Fig. B.1.
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Comparison of JWST-MIRI spectra (from top: Region 1, 2, and 3) with the ISO-SWS spectrum (bottom). The MIRI apertures are defined in Fig. 1. The black dashed line indicates the continuum which was subtracted in Figs. 2 and 3. We note that the JWST spectra are in surface brightness units (MJy/sr), while the ISO-SWS spectrum is in flux density (Jy).
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