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Fig. D.1.
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Angular autocorrelation function of galaxies in the COSMOS-Web survey, in redshift and mass limited bins. Dash-dotted lines show the HOD best-fit models with Jose et al. (2016) nonlinear scale-dependent halo bias, and solid lines are HOD best-fit models without it (assuming a large-scale bias of Tinker et al. 2010).
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