\begin{table}%t1 \caption{\label{Tablew0w1}Table resuming the obtained constraints for a pure CPL~model (1), parameterization~\ref{wqz} with $\Gamma=1$ (2), $\Gamma=0.85$ (3) and assuming a constant $w$ (4).} %\centering \par \begin{tabular}{c c c c c} \hline\hline\noalign{\smallskip} Param. & 1 & 2 & 3 & Vanilla + $w$ \\ \hline \noalign{\smallskip} $ \Ob h^2$\tablefootmark{a} & $0.0222\pm0.0006$ &$ 0.0228\pm0.0006$ & $0.0228\pm0.006 $ & $0.0228\pm0.0006$ \\ $ \Omega_c h^2$\tablefootmark{b} & $0.107\pm0.005$ &$0.107\pm0.005 $ & $0.107\pm0.005$ & $0.109\pm0.005$ \\ $ \theta$\tablefootmark{c} & $0.104\pm0.003 $ &$ 1.041\pm0.002$ & $1.041\pm0.002$ & $1.042\pm0.003$ \\ $ \tau$\tablefootmark{d} & $0.856\pm0.017$ &$ 0.088\pm0.017$ & $0.088\pm0.016$ & $0.087\pm0.017$ \\ $ n_{\rm s}$\tablefootmark{e} & $0.958\pm0.014$ &$0.969\pm0.008$ & $0.968\pm0.008$ & $0.967\pm0.014$ \\ $ \log(10^{10} A_{\rm s})$\tablefootmark{f}& $3.05\pm0.04$ &$3.06\pm0.04$ & $3.06\pm0.04$ & $3.06\pm0.04$ \\ $ w_0$\tablefootmark{g}& $-1.027\pm0.123$ &$ -0.994\pm0.141 $ & $ -1.005\pm0.119 $ & $-0.965\pm0.056$ \\ $ w_1$\tablefootmark{g}& $0.278\pm0.408$ &$ 0.036\pm0.452 $ & $ 0.186\pm0.404$ & $0$ \\ \noalign{\smallskip} $ \Omega_{\rm Q} (\Ol)$\tablefootmark{h} & $0.735\pm0.017$ &$ 0.747\pm0.018 $ & $0.738\pm0.018$ & $0.739\pm0.014$ \\ Age\tablefootmark{i} & $13.9\pm0.1$ &$ 13.7\pm0.1$ & $13.8\pm0.1$ & $13.7\pm0.1$ \\ $ \Om$\tablefootmark{j} & $0.265\pm0.017$ &$ 0.253\pm0.018$ & $0.262\pm0.018$ & $0.261\pm0.020$ \\ $ \sigma_8$\tablefootmark{k} & $0.766\pm0.037$ &$0.780\pm0.037$ & $0.776\pm0.037$ & $0.816\pm0.014$ \\ $ z_{\rm re}$\tablefootmark{l} & $11.0\pm1.5$ &$11.1\pm1.4$ & $11.1\pm1.4$ & $11.0\pm1.5$ \\ $ h$\tablefootmark{m} & $0.698\pm0.018$ &$ 0.718\pm0.020$ & $0.706\pm0.017$ & $0.713\pm0.015$ \\ \hline \end{tabular} \tablefoot{\tablefoottext{a}{Normalized baryon matter density times $h^2$,} \tablefoottext{b}{normalized CDM density times $h^2$,} \tablefoottext{c}{ratio of sound horizon to angular diameter distance,} \tablefoottext{d}{optical depth to reionization,} \tablefoottext{e}{primordial spectral index,} \tablefoottext{f}{primordial scalar power at $k=0.05~\rm Mpc^{-1}$,} \tablefoottext{g}{parameters describing the equation of state of dark energy,} \tablefoottext{h}{dark energy density,} \tablefoottext{i}{age of the universe in Gyr,} \tablefoottext{j}{normalized matter density,} \tablefoottext{k}{matter density fluctuation amplitude,} \tablefoottext{l}{reionization redshift,} \tablefoottext{m}{reduced Hubble parameter.}} \end{table}