Planetary absorption along the YARARA V1 and V2 sequence of the planetary injection test performed on HD 10700. Planets at 37 and 122 days were injected at the spectrum level. A 2-Keplerian circular model at the periods of the injected planet was fit at each step of the pipeline to trace the recipes with potential absorption facilities. An uncertainty of 10% on the K semi-amplitude was typical expected due to the presence of smaller amplitude planetary candidates (Feng et al. 2017; Cretignier et al. 2021). Top: representation of the 2-circular solution fit into a polar diagram, the radius represents the K semi-amplitude and angle the phase of the signal. Injected amplitudes (2 and 3 m s⁻¹) are highlighted by the dark circle, and reference phase were at null value. Middle: variation of the fit K-semi amplitudes as a function of the YARARA’s stage. Separation between YV1 and YV2 is depicted (vertical black dotted line). The shell correction (Cretignier et al. 2022) is considered as the first stage of YARARA V2, whereas the three steps corrections described in Sect. 2.6 are labelled as slice, colour and lbl respectively. Bottom: same as middle in relative percentage difference. At the end of YV2, the recovered amplitudes and phases are plainly compatible with the injected ones.