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Kiloparsec scale gaseous clumps and star formation at $z=5 7$

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Figure

Table 1. Overview of the z > 5 star-forming galaxies observed with ALMAused in this paper, ordered by name.
Figure 2. Top: [Cii] flux map of BDF2203 obtained integrating the ALMAcube over the velocity range between -60 km/s and 132 km/s
Figure 3. Rest-frame UV images of the nine z > 5 star-forming galaxies showing multi-clump morphology in [Cii] and/or rest-frame UV emission
Figure 5. Deviations from the local L[CII]-SFR relation as a function ofSFR. The 1σ dispersion of the local relation is indicated with the shadedgreen region
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