Amplitude of RM anomalies as a function of the time that anomaly appears in the RM signal. RM anomalies for the case of occultation with stellar spot are shown in the positive part of y-axis and the occultation with the stellar plage are presented in the negative part of y-axis. Panel on the top-right corner shows the same but as a function of the position of planet-active region occultation (0 on the x-axis means overlap occurs while the active region is at the center of stellar disk, and 1 means occurs on the limb of the stellar disk).