Fig. 9.
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Comparison between the M-to-σ relation estimated by our analysis and those adopted for the cluster galaxies in the SL models of MACS J0416 (B23), AS1063 (B19; G22), MACS J1206 (B19), and A2744 (Bergamini et al. 2023b). Top panel: comparison with the SL models describing the cluster galaxies according to Eqs. (5) and (6). Bottom panel: comparison with the SL model of AS1063 by G22, based on the FP.
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