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Fig. 2

image

FIRST vs. [O III] line luminosity (erg s-1). The colored points represent the 12 galaxies observed with the JVLA coded as in Fig. 1. The small dot points correspond to the SDSS/NVSS sample studied by Baldi & Capetti (2010). The solid line represents the correlation between line and radio-luminosity derived for the 3CR/FR I sample. The dotted lines include the region where Seyfert galaxies are found. The empty pink triangles are the CoreG, and green stars the 3CR/FR Is.

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