Fig. 18
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Contribution of individual opacities for the MIRI photometric region. The black spectrum is the PO/CO2 model that is also shown in Figure 1. Coloured spectra correspond to models where the indicated species is the dominant opacity contributor. The calculated MIRI photometric noise corresponds to 3 eclipses for the F1800W and F2100W filters, and 4 eclipses for the F2550W filter.
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