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Fig. 7.

Fig. 7. Refer to the following caption and surrounding text.

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Same as Fig. 4 but for the dark matter profiles in the FP runs. We fit all profiles with the Einasto and Y24 models and calculated the running means. For Y24, instead of plotting rc/r200c, here we show the ratio between the FP best-fit value and the DMO one to highlight the changes brought in by the presence of baryons. Bottom: Concentration-mass relation in the FP runs.

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