Likelihoods in ﹩{{\rm{\Omega }}}_{0{\rm{m}}},{H}_{0},{\sigma }_{8},{w}_{0},{w}_{a},{w}_{\mathrm{DM},\mathrm{eff}}﹩ for cosmological reconstruction using Planck (black lines), Planck+R16 (red lines), and Planck+BSH (blue lines) for non-phantom (non)interacting models under consideration.