\begin{table}%t4
\caption{\label{tn2hh}Parameters of the hyperfine fits to the \nth~(1--0) line.}
%\footnotesize
%\centerline
{\begin{tabular}{lccccccc}
%\noalign{\smallskip}
\hline\hline\noalign{\smallskip}
&&$A\tau_{\rm m}$\tablefootmark{b}
&Velocity\tablefootmark{c}
&Linewidth\tablefootmark{c}
&&$\Tex$
&$N$(\nth)
\\
Object
&Line\tablefootmark{a}
&(K~\kms)
&(\kms)
&(\kms)
&$\tau_{\rm m}$\tablefootmark{b}
&(K)
&(cm$^{-2}$)
\\
\noalign{\smallskip}
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
\hline\noalign{\smallskip}
MM1     &1	&$0.062\pm0.003$   &$-36.7$     &$0.66$   &$0.20\pm0.02$    &3.1  &$6.7\times10^{11}$\\
        &2      &$0.060\pm0.001$   &$-35.9$     &$1.40$   &$\lesssim$$0.1$    &3.4  &$8.5\times10^{11}$\\
MM1-NE  &1	&$0.072\pm0.003$   &$-36.7\pm0.1$&$0.68\pm0.02$&$0.15\pm0.02$&3.3  &$5.8\times10^{11}$\\
        &2      &$0.038\pm0.001$   &$-35.6\pm0.1$&$0.98\pm0.04$&$\lesssim$$0.1$&3.2  &$5.3\times10^{11}$\\
%MM1-S   &1      &$0.0426\pm0.0005$ &$-36.6$   &$0.87$   &$0.100\pm0.002$  &3.24  &$4.8\times10^{11}$\\
%        &2      &$0.0617\pm0.0005$ &$-35.7$   &$1.08$   &$0.100\pm0.001$  &3.46  &$6.6\times10^{11}$\\
%MM1-SW  &1      &$0.0437\pm0.0006$ &$-36.6$   &$0.93$   &$0.100\pm0.006$  &3.25  &$5.1\times10^{11}$\\
%        &2      &$0.0579\pm0.0006$ &$-35.8$   &$1.13$   &$0.100\pm0.001$  &3.41  &$6.7\times10^{11}$\\
MM2     &       &$0.031\pm0.001$   &$-34.9\pm0.1$&$1.49\pm0.05$&$\lesssim$$0.1$ &3.1 &$7.6\times10^{11}$\\
\hline
\end{tabular}}
\par
\tablefoot{
\tablefoottext{a}{For MM1 and the NE position of the MM1 ridge,
  the hyperfine structure is fitted with two velocity components.
  For MM2 the fit is made with one single velocity component.}
\tablefoottext{b}{$A=f[J_\nu(T_{\rm ex})-J_\nu(T_{\rm bg})]$. $\tau_{\rm m}$
  is the optical depth of the main hyperfine, adopted to be the
  $F_1F=23\rightarrow12$ line. The otpical depth of the isolated line
  can be obtained by multiplying $\tau_{\rm m}$ by the factor 3/7.}
\tablefoottext{c}{When errors are not given, the velocity and
  linewidth have been fixed from a fit of two Gaussian to the isolated
  line. When errors are given, the fit of two Gaussian to the isolated line
  was used to provide initial values for the velocity and linewidth
  of the hyperfine fit.}}
\end{table}