Fig. 5.
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Dust attenuation curves of the three slit regions (S1–S3) at z = 6.5676 derived from the slit-level spectro-photometric fits. S1, S2, and S3 are shown as solid blue, dashed orange, and solid green lines, respectively. Standard Milky Way (MW), Calzetti, and Small Magellanic Cloud (SMC) attenuation curves are overplotted for comparison (dashed, dotted, and solid gray lines, respectively). Inset: Corresponding SFHs of the three slit regions.
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