Fig. 1
Upper panel: present-time (t = t0) matter density parameters in the standard (ΛCDM, black line) and the void (GBH) cosmological models (red and cyan lines). Lower panel: redshift evolution of the dimensionless matter density parameters in the standard (ΛCDM) and the void (GBH) cosmological models. The dotted vertical lines delimit the lowest redshift interval considered in the computation of the LF at which the faint-end slopes are fit.
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