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Fig. D.1.
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β-curves of Fig. 1 against the particle radius, available simulation sets of (β, Q/m) (grey dots), and the selected simulation sets (blue circles) that are closest to the β-curve of the adapted astronomical silicates with ρd = 2500 kg/m3 (maroon line). (See Hunziker et al., in prep.; after Sterken et al. 2013, Fig. 3.)
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