Fig. 1: cWB and Bilby reconstruction results.
From: An interference-based method for the detection of strongly lensed gravitational waves
Top, the blue and red curves represent the reconstruction results of cWB and Bilby, respectively. The black curve is the injected GW waveform. The x axis is the GW frequency, and the y axis is the absolute value of the waveform. Bottom, the blue curve shows the ratio of cWB and Bilby results. The black curve is the injected ratio of the wave optics magnification factor F(f) and the square root of the macromagnification \(\sqrt{\mu }\). In this figure, the macromagnification is set to μ = 66, and the microlensing convergence is set to κ* = 0.09. The BBH parameters used in this figure are provided in Table 1.
