Fig. B.1
2-component MBB fits for 14 dwarfs with available IRAS and ISO photometry. Filled red dots correspond to IRAS or ISO data, while black dots show Herschel photometry. The emissivity index of the cold dust component (dotted line) is fixed at βc = 1.5, while the warm dust component (dashed line) has βw = 2.0. The VCC catalogue ID is given at the upper-left corner of each plot.
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