Fig. 2.
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Emission model spectra (left panels) for WASP-33b (W33, blue) and KELT-20b (K20, red) and their corresponding VMRs of Si and SiO (middle panel) and T-p profiles (right panel). We assumed equilibrium chemistry and [Si/H] = 0 to generate the presented model spectra (for sub- and super-solar metallicity values, see Figs. C.2 and C.3).
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