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These figures are similar to Figs 3 and 4 from Rodriguez-Gomez+ (2019), but in this case we extend the analysis (originally for TNG100) to the highly detailed TNG50 simulation. Here we show idealized synthetic images (using Pan-STARRS1 g,r,i filters) of randomly selected galaxies from the TNG50 simulation, generated with the SKIRT radiative transfer code. The text labels indicate the total stellar mass and the 3D stellar half-mass radius.

No more images.