Fig. 2
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Dust emission of the diffuse ISM observed at high Galactic latitudes and normalised per H atom by Dwek et al. (1997) and Planck Collaboration XXI (2015) and as tabulated by Hensley & Draine (2021). Model (black) with 
µm (Table 1) and individual dust components as labelled. The area in grey shows the contribution of the dark dust.
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