\begin{table}%t3
\caption{\label{b2}Properties of the B2 sample.}
\par
%\centerline
{
\begin{tabular}{l | c c c c}
\hline\hline
Name  & $F_{\rm 1.4~GHz}$ & $F_{\rm core}$ & $F_{\rm [O~III]}$ & $P_{\rm c}$ \\
\hline	                              
   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 \\
\hline
\end{tabular}}
\par
\medskip 
Column description: (1) name; (2) total luminosity at 1.4 GHz in
  \ergsHz. Reference: (a) \citet{white92}; (b) \citet{condon98}; (c) \citet{FIRST};
  (d) \citet{condon02}; (3) core luminosity at 5 GHz in \ergsHz\ from
  \citet{giovannini88}; (4)~nuclear [O~III] luminosity in erg s$^{-1}$. Reference:
  (a) \citet{ho97}; (b)~Buttiglione et al. (2010); (c) [O~III] equivalent
  width from \citet{jansen00} and $\lambda$5007 continuum from
  \citet{marcha96}; (d) from SDSS spectrum; (e) from Ha + [N~II] measurement of
  \citet{marcha96} adopting [O~III]/(H$\alpha$ + [N~II]) $\sim$ 0.38
  (H$\alpha$/[O~III] = 1 and [N~II]/H$\alpha$ = 1.6) \citep{buttiglione09b}; (f)
  from H$\alpha$ + [N~II] image \citep{capetti:cccriga} with emission
  line ratios specified above; (5)~core dominance, $P_{\rm c} = P_{\rm
    core}/L_{1.4}$.\vspace*{-2.5mm}
\end{table}