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Fig. 9.

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Redshift evolution of the characteristic halo masses fitted in the HOD model for stellar mass-limited galaxy samples. Mh, min is the characteristic halo mass to host a central galaxy, Mh, 1 to host a satellite. Error bars are the 1σ uncertainties from the MCMC sample distribution, and quantities are shown for HOD models with and without nonlinear scale-dependent halo bias, respectively in dash-dotted and solid lines.

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