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Fig. 6


Same as in Fig. 5 but now we assume that in addition to sky position we also know the inclination of the binary. The uncertainty ratios of the parameters are between 7 × 7 VCM (MC2) and 4 × 4 VCM (MC4). The improvement factors in amplitude include corrections due to overestimated uncertainties in the amplitudes of face-on systems (see Sect. 4.1). Note that the last panel is plotted in log scale in order to highlight the relatively large improvements for the systems with smaller inclinations.

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