Caption: 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 is 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 Setc. 2 (Cucchetti et al. 2018). For z=1, carbon (C) and nitrogen (N) are not shown as the lines are outside the energy bandpass of the instrument (not fitted).

Additional comments: Figure reproduced from Cucchetti et al. 2018 (A&A, 620, A173).

Credits for data/References: Cucchetti et al. 2018 (A&A, 620, A173).

Creation date: 14/12/2020. Version #:3.

Credits: X-IFU Consortium. Copyright: © DB/X-IFU.