Fig. 23
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RV sequence of GJ 581 with the orbits of GJ 581 b (P = 5.37 days) and c (P = 12.91 days) is shown in the same plot using the solutions of Rosenthal et al. (2021). Our measurements are consistent with the known planetary solutions with a residual RMS of 1.35 m s−1. The exposure time is 2 × 300 s. The estimated photon-noise is 1.5 m s−1. White dots correspond the night-binning RVs.
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