\begin{table}%t3
\caption{\label{tab_ghzspec}Measured radio flux densities or peak brightnesses of \object{J1101+7225},
obtained with single-dish telescopes, local interferometers, and VLBI. The VLBI flux densities are our fitted core flux densities as presented in Tables~\ref{tab_gaussmod} and \ref{tab_britzfits}.}
 %\centerline
{
  \begin{tabular}{cccc}
\hline \hline
 Obs. type & Freq. [GHz] & Flux dens. [mJy] & \\
\hline 
 single-dish & 0.038 & \( (1.41\times 10^4\pm 800) \) & (a) \\
 single-dish & 0.178 & \( (3900\pm 600) \) & (b) \\
 single-dish & 1.4 & \( (1451\pm 30) \) & (c) \\
 single-dish & 2.7 & \( (1070\pm 35) \) & (d) \\
 single-dish & 5   & \( (858\pm 76) \) & (e) \\
 single-dish & 22  & \( (820\pm 100)\) & (f) \\
\hline 
 local interf. & 1.4 & $(748\pm 40)$/beam & (g), res~$\sim$~1.5$''$\\
 local interf. & 8.4 & $(349 \pm 20)$/beam & (h), res~$\sim$~0.2$''$ \\
\hline 
 VLBI & 1.66 & ($396\pm 20$) & EVN Feb. 2002\\
 VLBI & 2.3  & $(520\pm25)$/beam & B02, res~$\sim$~3~mas\\
 VLBI & 5  & ($139\pm7)$ & - 1991.4 - \\
 VLBI & 5  & $(282\pm14)$ & - 1993.4 - \\
 VLBI & 5  & $(337\pm17)$ & - 1996.6 - \\
 VLBI & 5  & $(439\pm22)$ & - 1999.9 - \\
 VLBI & 8.4  & $(383\pm20)$/beam & B02, res~$\sim$~1~mas\\
\hline
\end{tabular} }
\smallskip
{\em References and comments:} (a) Rees (\cite{Rees1990}), catalogue revised by Hales et~al. (\cite{Hales1995}); (b) Gower et~al. (\cite{Gower1967}); (c) White \& Becker (\cite{White1992}); (d) K{\"u}hr et~al.~(\cite{hr1981}); (e) Gregory et~al.~(\cite{Gregory1996}); (f) Ter{\" a}sranta et~al.~(\cite{sranta2001}); (g) Xu et~al.(\cite{Xu1995}) gave this peak brightness of a map, which was convolved to a circular beam of 1.5$''$ {\it FWHM}; (h) Patnaik et~al.~(\cite{Patnaik1992}) found this peak brightness to be 80\% of the total flux density of 436~mJy.\\
The  values are plotted over frequency in Fig.~\ref{fig_ghzflux}. 
For the interferometric observations 5\% flux density errors are given. 
\end{table}