\begin{table}%t3
\caption{\label{tpdb1mm}Parameters of the 1.2~mm subcondensations associated with MM1 from the uniform-weighted PdBI map\tablefootmark{a}.}
\vspace*{-2mm}
%\centerline
{\begin{tabular}{lccccccc}
\hline\hline\noalign{\smallskip}	
&\multicolumn{2}{c}{Position}
&$I_{\rm \nu}^{\rm peak}$\tablefootmark{b}
&$S_{\rm \nu}$\tablefootmark{b}
&Deconv. size\tablefootmark{c}
&PA\tablefootmark{c}
&M$_{\rm env}$\tablefootmark{d}
\\
\cline{2-3}
\noalign{\smallskip}
Source
&$\alpha (\rm J2000)$
&$\delta (\rm J2000)$
&(m\jpb)
&(mJy)
&($\arcsec\times\arcsec$)
&(\degr)
&(\mo)
\\
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
\hline
\noalign{\smallskip}
%-----------------------------------------------------------------------
MM1-main\tablefootmark{e}	&00 14 26.051	&64 28 43.69	&$12.8\pm1.1$	 &$39\pm6$	  &$3.2\pm1.8\times0.3\pm0.3$	&$-89\pm\phn5$	&1.46	\\
			&		&		&		 &		  &$2.1\pm0.9\times1.0\pm0.3$	&\phn$+3\pm13$	&	\\
%-----------------------------------------------------------------------
MM1-S			&00 14 26.065	&64 28 42.26	&\phn$4.7\pm1.1$ &\phn$5.4\pm1.4$ &$1.6\pm0.5\times0.8\pm0.2$	&$-30\pm30$	&0.20	\\
%-----------------------------------------------------------------------
MM1-SW			&00 14 25.861	&64 28 42.25	&\phn$5.9\pm1.1$ &\phn$6.4\pm1.5$ &$1.3\pm0.4\times0.2\pm0.1$	&$+85\pm\phn9$	&0.24	\\
\hline
\end{tabular}}
\vspace*{-2mm}
\tablefoot{\tablefoottext{a}{Synthesized beam of the uniform-weighted map is
  $0\farcs96\times0\farcs77$ with PA$=+66$\degr. The rms noise
  level of the map is 1.0~mJy~beam$^{-1}$.}
\tablefoottext{b}{Primary beam corrected. Error in intensity and flux density as in Table~\ref{tmultiwave}}.
\tablefoottext{c}{Deconvolved sizes and PA obtained from a fit
  with two Gaussian for MM1-main, and one single Gaussian for MM1-S and MM1-SW.}
\tablefoottext{d}{Masses derived assuming a dust mass opacity
  coeffecient at 1.2~mm of 0.9~g~cm$^{-1}$ (agglomerated grains with
  thin ice mantles in cores of densities $\sim$$10^6$~cm$^{-3}$,
  Ossenkopf \& Henning \cite{ossenkopfhenning1994}), and a dust temperature of 30~K.  The
  uncertainty in the masses due to the opacity law is estimated to be of
  a factor of 2.}
\tablefoottext{e}{Throughout all the text, we refer to MM1-main as MM1, for simplicity.}}
\vspace*{-1.5mm}
\end{table}