Synthetic light curves of all five planets relative to the brightness of the parent star in different wavelength ranges. We show the eight days after the periastron passage, except for HAT-P-2 b because of its short orbital period. A vertical grey line in the top right indicates the typical MIRI LRS precision when using the full 5–12 µm range for a star of that visual magnitude. Ringing is seen as the local maxima in the light curves of HD 80606 b and TOI-4127 b, which is especially pronounced at longer wavelengths. HD 17156 b also displays a local maximum after the periastron peak in the long wavelength regimes.