Fig. 2.

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L150 MHz of radio AGNs versus the ϵ and λRe of their host galaxies. The top panels show the L150 MHz of radio AGNs as a function of the ϵ of the host galaxies in three M⋆ bins (from left to right): log(M⋆/M⊙) = 11.2 − 11.5, 11.5 − 1.8, and > 11.8. The bottom panels show the L150 MHz as a function of the λRe of the host galaxies in three M⋆ bins. In all panels, the blue points denote radio AGNs from M22, and the red points denote radio AGNs from the BH12 sample.
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