Least-squares deconvolution profiles for the young, Sun-like stars examined in this work. Each panel corresponds to a different star and contains the Stokes V (solid blue line) and Stokes N (dashed blue line) profiles. The vertical dotted line indicates the radial velocity of the star. We observe that some stars have a clearly detected Zeeman signature (e.g. HD 1835, HD 82443), while others present a flat Stokes V profile (HD 149026, HD 219828), hence they were excluded from tomographic inversion.