Fig. 8.

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Comparison between the projected sAM of each ePN.S galaxy jp,ePN.S and the median of the distribution of jp(≤6Re) of the ePN.S analogs among the TNG100 ETGs, divided by the sum in quadrature of 1σ-scatter of distribution of the TNG analogs and the error on the ePN.S jp,ePN.S. The three histograms correspond to the three jp determinations for the ePN.S galaxies: the light-weighted jp, light, the mass-weighted jp, mass, and the jp, mass + IMF corrected for IMF gradients. The jp values for the TNG100 galaxies are mass-weighted. Vertical dashed lines show the median of the three distributions.
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