Fig. 6.
Energy balance plots showing the SMBH binary orbital energy changes compared to the cumulative energy changes of stellar particles for different times. The blue lines represent the cumulative energy changes of all stars that come within 10abh of the SMBH binary during the specified time period. The thick green line corresponds to the total SMBH binary orbital energy change for the same time period. The red dashed line corresponds to the cut-off value we use to define the high-energy tail.
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