Activity time series of old stars from late F to early K - V. Effect on exoplanet detectability with high-precision astrometry

Open Access

Fig. C.1

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rms (left) and skewness (right) distributions of the activity time series in both directions for (from upper to lower panel) the X direction and ΔT_spot1, the Y direction and ΔT_spot1, the X direction and ΔT_spot2, and the Y direction and ΔT_spot2. Different curves show the ten inclinations (same colour code as in Fig. 1).

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