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Table 3:

Properties of the B2 sample.
Name $F_{\rm 1.4~GHz}$ $F_{\rm core}$ $F_{\rm [O~III]}$ $P_{\rm c}$
B2 0055+30 30.93a 30.46 39.45a 0.34
B2 0222+36 30.60b 30.46 40.63b 0.72
B2 0722+30 29.93c 29.55 - 0.42
B2 1101+38 31.18d 31.04 40.54c 0.72
B2 1557+26 30.67a 30.06 39.64d 0.25
B2 1638+32 32.11a 31.38 40.59d 0.19
B2 1652+39A 31.53d 31.43 40.65e 0.79
B2 2116+26 30.03d 29.38 39.44f 0.22

Column description: (1) name; (2) total luminosity at 1.4 GHz in \ensuremath{{\rm erg}~{\rm s}^{-1}~{\rm Hz}^{-1}}. Reference: (a) White & Becker (1992); (b) Condon et al. (1998); (c) Becker et al. (1995b); (d) Condon et al. (2002); (3) core luminosity at 5 GHz in \ensuremath{{\rm erg}~{\rm s}^{-1}~{\rm Hz}^{-1}} from Giovannini et al. (1988); (4) nuclear [O III] luminosity in erg s-1. Reference: (a) Ho et al. (1997); (b) Buttiglione et al. (2010); (c) [O III] equivalent width from Jansen et al. (2000) and $\lambda$5007 continuum from Marcha et al. (1996); (d) from SDSS spectrum; (e) from Ha + [N II] measurement of Marcha et al. (1996) adopting [O III]/(H$\alpha $ + [N II]) $\sim$ 0.38 (H$\alpha $/[O III] = 1 and [N II]/H$\alpha $ = 1.6) (Buttiglione et al. 2009b); (f) from H$\alpha $ + [N II] image (Capetti et al. 2005) with emission line ratios specified above; (5) core dominance, $P_{\rm c} = P_{\rm core} / L_{1.4}$.


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