Fig. 2.

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Distributions of the Bullock parameter λ as derived in Eq. (2). The black line refers to the total sample, the dotted red line refers to high-mass galaxies, and the dashed blue line refers to low-mass galaxies. The vertical purple lines are located at the 25th and 75th percentiles of the λ distribution and represent a qualitative distinction between high-spin parameter and low-spin parameter galaxies.
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