Average abundance ratio with respect to iron within R500 at z ∼ 0.1 over the cluster sample for z = 0.1 (left) and z = 1 (right) recovered using 100 ks observations. The input abundance ratio are shown as histogram bars filled with the respective contributions of SNIa (blue), SNcc (magenta) and AGB stars (yellow), computed from the outputs of the hydrodynamical simulation presented in Sect. 2. For z = 1, carbon (C) and nitrogen (N) are not shown as the lines are outside the energy bandpass of the instrument (not fitted).
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