Fig. A.3
Top three rows: correlations between the asymmetry parameters and their corresponding RVs for HD 10700. Bottom row:correlations between the FWHM and RVs for HD 10700. The correlations are consistently stronger when using SN mean RV compared to N mean RV for the asymmetry parameters; however, the correlation between the FWHM and the N mean RV, only for this quiet star, is stronger the analogous correlations with the estimated SN RVs. The estimated R are statistically significant, except for the correlation between FIG BIS and RV (p-values = 0.36).
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