Activity time series of old stars from late F to early K - VI. Exoplanet mass characterisation and detectability in radial velocity

Open Access

Fig. D.1

Rms of the binned RV residuals vs. spectral type from the follow-up analysis for ∆T_spot1 (solid line) and ∆T_spot2 (dashed line) for the middle of the habitable zone. The fitted 1 M_Earth planetary signal has been subtracted.

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