Fig. 10.

Difference in the νmax values extracted from the fits using a two super-Lorentzian and a four super-Lorentzian granulation model. Left and middle panels: difference in νmax, fit for the RG-binary light curves where both components (Star A and Star B) are pulsating. Right panel: difference in νmax, fit for the RG-binary light curves where only one component (Star A) is pulsating. The axes, symbols, error bars and colour-coding is the same as in Fig. 5, except that the horizontal axis corresponds to the absolute percentage difference between the νmax, fit values for the two super-Lorentzian (2SL) and four super-Lorentzian (4SL) cases.
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