Fig. B.1.
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Comparison of the inner DM slope γ obtained using different HI surface density models in the disk-halo decomposition. Shown are the constant HI surface mass density vs the Martinsson et al. (2016) profile (left) and vs the Wang et al. (2025) profile (right). The error bars indicate 95% confidence intervals from the MCMC posterior. The dashed 1:1 line marks perfect agreement.
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