Table 2: The basic cosmological parameters derived from our model are compared with observational data.

Dataset		 s $\widehat{H}_0$ ${\Omega_{\Lambda_{\rm eff}}}$ $w_\phi $

high redshift SNIa		 $\rm -1.46^{+0.04}_{-0.03}$ $\rm0.96^{+0.05}_{-0.05}$ $\rm0.69^{+0.04}_{-0.06}$ $-1.01\pm 0.02$
dimensionless coordinates test $\rm -1.49^{+ 0.02}_{-0.04}$ $\rm0.97^{+0.04}_{-0.03}$ $ 0.73\pm 0.08 $ $-0.98 \pm 0.03$
relative galaxy ages $\rm -1.49^{+0.03}_{-0.09}$ $\rm 1.01^{+0.01}_{-0.03}$ $ 0.80 \pm 0.07$ $-0.99 \pm 0.04$
sze data $\rm -1.49^{+0.03}_{-0.05}$ $\rm 1^{+0.01}_{-0.03}$ $ 0.70\pm 0.05$ $ -1 \pm 0.04$
GRBs dataset $\rm -1.43^{+0.02}_{-0.04}$ $\rm0.98^{+0.03}_{-0.03}$ $ 0.76 \pm 0.06 $ $-0.9\pm 0.04 $
fraction of gas in clusters $\rm -1.39^{+0.04}_{-0.01}$ $ 0.98\pm 0.04$ $\rm0.77^{+0.05}_{-0.03}$ $-0.87 \pm 0.05$
galaxies peculiar velocity $-1.4\pm 0.1$ $\rm0.94^{+0.05}_{-0.02}$ $ 0.65\pm 0.08 $ $-0.85 \pm 0.04$
average ${-1.46 \pm 0.09}$ ${ 0.97 \pm 0.02}$ $ {0.74\pm 0.03}$ $-1.01\pm 0.02$


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