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Tracing the nature of dark energy with galaxy distribution

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Academic year: 2021

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Figure

Figure 1. Geometrical and evolutionary terms on the cluster mass scale.
Figure 2. The upper panel shows how the redshift distribution on the cluster mass scale depends on the models
Figure 3. The halo mass function at z = 0. Results for ’3CDM (dashed line), RP (solid line), and SUGRA (dotted line) overlap.
Figure 5. Galaxy (cumulative) mass function at z = 0 from simulations (dots) versus an integral Schechter function, with o , α and M ∗ shown in the frame.
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