Fig. 4.
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Radial profiles of the galaxies in this paper with both [CII] and continuum emission (using the HR+MR+LR concatenation). The [CII] emission was converted to a molecular gas surface density and the continuum to an obscured SFR. The aperture of which the galaxies fluxes in Sect. 3.4 were taken in the HR+MR+LR concatenation which is shown by the blue line.
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