Exo-REM best-fit model (black curve) and the lighter black models come from the posterior distribution from the best fit. The points represent the photometric values from VLT/SPHERE (green), Suburu/HiCIAO (purple), LBTI/LMIRcam (orange), and Subaru/ICRS (blue). The MIRI photometry is shown in red. Photometric points are plotted at the filter’s central wavelength, with the width indicated. The bottom plot represent the residuals between the photometric points and the best fits models: all point agree within a 3 σ precision. Right: zoom on the MIRI data and the NH₃ absorption, fluxes values are displayed with a linear scale.