Fig. E.1
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Variation in RV, bisector inverse slope (BIS), and full width at half maximum (FWHM) as a function of stellar rotation phase for an equatorial stellar spot with a filling factor of 1% and a temperature contrast of 663 K below the photosphere. Top: Comparison of the crosscorrelation function (CCF) properties simulated using S0AP2.0 and SOAPv4. Bottom: Difference between the simulations obtained with SOAPv4 and S0AP2.0.
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