Fig. 3
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Model spectra, CCF maps, and Kp maps for OH, Fe, and both species combined. Left panel shows the model spectra after continuum removal. Middle panel displays the CCF map in the stellar rest frame (i.e. corrected for BERV and systemic velocity). The dashed cyan line represents the planetary RV derived from the expected value of Kp. Right panela presents the Kp map for each molecule. The dashed lines intersecting at the cross mark indicate the position of the S/N peak. The colour bar represents the S/N values.
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