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Fig. 2.

image

Stellar mass-weighted average age LOESS-smoothed distributions on the dynamical mass–size plane for E-SDGs (left panel), E-DDGs (middle panel), and all galaxies (right panel) in the EAGLE simulation at z = 0. The dashed lines show the predicted distributions for systems with constant σe at 100, 125, 150, 200, 225, 250, and 300 km s−1 (from left to right).

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