Fig. A.2.
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Eigenvalues ratios b/a (left panel) and c/a (right panel) as a function of the logarithm of stellar mass (solid black lines) and the logarithm of DM halo mass (dashed black lines) for the three smoothing scales analyzed (1, 2, and 4 Mpc h−1) differentiated by the thickness of the lines, as indicated in the legend. Eigenvalues are estimated from the shear velocity field.
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