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Fig. 1.

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Scaling relation between M and M* for central and satellite galaxies, shown as red and cyan dots, respectively. The best-fit power-law relations for central (red line) and satellite galaxies (blue line) are compared to the observational results from Kormendy & Ho (2013) (KH2013, dashed black line), and the best-fit parameters are given in the lower-right legend. The plot highlights the very small discrepancy between central and satellite galaxies and the observed relation.

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