\begin{table}%t2
\caption{\label{tab:HI_properties}Summary of the \ion{H}{i} properties.}
%\centerline
 {\small 
\begin{tabular}{cccccccccccccc}
 \hline \hline\noalign{\smallskip}
Object & $v_{\rm 0}$~(LSR) & $I_{\rm \ion{H}{i}}$$^a$ & $W_{\rm
50}$$^b$ & LS$^c$ & $M_{\rm \ion{H}{i}}$ & $M_{\rm dyn}$ &
$M_{\rm tot, gas}$ & $L^{\prime}$$_{\rm CO}$~/~$M_{\rm
\ion{H}{i}}$ & $L_{\rm IR}$  & \textit{f} & $\Sigma$$_{{M}}$ & $M_{\rm \ion{H}{i}}$$/$$L_{\rm IR}$ & $M_{\ion{H}{i}}$~/~$L_{\rm B}$ \\
\noalign{\smallskip}
&   [km~s$^{-1}$] & [Jy~km~s$^{-1}$] & [km~s$^{-1}$] & & [10$^{\rm 9}$~$M_{\sun}$] & [10$^{\rm 10}$~$M_{\sun}$] &
10$^{\rm 10}$~$M_{\sun}$] & [$\frac{\rm{K~km~s}^{\rm -1}{\rm pc}^{\rm 2}}{{M}_{\sun}}$] & [10$^{\rm 10}$~$L_{\sun}$] & & [$M_{\sun}$~pc$^{\rm -2}$] & [$M_{\sun}$~/~$L_{\sun}$] & [$M_{\sun}$~/~$L_{\sun}$] \\
 \hline 
 \object{HE~0045} & 6~403  & 3.29  $\pm$  0.13 & 180.8 & $\upuparrows$$_{\rm A}$ & 5.7 $\pm$ 0.2  & 7.1   & 11.5 & 0.13 & 8.10  & 0.6 & 20.0  & 0.08 & 1.2\\
 \object{HE~0150} & 14~329 & 2.70 $\pm$ 0.28 & 263.0 & $\upuparrows$$_{\rm A}$ & 23.8 $\pm$ 2.5 & 45.0  & 26.8 & 0.02 & 11.10 & 0.9 & 27.0  & 0.21 & 4.9\\
 \object{HE~0212} & 7~921  & 1.97 $\pm$ 0.18 & 206.4 & $\wedge$$_{\rm A}$      & 5.3 $\pm$ 0.5  & 3.3   & 11.7 & 0.09 & 4.07  & 1.1 & 121.6 & 0.13 & 0.4\\
 \object{HE~0224} & 18~150 & $2.64 \pm 0.26$ & 271.0 & $\sqcap$$_{\rm A}$      & 37.5 $\pm$ 3.7 & 90.8  & 41.5 & 0.01 & 10.50 & 0.3 & 20.3  & 0.34 & 3.8\\
\object{HE~0227} & 4914  & $2.58 \pm 0.16$ & 193.9 & $\sqcap$                & 2.6 $\pm$ 0.2  & 0.9   & 3.4  & 0.07 & 1.08  & 1.0 & 466.9 & 0.24 & 0.7\\
\object{HE~0232} & 12~886 & 3.31 $\pm$ 0.40 & 559.0 & $\wedge$$_{\rm A}$      & $23.6 \pm 2.8$ & 46.9  & 56.6 & 0.18 & 18.50 & 0.8 & 114.9 & 0.13 & 0.8\\
\object{HE~0949} & 5974  & 5.88 $\pm$ 0.46 & 181.4 & $\wedge$$_{\rm A}$      & 8.7 $\pm$ 0.7  & 3.5   & 9.5  & 0.01 & --  & 1.5 & 58.0  & -- & 1.7\\
\object{HE~1029} & 12~112 & $1.05 \pm 0.10$ & 241.0 & $\upuparrows$           & 6.6 $\pm$ 0.6  & 24.2  & 17.2 & 0.20 & 21.20 & 0.9 & 14.4  & 0.05 & 0.6\\
\object{HE~1237} & 2531  & $7.55 \pm 0.36$ & 355.5 & $\upuparrows$           & $2.0 \pm 0.1$  & 67.5  & 2.82 & 0.05 & 1.44  & 0.9 & 1.00  & 0.14 & 1.2\\
\object{HE~1248} & 4338  & $0.78\pm0.03$ & 119.5 & $\wedge$$_{\rm A}$& $1.2 \pm 0.2$$^d$ & 5.7 & 2.2 & 0.08 & 1.29  & 1.4 & 2.6  & 0.12 & 3.5\\
\object{HE~1330} & 6744  & $1.84 \pm 0.35$ & 180.4 & $\upuparrows$           & $3.6 \pm 0.7$  & 16.1  & 5.0  & 0.05 & --    & 1.0 & 6.3   & --   & 1.6\\
