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Fig. 3

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Architectures of 27 systems with both SPs and CJs in the mass range 0.3 ≤ Mp ≤ 13 MJup, ordered according to increasing orbital eccentricity of the CJs (from top to bottom; for multiple CJs, the highest eccentricity is considered). The planet circles have sizes proportional to their mass (see legend in the top right corner), and colors indicating orbital eccentricity (more eccentric planets are shown in yellow). Host stars are color coded as a function of stellar metallicity (metallicity increases from blue to red). All systems with three or more inner SPs are accompanied by CJs with low eccentricities.

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