Decomposition of the individuals components corrected in YARARA for HD 10700 on HARPS. Each RV component was obtained, as in Fig. 4, by computing the RVs before and after the flux corrections of a dedicated YARARA recipe. The RVs are obtained from the tailored line selection. Systematics known to be related to 1-year systematics are time-folded. We note that systematics can be folded at one sidereal year but are not described by sinusoid, explaining why their power can leak afterwards onto others frequencies in the periodogram. Despite the moderate rms of some components, the peak-to-peak of most of them is above 10 cm s⁻¹.