JWST/MIRI images of the Fomalhaut system reproduced from the publicly available data from Gáspár et al. (2023), with their additional scaling factor of |$3.14$| for the F2300C image reversed (discussed in Section 5). Total image fluxes are 89 |$\pm$| 57, 176 |$\pm$| 50, and 895 |$\pm$| 73 mJy (from left to right; uncertainties extracted from Gáspár et al., 2023, their fig. 3).