Same as Fig. 3, but for a stellar mass of 0.4 M⊙. In these plots, the temperature range was shifted to 300–1100 K, instead of 700–1500 K, to make the range of orbital separations comparable to that of other stellar masses and because of the cut on the Roche lobe for planets with an equilibrium temperature of 1500 K orbiting 0.4 M⊙ stars.
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