Mass vs heavy element mass relation for the ten simulated planets. Blue points show simulations where the initial formation location matched the observed heavy element mass most closely. Data from Thorngren et al. (2016) are shown in red (T16). Planets that are simulated in this work are plotted as red squares, while those that are not simulated in this work, either because they are less massive than 0.5 M_J or because the stellar chemical abundances of their host star are not included in Teske et al. (2019), are plotted as pale red diamonds.