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Fig. 8.

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Variation of continuum (Aconti) and BEL amplitudes (ABEL) with different inclination angles for BBHs with M•• = 109M, ω = 0°, and e = 0.0–0.6. The two left panels show the case when only the secondary BH is active (qL = 1 : 0), and the two right panels show the case when both the BHs are active with qL = 1 : 1. In each panel, the points colored from dark blue to red represent the orbital eccentricity of BBHs e = 0.0–0.6, respectively.

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