\begin{table}%t2
\caption {\label{tmultiwave}Multiwavelength results for the intermediate-mass YSOs in the star-forming region IRAS~00117+6412.}
\begin{tabular}{c l c c c c c c c}
\hline\hline\noalign{\smallskip}	
Wavelength
&
&Beam
&PA
&rms
&$I_\nu^{\rm peak}$\tablefootmark{a}
&$S_\nu$\tablefootmark{a}
&Deconv. size
&PA
\\
(cm)
&Instrument
&($\arcsec\times\arcsec$)
&($\degr$)
&($\mu$Jy~beam$^{-1}$)
&(mJy~beam$^{-1}$)
&(mJy)
&($\arcsec\times\arcsec$)
&($\degr$)
\\
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
\hline
\noalign{\smallskip}
\multicolumn{1}{l}{\uchii\ region}	&\multicolumn{2}{l}{$\alpha(J2000.0)=00^{\rm h}14^{\rm m}28\fs23$\tablefootmark{b}}	\\
					&\multicolumn{2}{l}{$\delta(J2000.0)=+64\degr28\arcmin46\farcs6$\tablefootmark{b}}		\\
\hline
\noalign{\smallskip}
6.0\phn\phe		&VLA-C		&$5.2\times4.0$		&\phn$-4$	&\phnn$30$
			&$1.21\pm0.03$	&$\phn1.72\pm0.08$	&$3.1\pm0.5\times2.7\pm0.4$	&\phn$95\pm50$	\\
3.6\phn\phe		&VLA-CD		&$3.8\times3.7$		&$+45$		&\phnn$30$
			&$1.03\pm0.03$	&$\phn1.88\pm0.09$	&$3.7\pm0.4\times3.1\pm0.4$	&\phn$10\pm60$	\\
3.6\phn\phe		&VLA-BCD	&$1.9\times1.7$		&$-70$		&\phnn$50$
			&$0.43\pm0.05$	&$\phn1.62\pm0.16$	&$3.9\pm0.4\times3.7\pm0.4$	&$180\pm60$	\\
1.3\tablefootmark{c}\phn     &VLA-D		&$5.9\times4.5$		&$-21$		&\phnn$70$
			&$0.59\pm0.07$	&$\phn1.7\pm0.2$	&$5.9\pm1.8\times5\pm2$\phn\phn\phn    	&$120\pm50$ \\
0.7\phn\phe		&VLA-D		&$4.0\times3.0$		&$+64$		&\phn$170$
			&$1.35\pm0.17$	&\phn$1.4\pm0.3$	&$2.7\pm1.2\times0.0$\phn\phn\phn\phn\phe &$150\pm30$	\\
0.32\phe		&PdBI-CD	&$4.3\times3.4$		&$+61$		&\phn$180$
			&\ldots			&\phn$<$$1$		&\ldots				&\ldots		\\
0.13\phe		&SMA-comp	&$3.2\times2.0$		&$+45$		&\phn$600$
			&\ldots			&\phn$<$$4$		&\ldots				&\ldots		\\
0.12\tablefootmark{d}	&PdBI-CD	&$1.5\times1.2$		&$+58$		&$1000$
			&\ldots			&$<$$25$		&\ldots				&\ldots		\\
\hline\hline
\noalign{\smallskip}
\multicolumn{1}{l}{MM1}	                &\multicolumn{2}{l}{$\alpha(J2000.0)=00^{\rm h}14^{\rm m}26\fs05$\tablefootmark{b}}	\\
					&\multicolumn{2}{l}{$\delta(J2000.0)=+64\degr28\arcmin43\farcs7$\tablefootmark{b}}		\\
\hline
\noalign{\smallskip}
6.0\phn\phe		&VLA-C		&$5.2\times4.0$		&\phn$-4$	&\phnn$30$
			&\ldots			&$<$$0.12$		&\ldots				&\ldots		\\
3.6\phn\phe		&VLA-CD		&$3.8\times3.7$		&$+45$		&\phnn$30$
			&$0.14\pm0.03$	&$0.17\pm0.07$	&$6.4\pm3.0\times3\pm2$\phn\phnn	&$120\pm30$	\\
3.6\phn\phe		&VLA-BCD	&$1.9\times1.7$		&$-70$		&\phnn$50$
			&$0.21\pm0.05$	&$0.15\pm0.06$	&$4.0\pm1.5\times2.2\pm1.5$	&$160\pm50$	\\
1.3\phn\phe		&VLA-D		&$5.9\times4.5$		&$-21$		&\phnn$70$
			&\ldots			&$<$$0.27$		&\ldots				&\ldots		\\
0.7\phn\phe		&VLA-D		&$4.0\times3.0$		&$+64$		&\phn$170$
			&\ldots			&$<$$0.69$		&\ldots				&\ldots		\\
0.32\phe		&PdBI-CD	&$4.3\times3.4$		&$+61$		&\phn$180$	
			&$4.16\pm0.19$	&$5.1\pm0.9$	&$3.2\pm0.4\times0.0$\phn\phn\phn\phn\phe       &\phn$75\pm10$	\\
0.13\phe		&SMA-comp	&$3.2\times2.0$		&$+45$		&\phn$600$
