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Fig. 1.

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Hertzsprung-Russel diagram of the characterized binaries. The absolute magnitude of the unresolved binary in the G band MG is plotted as a function of the colour GBP − GRP. The blue dots correspond to the APOGEE binaries, and the red dots correspond to the SB9 binaries. They are overplotted on the low-extinction Gaia DR3 HR diagram (in grey).

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