Planetary injection recovery in the HD 10700 dataset; comparison between the injected K semi-amplitudes (black dotted line) and the recovered ones obtained after fitting a two-sinusoid model for the planets at 37.87 (K = 2 m s⁻¹) and 122.42 days (K = 3 m s⁻¹). No significant absorption of the planetary signals is observed after YARARA processing, neither by flux correction (green markers) nor by morphological correction (red markers), since values similar to those without correction (orange markers) or DRS (blue markers) are found. All the recovered amplitudes are compatible with the injected values considering the uncertainty due to pre-existing signals.