Fig. F.1
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Spectra of a bulk silicate Earth-like (TERRA) planet of 1 R⊕ (as per Fig. 7) and 2500 K when no pressure broadening is considered (bold lines) vs. the broadened spectra (dashed) seen in the main paper (see Fig. 7). The unbroadenend lines are sampled at a constant pressure of 10−8 bar. The SiO features are significantly less pronounced when pressure broadening is ignored.
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