Fig. 10
Star formation rate as a function of stellar mass. Symbols are the same as in Fig. 9. The AGN SFR is shown with different contributions of the Hα+[NII] stellar emission to the total flux. We compare our results with those from other works. The dashed and the dashed-dotted lines represent the best fit with 1σ scatter for the MS of field galaxies from Tacconi et al. (2013).
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