Activity time series of old stars from late F to early K - II. Radial velocity jitter and exoplanet detectability

Open Access

Fig. 5

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Upper panel: RV jitter (computed on rvact2 added to rvogs and rvinst) vs. B− V (right) and Log (left), for θ_max equal to the solar value, and after binning in B−V and Log , respectively. The color code is similar to Fig. 1. Middle panel: same for θ_max equal to the solar value +10°. Lower panel:same for θ_max equal to the solar value +20°.

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