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Fig. 7.


SFR versus stellar mass plot for the BAT6 sample at 1 <  z <  2 (squares). The circles are from the MOSDEF sample at 1 < z < 2. The red line is the best fit to the MOSDEF data and the dotted lines represent the intrinsic scatter, following the method of Shivaei et al. (2015). The points are coloured by metallicity in the M08 calibrator. Galaxies where no metallicity could be measured are coloured in grey with a cross.

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