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Fig. 6.

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Comparison between the L-FP and the SM-FP as a function of redshift. The panels show the evolution of FP coefficients b (top) and c (middle), and the zero-point offset, Δa = az − azi (bottom). Results are shown for two stellar mass-selected samples: a massive sub-sample with M* > 1 × 1011 M (red) and the full sample with M* > 2 × 109 M (blue). Solid lines correspond to the SM-FP, while dashed lines indicate the L-FP.

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