Fig. 23.

Stellar mass vs 1.4 GHz radio luminosity for RL HERGs (blue dots) and LERGs (open red squares) at z < 1.3 with Mi < −22. The semi-transparent cyan squares and magenta circles show the RL HERGs and LERGs, respectively, that would have been selected by the cuts that Pracy16 made (Mi < −23 and S1.4 GHz > 2.8 mJy). The latter galaxies are some of the most massive, most radio luminous in the XXL-S sample.
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