DM density profiles in M_⊙/kpc³. Each panel show ρ_dm(r) as a function of r/R_e obtained from our disk-halo decompositions (Fig. 4). The stellar-to-halo-mass ratio (log X ≡ log M_⋆/M_vir) is indicated. The gray bands represent the 95% confidence interval and the dotted lines represent NFW profiles. The vertical dotted lines represent the 1 kpc physical scale, corresponding to ≈1 MUSE spaxel, and indicates the lower limit of our constraints.