\begin{table}%t1
\caption{\label{Tabiras}6.7-GHz methanol masers observed with ATCA.}
%\centerline
 {\small 
\begin{tabular}{lccrrrrccrr}
\hline \hline 
Source &  RA(2000) & Dec(2000) & $l$ & $b$ & $V_{\rm LSR}$ & $V_{\rm mol}$ &  $S_{\rm peak}$ &  $R$ & $d_{\rm far}$ & $d_{\rm near}$\\
name & ($^{\rm h}~^{\rm m}~^{\rm s}$) &  $(\degr~ \arcmin~\arcsec$) & ($\degr$) & ($\degr$) &  (km~s$^{-1}$) &  (km~s$^{-1}$) &   (Jy/beam) &  
 (kpc) &    (kpc) &     (kpc) \\
\hline
$G$8.832-0.028 &18\ 05\ 25.66 &--21\ 19\ 25.5 & 8.832 & --0.028 & --3.9 &   0.5(1)& 132.0 & 8.4 & 16.7($\pm$3.6) & 0.1($\pm$2.0) \\
$G$8.872-0.493 &18\ 07\ 15.32   &--21\ 30\ 54.4  &  8.872 & --0.493 &  23.4 &  &  30.9 & 4.9 & 13.2($\pm$1.1) & 3.6($\pm$1.1) \\
$G$14.101+0.087     &18\ 15\ 45.80   &--16\ 39\ 09.7  & 14.101 &  0.087 &  15.2 &   9.3(2) &  90.2 & 7.2 & 15.1($\pm$1.5) & 1.3($\pm$1.1) \\
&18\ 15\ 45.80   &--16\ 39\ 09.5  & 14.101 &  0.087 &   5.9 &          &  15.4 &     &              &             \\
&18\ 15\ 45.81   &--16\ 39\ 09.5  & 14.102 &  0.087 &  10.1 &          &  25.1 &     &              &             \\
&18\ 15\ 45.81   &--16\ 39\ 09.6  & 14.101 &  0.087 &  11.0 &          &  22.8 &     &              &             \\
&18\ 15\ 45.80   &--16\ 39\ 09.7  & 14.101 &  0.087 &  13.1 &          &  16.3 &     &              &             \\
&18\ 15\ 45.80   &--16\ 39\ 09.7  & 14.101 &  0.087 &  13.6 &          &  22.6 &     &              &             \\
$G$23.010-0.411     &18\ 34\ 40.29   &--09\ 00\ 38.1  & 23.010 & --0.411 &  74.8 &  74.8(2) & 415.4 & 4.4 & 10.8($\pm$0.5) & 4.9($\pm$0.5) \\
&18\ 34\ 40.29   &--09\ 00\ 38.2  & 23.010 & --0.411 &  72.7 &          &  43.4 &     &              &             \\
&18\ 34\ 40.28   &--09\ 00\ 38.4  & 23.010 & --0.411 &  80.6 &          &  49.1 &     &              &             \\
&18\ 34\ 40.28   &--09\ 00\ 38.4  & 23.010 & --0.411 &  81.6 &          &  52.0 &     &              &             \\
&18\ 34\ 40.27   &--09\ 00\ 38.5  & 23.010 & -0.411 &  82.3 &          &  43.4 &     &              &             \\
$G$23.207-0.378     &18\ 34\ 55.20   &--08\ 49\ 14.2  & 23.207 & --0.378 &  81.7 &          &  38.2 & 4.3 & 10.5($\pm$0.5) & 5.2($\pm$0.5) \\
&18\ 34\ 55.21   &--08\ 49\ 14.4  & 23.207 & --0.378 &  76.5 &          &  19.4 &     &              &             \\
&18\ 34\ 55.21   &--08\ 49\ 14.6  & 23.207 & --0.378 &  77.0 &          &  35.4 &  & & \\
$G$24.148-0.009&18\ 35\ 20.94& --07\ 48\ 55.6 & 24.148 & --0.009 &  17.7 &  23.1(3) &  26.8 & 6.7 & 13.5($\pm$0.8) & 2.0($\pm$0.8) \\
$G$24.329+0.144 &18\ 35\ 08.14   &-07\ 35\ 04.0  & 24.329 &  0.144 & 110.2 & 112.0(2) &   5.0 & 3.7 &  8.9($\pm$0.9) & 6.6($\pm$0.9) \\
$G$27.220+0.260 &18\ 40\ 03.72   &--04\ 57\ 45.6  & 27.220 &  0.260 &   9.3 &  &   6.2 & 7.8 & 14.3($\pm$0.9) & 0.8($\pm$0.8) \\
$G$27.365-0.166 &18\ 41\ 51.06   &--05\ 01\ 42.8  & 27.365 & --0.166 & 100.0 &  92.2(4) &  28.0 & 4.2 &  9.2($\pm$0.7) & 5.9($\pm$0.7) \\
&18\ 41\ 51.06&--05\ 01\ 42.8  & 27.365 & --0.166 &  98.0 & &  10.2 & & & \\
&18\ 41\ 51.06   &--05\ 01\ 42.8  & 27.365 & --0.166 &  98.9 & &  13.7 & && \\
&18\ 41\ 51.06   &--05\ 01\ 42.8  & 27.365 & --0.166 & 100.7 & & 14.2 & & & \\
&18\ 41\ 51.06   &--05\ 01\ 42.7  & 27.365 & --0.166 & 101.5 & &10.8 && & \\
$G$29.863-0.044     &18\ 45\ 59.57   &--02\ 45\ 04.4  & 29.863 & --0.044 & 101.4 & 100.4(4) &  76.5 & 4.3 &  8.2($\pm$0.8) & 6.6($\pm$0.8) \\
&18\ 45\ 59.57&--02\ 45\ 04.5 & 29.863 & --0.044 &100.3 & &  52.0 & &  & \\
&18\ 45\ 59.57 &--02\ 45\ 04.5  & 29.863 & --0.044 & 101.7 & & 54.2&&&\\
$G$30.199-0.169 &18\ 47\ 03.07 &--02\ 30\ 33.6 & 30.199 & --0.169 & 108.6 & 103.3(4) & 16.0 & 4.3 &  7.8($\pm$1.0) & 6.9($\pm$1.0) \\
$G$30.225-0.180 &18\ 47\ 08.30   &--02\ 29\ 27.1  & 30.225 & --0.180 & 113.5 & 104.5(4) &  10.8 & 4.3 & 7.7($\pm$1.1) & 7.0($\pm$1.1) \\
$G$30.899+0.162 &18\ 47\ 09.13   &--01\ 44\ 08.8  & 30.899 & 0.162 & 101.8 &   &  25.7 & 4.4 &  7.7($\pm$1.1) & 6.9($\pm$1.1) \\
&18\ 47\ 09.13   &--01\ 44\ 08.7  & 30.899 &  0.162 & 103.0 &&14.2&&&\\
\hline
\end{tabular}}
\medskip
The first column lists the source name. The next two columns give their J2000~equatorial coordinates. Columns~(4) and~(5) give their galactic coordinates. Columns~(6) and~(7) show the radial velocity of peak emission from the maser and molecular lines. Column~(8) presents the peak flux density. Columns~(9)--(11) present the distance from the Galactic center, and the far and near kinematic distances. \\
 References for the velocities: 
1~--~Zhang et~al. (\cite{Zhang2005});    2~--~Larionov et~al. (\cite{Larionov1999});    3~--~Szymczak et~al. (\cite{Szymczak2007}); 4~--~van der Walt et~al. (\cite{van2007}).
\vspace*{5mm}
\end{table}