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Fig. B.1.

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Dust attenuation curve parameters S and B derived from SED fitting using two different star formation histories: a constant SFH and the fiducial flexible (non-parametric) SFH model (Leja et al. 2019). The left panel shows the slope parameter S (blue), and the right panel shows the UV bump strength B (orange). The solid black line indicates the 1:1 relation.

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