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Fig. 3.

image

Luminosity of [C II] as a function of UV-based SFR in ID22914 (large symbol) and in a compilation of UV-selected star-forming galaxies at z >  5 (see Carniani et al. 2018, and references therein). The relation for intermediate- to low-redshift main sequence star-forming galaxies from Herrera-Camus et al. (2018) is also shown for comparison as a dashed line, with its 1σ scatter in green shading. ID22914 falls close to the expected relation, and within the scatter of values observed in similar galaxies at high redshift.

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