Fig. 12
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NUV-to-NIR transmission spectra normalised by the scale height for WASP-79 b (Teq = 1716 K) and three additional hot Jupiters: WASP-121 b (Teq = 2358 K) (Evans et al. 2017, 2018), HAT-P-41 b (Teq = 1941K) (Wakeford et al. 2020; Sheppard et al. 2021), and WASP-I78b (Teq = 2450 K) (Lothringer et al. 2022). WASP-121 b and WASP-79 b’s HST STIS E230M measurements are from this work. The formalism is similar to Fig. 2 in Lothringer et al. (2022).
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