Fig. 10
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Spectrum of the different dust compositions (colour) and sizes (line style) compared to the total dust continuum (olive; star, rim, midplane, and surface layer) and the JWST/MIRI spectrum of Sz 28 (black). Both are offset by −9 mJy. The error tubes denote the 16th and 84th percentile of the dust flux from the posterior of models.
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