Sensitivity of JWST/MIRI observations using ATMO-strong (strong chemical disequilibrium) evolutionary models. From left to right: 10 μm filter F1065C, 11 μm F1140C, and 15 μm F1550C. The color bar in each plot means the detection probability and the solid lines highlight the 10%, 50%, and 90% detection thresholds. The dotted and dashed lines correspond to 1σ uncertainties, respectively.