Observational signatures of microlensing in gravitational waves at LIGO/Virgo frequencies

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Fig. 17.

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F(w) for the two lensed sources shown in Fig. 15 (a and b). The red and dark blue curves are for source a. The dark blue curve is the corresponding amplification that it is obtained if only the peaks below 1.8 ms are considered. The light blue curve is for the source b in Fig. 15.

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