Fig. 1.
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Corrected DM halo spin distribution for the NIHAO sample (solid gray curve, Jiang et al. 2019) and from the dark-matter-only simulations of Bullock et al. (2001; dashed gray curve), together with the MW predictions for the NFW and contracted NFW mass models (faint and solid red points), and the spins of the MW-type galaxies in NIHAO (green stars).
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