0.14}$|−19.03|$^{+0.02}_{-0.02}$||$^{+0.05}_{-0.05}$|−19.17|$^{+0.07}_{-0.07}$||$^{+0.13}_{-0.13}$|
ΔM−0.054|$^{+0.023}_{-0.022}$||$^{+0.044}_{-0.045}$|−0.054|$^{+0.022}_{-0.023}$||$^{+0.045}_{-0.045}$|−0.050|$^{+0.022}_{-0.022}$||$^{+0.044}_{-0.045}$|
α0.127|$^{+0.006}_{-0.006}$||$^{+0.012}_{-0.012}$|0.127|$^{+0.006}_{-0.006}$||$^{+0.012}_{-0.012}$|0.130|$^{+0.006}_{-0.006}$||$^{+0.012}_{-0.012}$|
β2.624|$^{+0.071}_{-0.068}$||$^{+0.136}_{-0.140}$|2.625|$^{+0.065}_{-0.069}$||$^{+0.137}_{-0.135}$|2.667|$^{+0.068}_{-0.069}$||$^{+0.137}_{-0.135}$|
rd149.2|$^{+3.7}_{-4.1}$||$^{+7.7}_{-7.5}$|148.6|$^{+3.5}_{-3.8}$||$^{+7.5}_{-7.1}$|147.2|$^{+3.7}_{-4.0}$||$^{+7.8}_{-7.5}$|
ParameterTaylorPadéRational Chebyshev
MeanMeanMean
H065.80|$^{+2.09}_{-2.11}$||$^{+4.22}_{-4.00}$|64.94|$^{+2.11}_{-2.02}$||$^{+4.12}_{-4.13}$|64.95|$^{+1.89}_{-1.94}$||$^{+3.77}_{-3.77}$|
q0−0.276|$^{+0.043}_{-0.049}$||$^{+0.093}_{-0.091}$|−0.285|$^{+0.040}_{-0.046}$||$^{+0.087}_{-0.084}$|−0.278|$^{+0.021}_{-0.021}$||$^{+0.041}_{-0.042}$|
j0−0.023|$^{+0.317}_{-0.397}$||$^{+0.748}_{-0.685}$|0.545|$^{+0.463}_{-0.652}$||$^{+1.135}_{-1.025}$|1.585|$^{+0.497}_{-0.914}$||$^{+1.594}_{-1.453}$|
s0−0.745|$^{+0.196}_{-0.284}$||$^{+0.564}_{-0.487}$|0.118|$^{+0.451}_{-1.600}$||$^{+3.422}_{-1.921}$|1.041|$^{+1.183}_{-1.784}$||$^{+3.388}_{-3.087}$|
M−19.16|$^{+0.07}_{-0.07}$||$^{+0.14}_{-0.14}$|−19.03|$^{+0.02}_{-0.02}$||$^{+0.05}_{-0.05}$|−19.17|$^{+0.07}_{-0.07}$||$^{+0.13}_{-0.13}$|
ΔM−0.054|$^{+0.023}_{-0.022}$||$^{+0.044}_{-0.045}$|−0.054|$^{+0.022}_{-0.023}$||$^{+0.045}_{-0.045}$|−0.050|$^{+0.022}_{-0.022}$||$^{+0.044}_{-0.045}$|
α0.127|$^{+0.006}_{-0.006}$||$^{+0.012}_{-0.012}$|0.127|$^{+0.006}_{-0.006}$||$^{+0.012}_{-0.012}$|0.130|$^{+0.006}_{-0.006}$||$^{+0.012}_{-0.012}$|
β2.624|$^{+0.071}_{-0.068}$||$^{+0.136}_{-0.140}$|2.625|$^{+0.065}_{-0.069}$||$^{+0.137}_{-0.135}$|2.667|$^{+0.068}_{-0.069}$||$^{+0.137}_{-0.135}$|
rd149.2|$^{+3.7}_{-4.1}$||$^{+7.7}_{-7.5}$|148.6|$^{+3.5}_{-3.8}$||$^{+7.5}_{-7.1}$|147.2|$^{+3.7}_{-4.0}$||$^{+7.8}_{-7.5}$|
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