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Fig. 7.

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Stellar mass-halo mass relation at z = 0 is assessed by considering galaxies across all our five simulated boxes, fb = 0.157 is the baryon fraction Ωbm. The stellar mass is computed within 0.1R200. The colour contours delineate grids containing a specific number of galaxies as indicated in the colour bar, utilizing 0.2 and 0.2 dex-wide bins along the x and y axes, respectively. We compare our results with abundance matching estimate by Moster et al. (2013), and with the empirical model by Moster et al. (2018).

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