\begin{table}%t3
\caption{\label{tvlapar}Parameters of the continuum sources detected in the IRAS 00213+6530 region.}
%\centerline
{\begin{tabular}{lccccc}
\hline\hline
&\multicolumn{2}{c}{Position$^{\rm a}$}&	Flux Density&	Flux
Density&	Spectral\\
\cline{2-3}
&$\alpha$ (J2000) &$\delta$ (J2000) &at 6~cm &at 3.6~cm &Index\\
Source&	(h m s)& ($\degr$ $'$ $''$)& (mJy)& (mJy)& 6~cm--3.6~cm \\
\hline\noalign{\smallskip}
1&  00 23 21.01& $+$65 43 46.5&  0.87~$\pm$~0.07& \ldots$^{b}$&             \ldots\\
2&  00 23 45.65& $+$65 48 36.1&  0.17~$\pm$~0.03& $<$0.18$^{c}$&         $<$0.10\\
3&  00 23 46.41& $+$65 49 12.7&  1.66~$\pm$~0.04& 0.38~$\pm$~0.07$^{d}$&   $-$2.7~$\pm$~0.3\\
4&  00 23 49.01& $+$65 46 14.7&  0.69~$\pm$~0.03& 0.42~$\pm$~0.02&                $-$0.9~$\pm$~0.1\\
5&  00 23 52.06& $+$65 39 58.9&  4.20~$\pm$~0.60& \ldots$^{b}$&             \ldots\\
6&  00 23 53.70& $+$65 49 41.6&  0.86~$\pm$~0.03& $<$0.25$^{c, d}$&      $<$$-2.1$\\
7&  00 24 09.11& $+$65 46 58.0&  0.57~$\pm$~0.03& 0.24~$\pm$~0.02&                $-$1.6~$\pm$~0.2\\
8&  00 24 11.39& $+$65 47 09.6&  0.16~$\pm$~0.03& 0.21~$\pm$~0.02&                \phb0.5~$\pm$~0.4\\
9&  00 24 24.46& $+$65 49 05.9&  0.13~$\pm$~0.03& 0.27~$\pm$~0.02&                \phb1.3~$\pm$~0.4\\
10& 00 24 36.71& $+$65 48 27.5&  0.55~$\pm$~0.03& 0.22~$\pm$~0.03&                $-$1.7~$\pm$~0.3\\
11& 00 24 56.70& $+$65 49 10.3&  0.63~$\pm$~0.05& \ldots$^{b}$&             \ldots\\
12& 00 25 24.75& $+$65 45 48.3&  4.90~$\pm$~1.10& \ldots$^{b}$&             \ldots\\
\hline
\end{tabular}}
\medskip
$^a$~Positions taken from the 3.6~cm map, except for
non-detected sources at this band, for which positions correspond to
the 6~cm map.
$^b$~Source well outside the primary beam at this wavelength. Primary beam correction greater than
12, and the uncertainty in the corrected flux is very large.
$^c$~The upper limit for non-detected sources is 4$\sigma$.
$^d$~Flux density measured in 2000 September 23. Source 
highly variable, so to compute the spectral index we used
observations carried out at the same epoch.
\end{table}