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Fig. 1.
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Face-on view of a simulated galaxy at z = 4. From left to right, the columns show the surface density of young stars (with ages ≤ 200 Myr), total gas (including H2) surface density, H2 surface density, and [C II] surface brightness. In each panel, the circle indicates 0.1 times the virial radius of the parent DM halo.
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