Fig. 7.
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Distribution of Gini and M20 parameters for all our models at the final redshift z = 2. Models in low- and high-spin halos are labeled with hollow and solid markers separately. Models with the same BH-related parameters in Table 1 are labeled with the same marker shapes and colors. Dashed lines separate the regimes into mergers/ellipticals/spirals morphological types (Lotz et al. 2008).
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