Fig. 11
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JWST Emission Spectroscopy Metric (ESM) (Kempton et al. 2018) as a function of planet orbital period for TOI-2431 b and other confirmed USP planets. TOI-2431 b is highlighted with the star, and other well-characterized USPs are shown with the thicker labels. The color bar shows the dayside equilibrium temperature assuming an albedo of AB = 0.
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