Fig. 3
Spectroscopic orbits of the two planets in the π Men system (upper panel: π Men b; lower panel: π Men c; best-fit solutions in Table 3). The orange curve represents the best-fit model. For π Men c, we do not show the more scattered and less precise UCLES and CORALIE data for a bettervisualization, and the error bars include uncorrelated jitters added in quadrature to σRV.
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