Fig. 9

Evaluation of the correlation between the RVs and the asymmetry parameters of the simulated data with a 1% spot and an injected planetary signal. The shape of the CCF changes as the spot moves, producing statistically significant correlations only between the estimated RVs and the asymmetry parameter. The correlations between the estimated RVs and the width parameter of the CCF are weaker than the case with only a spot.
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