\begin{table}%t4
\caption{\label{ta:noclump}Positions (J2000) and determined properties toward the positions without clumps.}                           
%\centering
\par
\begin{tabular}{l l r r r r r r r }
\hline\hline \noalign{\smallskip}
HEC name &  & \multicolumn{1}{c}{RA}     & \multicolumn{1}{c}{Declination} & \multicolumn{1}{c}{$d_{\rm kin}$}  &\multicolumn{1}{c}{$F^i_{{\rm 0.25 pc}}$}&\multicolumn{1}{c}{$M_{0.25~{\rm pc}}$} &\multicolumn{1}{c}{$T_{{\rm rot}}$} &\multicolumn{1}{c}{${N_{{\rm NH_3}}}$} \\
      &   & \multicolumn{1}{c}{(h:m:s)}  & \multicolumn{1}{c}{(\degr:~\arcmin:~\arcsec)} &(kpc)&(mJy)& \multicolumn{1}{c}{(${M_\odot}$)}  &\multicolumn{1}{c}{(K)} & \multicolumn{1}{c}{($10^{15}$~cm$^{-2}$)}\\
\hline
G012.73--00.58... &MM2   & 18:15:32.7   & --18:10:15  & 1.1&178  &8    & 11.4(0.7)  & ..    \\
G013.97--00.45... &MM1    & 18:17:16.5   & --17:01:16 & 2.4&189  &25   & 16.6(0.9)   & ..    \\
G014.39--00.75A.. &MM2   & 18:19:17.4   & --16:44:04  & 2.1&382  &32   & 20.0(2.3)  & ..     \\
G023.38--00.12... &MM2   & 18:34:20.4   &  --8:33:16  & 5.6&..   & 44  &17.8(2.0).    &..    \\
G025.79+00.81... &MM1   & 18:35:20.5   &  --5:56:36  & 3.4 &196 & 77  &  13.1(0.7) & .. \\
              &MM2   & 18:35:26.3   &  --5:59:21  & 3.4 & 63 &  31  & ..   &..\\
G034.03--00.33... &MM1   & 18:54:25.1   &   0:49:56  & ..  &..  & .. & .. &..  \\
              &2     & 18:54:39.2   &   0:51:37  & ..  &..  & .. & .. & .. \\
G034.34--00.90... &1      & 18:57:16.5   &   0:50:48 &..   &..  &..  &..\\
G034.77--00.81... &MM1    & 18:57:40.7  &   1:16:09 & 2.9   & 49 & 11  & ..   & ..\\
G034.85+00.43... &MM1    & 18:53:23.2  &   1:53:16 &3.6  & 73 & 31   &13.2(1.5)    & ..\\
G037.44+00.14A.. &MM1   & 18:59:14.0   &   4:07:37 &1.3  & 163 &  8  & ..   &..  \\
G037.44+00.14B..              &MM2   & 18:59:10.2   &   4:04:32 &1.7  & 130 &  ..  &  ..  &..\\
\hline
\end{tabular}
\tablefoot {The first two columns give the HEC name and the millimeter clump number, the following columns represent (in order of appearance): right ascension, declination, kinematic distance, integrated 1.2~mm flux within 0.25~pc diameter, mass within 0.25~pc diameter, \amm\ rotational temperature, and \amm\ column density.}
%\vspace*{5mm}
\end{table}