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Fig. 7.

image

Top panels: correlation between the stellar disc scale-length Rd and the dark matter halo parameter r−2 (left panel: MLconst; right panel: L18a). Bottom panels: cored profiles with n <  2, correlation between Rd and the core size r0 defined as the radius at which the DM density becomes half the central one (left panel: MLconst; right panel: L18a).

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