Fig. C.1
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GLSP of the RV and the available activity indicators measured on HD 27969 with the SOPHIE (SOPHIE+) spectrograph. From top to bottom: GLSP of the RV, FWHM, BIS, and 
time series and the window function of the data. The best-fit orbital period of the planet is marked by a vertical dashed red line. The black horizontal dotted, dash-dotted and dashed lines correspond to levels of 0.1, 1 and 10% of FAP (Zechmeister & Kürster 2009).
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