Fig. 15
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Emission spectra of TRAPPIST-1b (upper panel) and c (lower panel), calculated at the secondary eclipse. The spectra are calculated using GCM simulations of H2O-rich (blue to gray) and CO2-rich atmospheres (red to orange). Emission spectra are also computed for airless planets (in bold black). The 1σ error bars are calculated using the JWST Cycle 1 observation program (for more details, see Sect. 3.5.3).
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