Fig. C.2.
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Best-fit Keplerian solution for the astrometric measurements based on the Doppler-shifted Brγ line observed with SINFONI. The red fit represents the orbital solution shown in Ciurlo et al. (2023). While we find some overlap with our solution, the fit presented in Ciurlo et al. suffers from a low significance when we compare the astrometric measurements presented in this work.
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