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Fig. 7.

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Radial velocity fit for the binary system Gaia DR3 702393458327135360 (HD 80234) from APOGEE. The radial velocity (km s−1) is plotted as a function of the phase. The orange dots correspond to the radial velocity epochs of the primary, and the purple dots show the radial velocity epochs for the secondary. The black curves represent the corresponding fits obtained by combining the APOGEE epoch radial velocity with the Gaia DR3 NSS astrometric orbital solution with BINARYS.

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