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Fig. C.1

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The North of the Dark Bay as seen by the JWST’s NIRCam instrument with north up and east left. Several images in different filters were combined to produce an RGB composite image as in Fig. 3: F335M (red), F470N (green) and F187N (blue) that trace emission from hydrocarbons (AIBs), dust and molecular gas (H2 0-0 S(9) line), and ionized gas (Pa α line), respectively. The individual images used to make the RGB composite one are shown below. No continuum was subtracted. The size of the images is ~150″ × 150″ and it is centered on RA=05h35m21s.09, DEC=-05°21′40″0L White boxes (labeled A, B) are enlarged in Fig. C.3.

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