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Fig. D.1.

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Predicted Hα line profiles from simulations for E19, E31, E36 and E52 (first, second, third, and last rows, respectively) shown along LOS in the z, y, and x (first, second and last columns, respectively) directions. The grey-shaded regions represent the calculated results. The solid black lines indicate the total flux (from SF, the accreting primary and secondary MBHs) along with the noise component and the red-dotted lines show the contribution only from SF.

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