Fig. 3
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Polarised extinction of the diffuse ISM (circles) with error bars indicating the observed scatter (Voshchinnikov et al. 2012; Bagnulo et al. 2017). The model (black) with 
µm (Table 1) and contributions (dashed) from large amorphous carbon (brown), large silicate grains (green), and the dark dust area in grey, when treated as prolate particles is shown.
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