Radio and spectroscopic properties of miniature radio galaxies: revealing the bulk of the radio-loud AGN population

R. D. Baldi; A. Capetti

doi:10.1051/0004-6361/200913021

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Volume 508 / No 2 (December III 2009)

A&A, 508 2 (2009) 603-614

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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	30.93^a	30.46	39.45^a	0.34
B2 0222+36	30.60^b	30.46	40.63^b	0.72
B2 0722+30	29.93^c	29.55	-	0.42
B2 1101+38	31.18^d	31.04	40.54^c	0.72
B2 1557+26	30.67^a	30.06	39.64^d	0.25
B2 1638+32	32.11^a	31.38	40.59^d	0.19
B2 1652+39A	31.53^d	31.43	40.65^e	0.79
B2 2116+26	30.03^d	29.38	39.44^f	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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