Fig. 9.
Time series of the four parameters derived from the CCF for the star YZ CMi in the VIS channel. We show RV, FWHM, contrast, and BIS (from top to bottom) as a function of barycentric Julian Date (left), phase of the rotation period (middle), and also plot the correlation of the activity indicators with the RV (right). The data points are coloured according to the phase.
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