Fig. B.3.

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CMD of the 279 final MS+BH candidates (white stars), overlaid on the initial MS candidate sample (2D histogram). The confirmed BH binary Gaia BH 1 is highlighted, together with known Gaia NS binaries (triangles). The apparent clustering of candidates at MG < 4.5 mag (shaded grey) likely reflects the less efficient removal of MS+MS binaries on the upper main sequence by the XP-based filtering.
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