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Fig. 1.

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Distribution of central galaxies at z = 0 as a function of SFR and M*, for SIMBA and TNG in 100 Mpc/h, from left to right, respectively. The coloured background is the logarithmic number of central galaxies. The black dot-dashed line is the SFMS of TNG100, following the definition in Ma et al. (2022): log(SFR/yr−1M) = 0.83log M* − 8.32, and black cross represents SFMS of star-forming central galaxies in SIMBA100, where star-forming galaxies are simply selected with log(sSFR/Gyr−1M)≥ − 1.8. Magenta lines separate the star-forming and quenched galaxies in both panels.

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