Fig. 6.

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Distribution of SFR-M⋆-D bins on the main sequence plane. Each bin is characterised by the mean SFR and M⋆ of the galaxies contained in each bin. Blue squares correspond to the stacks with reliable X-ray flux measurements based on the X-ray stacking analysis and the blue circles to those with uncertain flux measurements. Black stars show the individual galaxies with reliable X-ray flux measurements and the grey circles the galaxies with uncertain fluxes. The black dashed lines indicate the SFR and M⋆ range of the bins. The diagonal dashed lines indicate three different sSFR values (i.e. sSFR: 10−9, 10−10, and 10−11 M⊙ yr−1/M⊙).
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