Fig. 1
Mass of the planet vs. bolometric optical and infrared incident flux in units of flux received at Earth. In grey, transiting exoplanets are shown with V < 16 and masses determined with a precision better than 20%. WASP-76b is shown in orange. For comparison WASP-49b (Wyttenbach et al. 2017), HD 189733b (Wyttenbach et al. 2015), and HD 209458b (for reference) are shown in red, blue, and green, respectively.
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