\object{HE~2302} & 14~120 & $1.39 \pm 0.18$ & 338.0 & $\upuparrows$$_{\rm A}$ & $11.9 \pm 1.5$ & 130.7 & 19.7 & 0.08 & --& 1.3 & 4.7& -- & 1.1\\
\noalign{\smallskip} \hline
\multicolumn{14}{c}{Non-detections}\\
\hline  
\object{HE~0021} & 15~889 & $<$2.03 & 222.7 &  & $<$22.2 &  & $<$2.4 & $>$0.01 & --   &  &  & --       & $<$4.1\\
\object{HE~0040} & 12~390 & $<$1.58 & 222.7 &  & $<$10.7 &  & $<$1.3 & $>$0.03 & --  & & & -- & $<$4.2\\
\object{HE~0114} & 13~672 & $<$1.75 & 222.7 &  & $<$14.0 &  & $<$1.7 & $>$0.03 & --   &  &  & -- & $<$2.5\\
\object{HE~0119} & 16~291 & $<$1.42 & 222.7 &  & $<$16.5 &  & $<$2.7 & $>$0.08 & 24.6 &  &  & $<$0.07 & $<$1.0\\
\object{HE~0253} & 9470  & $<$2.58 & 222.7 &  & $<$10.1 &  & $<$1.5 & $>$0.06 & 4.90 &  &  & $<$0.21 & $<$2.2\\
\object{HE~0433} & 10~658 & $<$2.21 & 222.7 &  & $<$10.7 &  & $<$2.9 & $>$0.21 & 22.7 &  &  & $<$0.05 & $<$1.1\\
\object{HE~0853} & 17~930 & $<$1.03 & 222.7 &  & $<$14.3 &  & $<$2.1 & $>$0.06 & --   &  &  & -- & $<$1.5\\
\object{HE~1011} & 17~388 & $<$0.56 & 222.7 &  & $<$7.5  &  & $<$1.5 & $>$0.12 & --   &  &  & --  & $<$0.2\\
\object{HE~1017} & 14~985 & $<$1.22 & 222.7 &  & $<$11.4 &  & $<$1.6 & $>$0.05 & 9.88 &  &  & $<$0.12 & $<$1.2\\
\object{HE~1107} & 17~088 & $<$1.03 & 222.7 &  & $<$13.6 &  & $<$1.8 & $>$0.04 & --   &  &  & --       & $<$0.8\\
\object{HE~1108} & 7199  & $<$0.50 & 222.7 &  & $<$1.1 & & $<$0.9 & $>$0.85 & 10.4 &  &  & $<$0.01 & $<$0.1\\
\object{HE~1126} & 17~988 & $<$1.83 & 222.7 &  & $<$25.7 &  & $<$3.4 & $>$0.04 & --   &  &  & --       & $<$0.5\\
\object{HE~1353} & 10~388 & $<$2.44 & 222.7 &  & $<$11.4 &  & $<$1.7 & $>$0.07 & --   &  &  & --       & $<$4.7\\
\object{HE~2222} & 17~431 & $<$1.22 & 222.7 &  & $<$15.9 &  & $<$1.7 & $>$0.01 & --   &  &  & --       & $<$3.7\\
\object{HE~2233} & 16~933 & $<$2.93 & 222.7 &  & $<$36.1 &  & $<$4.0 & $>$0.01 & --   &  &  & --       & $<$4.4\\
\noalign{\smallskip} \hline
%--------------------------------------------------------------------------
\end{tabular}}
\medskip
$^a$ Upper limits and errors represent 3$\sigma$ values; $^b$ for the non-detections, values of W$_{\rm 50}$ correspond to the median value of all detected sources; $^c$ line shape: $\wedge$ represents a triangular shaped line
profile; A stands for asymmetries in the line profiles; spectra with
$\sqcap$ show a boxy line profile; $\upuparrows$ mark line profiles
of a double-horn shape; $^d$~this detection was already confirmed by follow-up observations with the VLA. The obtained value for the \ion{H}{i} mass is $\sim$$1.0 \times 10^{\rm 9}$~$M_{\sun}$ \citep{koenig09}. 
\end{table}