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Fig. 12.


Distribution of MS subtracted SFR for the 0.85 <  z ≤ 1.21 redshift bin for CANDELS non-merging galaxies (blue) and merging galaxies (red). This is the only data that is fitted with a double Gaussian distribution due to the clear multi-modal population. As can be seen, the main and secondary populations have a slightly higher mean MS subtracted SFR than the non-merging galaxies.

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