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Fig. 8.


SFR–M* diagram of our sample. The solid blue line is the fit to our data, representing the main sequence of star-forming galaxies at these redshifts. The dotted cyan, orange, and green lines are extrapolations of the main sequence at our median redshift from Speagle et al. (2014), Schreiber et al. (2015), Pearson et al. (2018). Filled circles are galaxies with reliable photometry and open circles are galaxies with possible contamination from bright nearby objects. The magenta diamond is the AGN identified in our sample. The gray diamonds are estimations of SFRs from the FUV magnitudes using IRX–β relation.

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