Table 1: Variance of the overdensity field smoothed on $8~ h^{-1} ~{\rm Mpc}$ used in the normalization of number counts to the present-day halo abundance in $\Lambda$ -model with $\sigma _{\rm 8}=0.9$ for homogeneous (second column) and inhomogeneous (third column) dark energy models.
$\sigma_8$

Model Homogeneous Inhomogeneous

2EXP₁ 0.897 0.876

2EXP₂ 0.899 0.886

w=-0.8 0.898 0.857

w=-1.0 0.900 0.900

w=-1.2 0.901 0.942

**Table 1:** Variance of the overdensity field smoothed on $8~ h^{-1} ~{\rm Mpc}$ used in the normalization of number counts to the present-day halo abundance in $\Lambda$ -model with $\sigma _{\rm 8}=0.9$ for homogeneous (second column) and inhomogeneous (third column) dark energy models.
	$\sigma_8$
Model	Homogeneous	Inhomogeneous
2EXP₁	0.897	0.876
2EXP₂	0.899	0.886
w=-0.8	0.898	0.857
w=-1.0	0.900	0.900
w=-1.2	0.901	0.942

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