Fig. 4

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Transit spectra for our cloudless (dots) and cloudy (diamonds) simulations, noised with PandExo, for NIRISS-SOSS (green, with a bin width of 0.08 µm), NIRSpec-PRISM (blue, with a bin width of 0.1 µm), and MIRI-LRS (red, with a bin width of 0.35 µm), corresponding to one transit with each instrument. The shaded regions around the spectra correspond to the native resolution of the instruments and their errors, before binning. The GCM post-processed transit spectra are in black, with a solid line for the cloudless case and a dashed line for the cloudy case. Contributions from major chemical absorbers are shown at the bottom of the plot.
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