Planets presented in this paper for HD 39194 (left) and HD 96700 (right) compared with similar synthetic planet configurations from the NG76 population of the NGPPS, ID 126 (left) and ID 862 (right). We show in black the synthetic planets that are similar to the ones we found and in gray some of the other relevant synthetic planets of those systems, the rest were removed for clarity. The upward near-vertical steps seen in some tracks correspond to protoplanet-protoplanet collisions (giant impacts).