Iron abundance profiles up to R₅₀₀ for the individual MAGNETICUM sample (thin dashed grey lines). Simulated median profile and scatter are marked as blue thick dashed line and shaded area. Coloured datapoints refer to the observational profiles for individual X-COP clusters by Ghizzardi et al. (2021), with normalisation rescaled to the reference solar abundance by Asplund et al. (2009), used for the profiles of the simulated clusters.