AGN populations in the local Universe: Their alignment with the main sequence, stellar population characteristics, accretion efficiency, and the impact of AGN feedback

Open Access

Fig. 3.

Distribution of sources in the SFR–M_* plane. Different AGN populations are presented with different colors and lines, as indicated in the legend of the plot. The solid gray line shows the local SFR–M_* relation presented in Elbaz et al. (2007) for SDSS galaxies.

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