Fig. 1.
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Left panel: Dark matter distribution of the TNG50 simulation. Magenta empty circles show the position of the selected haloes of the zoom-in simulations. Right panel: Mocked images in JWST NIRCam F200W, F115W, and F070W filters (face-on) calculated in Nelson et al. (2018), (TNG database) for the TNG50 galaxies that are re-simulated. The NIRCam blue channel highlights the young population of the galaxy, and the NIRCam red channel older populations. The original TNG50 galaxies present a massive disc with a smaller bulge and form a strong bar.
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