Fig. 4
Various parameters of planets in no-migration simulations at 4 Myr. The top left, top right, bottom left, and bottom right panels show semimajor axis and eccentricity, semimajor axis and planetary mass, planetary mass and eccentricity, and planetary mass and inclination, respectively. The grey squares in the first three panels are corresponding values for planets observed by the RV method. In the top right panel, the error bars indicate pericentres and apocentres. Also, the blue, orange, and red symbols correspond to stellar metallicities of [Fe/H] = 0.5, 0.0, and –0.5, respectively.
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