Fig. A.1
Specific entropy spf at the bottom of the gaseous envelope as a function of envelope mass at the end of the disk lifetime (i.e., formation phase) for the cold-nominal (left) and hot population (right panel). The colors represent the core mass of the planets in units of log 10(Mcore/M⊕). The black lines show the least-squares fit of Eq. (A.1).
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