Fig. C.1
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Example of several regions within the nebula catalogues towards NGC 1566. The MUSE (first row) and HST (second row) observations, overlaid with contours showing the boundary of each source in the respective observations. (third row) We show a map of the complexity score for each region. (fourth row) We show the nebula (red contours) and 32 pc NUV-identified stellar association (Larson et al. 2023; blue contour) overlaid on a HST filter red (F814W) green (F555W) blue (F438W+F336W) image (see Lee et al. 2022).
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