Fig. 10.
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Comparison between the values of the stellar over total mass fraction of the cluster members obtained with our lensing model (in blue) and with the SHMR from Girelli et al. (2020) (in orange). Only the 63 cluster members with σ0, FP > 80 km s−1 are shown. Left panel: stellar over total mass fraction of members as a function of their stellar mass. Right panel: SHMR.
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