Characterising planetary systems with SPIRou: Questions about the magnetic cycle of 55 Cnc A and two new planets around B

Open Access

Fig. 8

Orbital solution obtained from SPIRou (‘s’) RV data of 55 Cnc B as a function of time (top) and phase (middle and bottom for planets b and c, respectively). The residuals are shown in panel b. Red points are mean measurements per regular 0.1 phase bins as calculated with RadVel when sufficient data is available.

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