Fig. 34.
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Left: comparison between the minimum companion mass derived in Sect. 5.1, and the AMRF-derived masses for the compact-object candidates. The sources where the AMRF mass is smaller than the minimum mass are AstroSpectroSB1, which have a non-negligeable flux ratio. Right: comparison between semi-major axes derived for the AstroSpectroSB1 systems using the astrometric parameters (horizontal axis) and the spectroscopic parameters (vertical axis). The yellow star is Gaia DR3 5136025521527939072.
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