English: The radial-velocity curve of HD81040 predicted by the Gaia astrometry solution (black curve, offset by the systemic velocity) and the measured radial velocities from Sozzetti et al. 2006 (black symbols). Because the radial-velocity period is much more precise and the radial-velocity data were taken >10 years before the Gaia data, the radial-velocity period was used for the purpose of this figure. The grey region shows the 1-σ-equivalent confidence interval of the Gaia solution.
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