Revised semi-major axes and minimum masses. Top: targets with reported a > 3 au in the CH survey (Mayor et al. 2011). Lines between the revised (indicated by stars) and published values (indicated by filled circles) are drawn to facilitate the comparison between these values. Green colors correspond to planets for which the final orbital parameters and minimum masses are well constrained; red colors correspond to planets for which the semi-major axes and/or the minimum masses are not well constrained. The dotted lines correspond to solutions that provide an rms of residuals within 1 m s⁻¹ from the minimum rms. An arrow at the end of a dashed line means that values even beyond the limit can meet this criterion. HD 7449c is not shown as it is identified as a star. Bottom: same as in the top, but for the CL survey (Rosenthal et al. 2021) targets with a reported a > 5 au. The purple color corresponds to planets for which the semi-major axis and the minimum mass cannot be constrained.