Fig. B.1.
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Top: Example X-ray spectrum of Abell 2597 from one of the two regions used to derive the hot gas-phase metallicity. The observed spectrum, corresponding to one Chandra observation, is shown as gray data points, while the best-fit model is overlaid in pink. Bottom: Example of MUSE spectrum of one spaxel of Abell 2597 shown in gray, and the best fit model is shown in pink.
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