Fig. C.1.
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Time evolution of the cumulative energy injected by the AGN (top) and the warm (middle) and cold (bottom) gas mass for the three variations of CRc_dsh listed in Table C.1. Grey shaded areas show the statistical variation of CRc_dsh from Appendix B. Neither a lower DCR nor a higher fb, st change the cooling flow properties of the clusters beyond stochastic variation.
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