Fig. 16.

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Example of galaxy at cosmic noon (z ∼ 2.5) as seen in MIRI/F560W (red), NIRCam/F182M (green) and HST/F814W (blue) from Boogaard et al. (2024). The MIRI emission unveils the presence of a disc-like stellar mass distribution, while the NIRCam and HST images highlight young star forming regions. The cutout is 4″ × 4″ (corresponding to ∼3 × 3 kpc). The FWHM (0.207″) of the MIRI/F560W PSF is shown as a white circle in the lower left.
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