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

Open Access

Fig. B.2

Average correlations between simulated RV_sppl (solid line) and F' vs. spectral type for ΔT_spot1 (upper panel) and ΔT_spot2 (lower panel). The dashed line shows only spots.

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