Fig. 19.
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SFMSs of the sample galaxies at z = 6. The upper and lower panels present the SFMSs constructed with SFR10 and SFR100, respectively, while the left and right panels show results obtained from the median posterior and the posterior with the minimum χ2, respectively. The solid black line marks the best fit to the true SPHINX20 data, and the solid coloured lines indicate best-fit relations derived with different SFH models in the attSNE_Z_F410M model. The best fit for the constant SFH model is excluded from the upper panels, as many galaxies return SFR10 values of zero. The minimum χ2 posterior more accurately reproduces the true SFMS from the simulation more closely, although it lies slightly below current high-z observations (Heintz et al. 2023; Rinaldi et al. 2022).
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