\begin{table}%t2
\caption{Details of the newly detected 6.7~GHz CH$_{3}$OH masers. The first column lists the source name (associated IRAS source or the galactic coordinates). The next two
columns give their J2000 equatorial coordinates. Column~(4) shows the
distances. Columns~(5) and (6) present the integrated flux density and
peak flux density. Columns~(7) and (8) show the radial velocity of peak emission
and the radial velocity range. Columns~(9)--(11) present the
infrared, CH$_{3}$OH and H$_{2}$O luminosities. The maser luminosities are
calculated assuming isotropic emission.}
         \label{tab2}
\par
\small%\centerline
 {
           \begin{tabular}{ccccccccccc}
             \hline \hline
{\parbox[t]{20mm}{%\centering
 Source \\ name}}&
{\parbox[t]{17mm}{%\centering
 RA(2000)\\
\mbox{${\rm (^h\;\;\;^m\;\;\;^s)}$}}}&
{\parbox[t]{17mm}{%\centering
 Dec(2000) \\
\mbox{$(\degr\;\;\;\arcmin\;\;\;\arcsec)$}}}&
{\parbox[t]{10mm}{%\centering
 $D$ \\(kpc)}}&
{\parbox[t]{15mm}{%\centering
 $S_{\rm i}$\\(Jy~km~s$^{-1}$)}}&
{\parbox[t]{10mm}{%\centering
 $S_{\rm p}$\\(Jy)}}&
{\parbox[t]{10mm}{%\centering
 $v_{\rm p}$\\(km~s$^{-1}$)}}&
{\parbox[t]{12mm}{%\centering
 $\Delta v$
\\(km~s$^{-1}$)}}&{\parbox[t]{10mm}{%\centering
\par
$L_{\rm IR}$\\($L_{\odot}$)}}& {\parbox[t]{12mm}{%\centering
\par
$L_{{\rm CH}_{3}{\rm OH}}$\\($L_{\odot}$)}}& {\parbox[t]{10mm}{%\centering
\par
$L_{{\rm H}_{2}{\rm O}}$\\($L_{\odot}$)}} \\[4mm]
\hline 
 $05137+3919$  & $05\ 17\ 13.3$ & $+$39\ 22\ 14 &  $12.0^{1}$& 0.7 & 1.5 & $-$16.2 & $-$21.1, $-$16.0  & 6.1(4)        & 7.0($-$7)         & 2.2($-$4) \\
 $06446+0029$  & $06\ 47\ 12.9$ & $+$00\ 26\ 07 &  $6.0^{1}$ & 2.8 & 1.6 &    48.6 &    42.7, 50.0     & 2.3(4)        & 7.0($-$7)         & 1.5($-$4) \\
 $18319-0802$  & 18\ 34\ 38.2 & $-$07\ 59\ 35 &  $2.8^{\ast}$  & 2.2 & 2.1 &    35.7 &    31.0, 45.2     & 7.2(3)        & 1.2($-$7)         & 4.5($-$6) \\
 $18355-0650$  & 18\ 38\ 14.3 & $-$06\ 47\ 47 &  $5.7^{4}$ & 4.2 & 3.9 &    58.2 &    56.6, 62.1     & 7.4(5)        & 9.4($-$7)         & 7.1($-$6) \\
 $18403-0440$  & 18\ 43\ 01.1 & $-$04\ 36\ 41 &  $3.3^{4}$ & 0.3 & 1.0 &    20.1 &    19.8, 20.4     & 4.1(3)        & 2.3($-$8)         & 3.2($-$6) \\
 $G29.91-0.05$ & 18\ 46\ 05.9 & $-$02\ 42\ 27 &  $7.1^{\ast}$  & 7.8 & 2.9 &   104.3 &    93.4, 105.3    &  $---$          & 2.7($-$6)         & 3.3($-$5) \\
 $18479-0005$  & 18\ 50\ 31.1 & $-$00\ 01\ 54 &  $13.0^{2}$& 1.3 & 1.5 &    27.4 &    24.9, 28.3     & 1.6(6)        & 1.5($-$6)         & 9.0($-$5) \\
 $20275+4001$  & 20\ 29\ 24.9 & $+40$\ 11\ 21 &  $2.0^{3}$ & 1.7 & 4.0 &  $-$6.9 &  $-$7.4, $-$6.5   & 6.7(4)        & 4.7($-$8)         & 1.5($-$5) \\
 $21306+5540$  & 21\ 32\ 13.0 & $+55$\ 52\ 56 &  $8.6^{1}$ & 1.5 & 1.1 & $-$69.9 &  $-$73.7, $-$68.0 & 1.4(5)        & 7.8($-$7)         & 9.9($-$4) \\
 $22176+6303$  & 22\ 19\ 18.3 & $+63$\ 18\ 48 &  $0.9^{6}$ & 0.2 & 0.5 &  $-$2.0 &  $-$2.3, $-$1.1   & 2.4(4)        & 1.1($-$9)         & 4.8($-$7) \\
\hline
\end{tabular}}
\medskip      
 References for the distances:\\
 1  Wouterloot et~al. (1993). 2   Palagi et~al. (1993).  3  Anglada et~al. (1996).  4  van der Tak et~al. (1999).  5  Wu et~al. (2006).  6  Crampton \& Fisher (1974). \\
$^{\ast}$ Heliocentric near kinematic distances.
\end{table}