Benchmark model including an astro-PAHs wind component as in Fig. 16 coded with a single red temperature color table. (upper) Model images at full resolution for selected wavelengths spanning the MIR for bands including astro-PAHs contributions (6.25, 7.7, 11.3 μm) or bands representing adjacent bands with more continuum (5.8, 10.25, 14.4 μm) for comparison. (middle) Model images once convolved with JWST PSF. Note the alternance of more rounded shape for continuum dominated bands and chalice/hourglass shape for the one with astro-PAHs contribution. (lower row) observed MIRI images. The colorbars indicate the intensity levels, normalised to the maximum intensity for each image, in log scale.