\begin{table}%t1
%\centering
\par
%\vspace{-0.5cm}
\caption { Parameters of the FR~1 galaxies, derived in the same
      way as by Haas et~al. (\cite{Haas04}).
      $L_{\rm eml}=L$(H$_\alpha$+[NII]) is adopted from Zirbel \& Baum
      (\cite{Zirbel95}).
      \label{msxxxx_tab_luminosities} 
    } 
%\vspace{-0.2cm}
\scriptsize
\begin{tabular}{@{\hspace{0.5mm}}r@{\hspace{1.1mm}}r@{\hspace{2.1mm}}r@{\hspace{2.1mm}}r@{\hspace{2.1mm}}r@{\hspace{2.1mm}}r@{\hspace{2.1mm}}r@{\hspace{1.1mm}}r@{\hspace{1.1mm}}r@{\hspace{1.1mm}}}
\hline\hline
      3CR & $D_{L}$ & $L_{\rm MIR}$  & $L_{\rm FIR}$& $P_{\rm 15~\mu m}$ & $P_{\rm 178~MHz}$ & $T_{\rm dust}$ & $M_{\rm dust}$ & $L_{\rm eml}$\\ 
      &   { Mpc}   &
      { log~[$L_{\odot}$]}&
      { log~[$L_{\odot}$]}&
      { log~[$W$]}&
      { log~[$W$]}&
      { [K]}&
      { log~[$M_{\odot}$] } & { log~[$W$]}\\
\hline
 31.0 & 70&$<$9.23& $<$9.84&$<$35.55&33.25&$\sim$24&$\sim$7.00&  ...\\
 66~B& 91&$<$8.85& $<$9.47&$<$35.10&33.64&$\sim$29&$\sim$6.23&  ...\\
 76.1 &136&$<$9.21& $<$9.97&$<$35.35&33.70&$\sim$28&$\sim$6.82&  ...\\
 84.0 & 74&   0.87&   10.80&   37.11&33.85&      35&      7.01&34.91\\
270.0 & 31&   8.84&    9.05&   35.10&33.03&      28&      5.81&32.76\\
272.1 & 12&   8.13&    8.33&   34.46&31.90&      27&      5.13&32.37\\
274.0 & 16&   8.43&    8.50&   34.72&32.56&      35&      4.75&33.47\\
293.0 &197&   9.98&   10.43&   36.32&34.04&      26&      7.41&34.55\\
296.0 &104&$<$9.24& $<$9.64&$<$35.57&33.45&$\sim$27&$\sim$6.51&  ...\\
305.0 &179&   9.97&   10.23&   36.29&34.04&      32&      6.66&33.12\\
338.0 &123&   9.29&$<$10.02&   35.52&34.21&      27&      6.95&33.77\\
\hline
\end{tabular}
\end{table}