			&$51\pm1$\phn	&$71\pm14$	&$2.4\pm0.3\times1.0\pm0.2$	&\phn$50\pm10$	\\
0.12\tablefootmark{d}	&PdBI-CD	&$1.5\times1.2$		&$+58$		&$1000$
			&$21\pm1$\phn	&$65\pm10$	&$2.9\pm0.4\times1.6\pm0.4$	&\phn$25\pm10$	\\
\hline\hline
\noalign{\smallskip}
\multicolumn{1}{l}{MM2}			&\multicolumn{2}{l}{$\alpha(J2000.0)=00^{\rm h}14^{\rm m}26\fs31$\tablefootmark{b}}	\\
					&\multicolumn{2}{l}{$\delta(J2000.0)=+64\degr28\arcmin27\farcs8$\tablefootmark{b}}		\\
\hline
\noalign{\smallskip}
6.0\phn\phe		&VLA-C		&$5.2\times4.0$		&\phn$-4$	&\phnn$30$
			&\ldots			&$<$$0.12$		&\ldots				&\ldots		\\
3.6\phn\phe		&VLA-CD		&$3.8\times3.7$		&$+45$		&\phnn$30$
			&\ldots			&$<$$0.12$		&\ldots				&\ldots		\\
3.6\phn\phe		&VLA-BCD	&$1.9\times1.7$		&$-70$		&\phnn$50$
			&\ldots			&$<$$0.21$		&\ldots				&\ldots		\\
1.3\phn\phe		&VLA-D		&$5.9\times4.5$		&$-21$		&\phnn$70$
			&\ldots			&$<$$0.27$		&\ldots				&\ldots		\\
0.7\phn\phe		&VLA-D		&$4.0\times3.0$		&$+64$		&\phn$170$
			&\ldots			&$<$$0.69$		&\ldots				&\ldots		\\
0.32\phe		&PdBI-CD	&$4.3\times3.4$		&$+61$		&\phn$180$	
			&$2.8\pm0.2$	&$3.2\pm0.6$	&$1.6\pm1.0\times1.0\pm1.5$	&$160\pm50$	\\
0.13\phe		&SMA-comp	&$3.2\times2.0$		&$+45$		&\phn$600$
			&$19\pm1$\phn	&$24\pm5$\phn	&$2.0\pm0.5\times0.0$\phn\phn\phn\phn\phe           &$170\pm20$	\\
0.12\tablefootmark{d}	&PdBI-CD	&$1.5\times1.2$		&$+58$		&$1000$
			&$20\pm5$\phn	&$50\pm13$	&$3.5\pm1.0\times1.1\pm0.8$	&$140\pm30$	\\
\hline
\end{tabular}
\tablefoot{\tablefoottext{a}{Primary beam corrected (mainly affecting the
  millimeter data). In case of non-detection at one of the
  frequencies, an upper limit of 4$\sigma$ was used. Error in
  intensity is $1\sigma$. Error in flux density has been calculated as
  $\sqrt{(\sigma\sqrt{\theta_{\rm source}/\theta_{\rm beam}})^{2}+(\sigma_{\rm flux-scale})^{2}}$,
  where $\sigma$ is the rms noise level of the map,
  $\theta_{\rm source}$ and $\theta_{\rm beam}$ are the size of the
  source and the beam respectively, and $\sigma_{\rm flux-scale}$ is
  the error in the flux scale, which takes into account the uncertainty on
  the calibration applied to the flux density of the source
  ($S_\nu\times\%_{\rm uncertainty}$)}.
\tablefoottext{b}{Coordinates for the \uchii\ region, MM1, and MM2
  were measured in the VLA 3.6~cm, PdBI 1.2~mm, and SMA 1.3~mm images
  (Fig.~\ref{fi_cont}), respectively. Note that the coordinates of MM1
  correspond to the coordinates of MM1-main, listed in
  Table~\ref{tpdb1mm}.}  
\tablefoottext{c}{Data from S\'anchez-Monge
  \et\ (\cite{sanchezmonge2008}). Deconvolved size and PA correspond
  to the component VLA~3 from S\'anchez-Monge
  \et\ (\cite{sanchezmonge2008}), which is the component associated
  with the easternmost 2MASS source shown in Fig.~\ref{fi_cont}c.}
\tablefoottext{d}{1.2~mm PdBI continuum map done with natural
  weighting; for flux densities and coordinates for the different
  subcondensations detected in the uniform-weighted map, see
  Table~\ref{tpdb1mm}.}} 
\end{table}