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Fig. 8.


Depletion time as a function of the ΣSFR, color-coded according to the distance to the main sequence. The solid and dashed lines are the fit to the sliding median and its 68% scatter respectively. The stars represent galaxies with LX, int > 1043 erg s−1. For comparison, the results of Elbaz et al. (2018) are shown by gray dots.

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