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\begin{document}
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\begin{table*}
\begin{center}
{\bf Table 1.} Line parameters for detected sources.
\end{center}
\label{cap1}
%\vspace{0.5cm}
\begin{tabular}{lrrrrrrrrl}
\hline
& & & & & & & & & \\
Source & \multicolumn{1}{c}{$\alpha_{1950}$} & 
\multicolumn{1}{c}{$\delta_{1950}$}
& \multicolumn{1}{c}{$\int {\rm S} dv$\footnotemark[1]} & 
\multicolumn{1}{c}{$v_{LSR}$\footnotemark[2]} & 
\multicolumn{1}{c}{$\Delta v$\footnotemark[2]} & 
\multicolumn{1}{c}{$\Delta \alpha ('')$\footnotemark[3]} & 
\multicolumn{1}{c}{$\Delta \delta ('')$\footnotemark[3]} & 
\multicolumn{1}{c}{$\theta ('')$\footnotemark[4]} & Notes \\
& & & \multicolumn{1}{c}{(Jy.kms$^{-1}$)} & 
\multicolumn{1}{c}{(kms$^{-1}$)} & 
\multicolumn{1}{c}{(kms$^{-1}$)} & & & & \\
& & & & & & & & & \\
\hline
& & & & & & & & & \\

W3(3) & $ \rm{02^{h}22^{m}06^{s}.1}$ & $61^{\circ}50'40''$ 
  & 3.3(0.8) & $-$39.3(1.0) & 7.5(2.0) & $-$15 &  15 
& \multicolumn{1}{c}{------} & \footnotemark[5] \\
& & & & & & & & & \\

W3(OH) & 02 23 16.5 & 61 38 57 
  & 4.2(0.4) & $-$46.3(0.2) & 2.2(0.2) & $-$15(1) & $-$13(1) 
& 10(2) & \\
& & & & & & & & & \\

Orion-KL & 05 32 47.0 & $-$05 24 23
  & 19.1(1.9) & 7.8(0.8) & 5.0(1.7) & $-$5(2) & $-$5(2) 
& 30(2) &  \\
& & & 23.5(1.8) & 7.6(0.2) & 1.7(0.5) & 0(2) & $-$10(2) 
& 30(2) &  \\
& & & 4.2(0.3) & 7.05(0.05) & 0.24(0.05) & 10(1) & $-$15(1) & 
P \hspace{7mm} & \\
& & & 5.1(0.7) & 7.55(0.05) & 0.5(0.1) & 16(2) & $-$10(2) & 
P \hspace{7mm} & \\
& & & & & & & & & \\

Orion S & 05 32 44.8 & $-$05 26 00
  & 8.5(0.5) & 6.3(0.2) & 3.2(1.0) & 15 & $-$10 & 
\multicolumn{1}{c}{------} & \footnotemark[6] \\
& & & 1.9(0.5) & 6.1(0.2) & 0.9(0.2) & 10(2) & 0(2) & 
\multicolumn{1}{c}{------} & \footnotemark[6] \\
& & & & & & & & & \\

OMC2  & 05 32 59.6 & $-$05 11 32
  & 2.5(0.1) & 11.1(0.05) & 0.25(0.05) & 0(1) & 1(1) & P \hspace{7mm} & \\
& & & & & & & & & \\


S231 & 05 35 51.3 & 35 44 16
    & 1.7(0.1) & $-$16.0(0.05) & 0.4(0.1) & $-$15(1) & 1(2) & P \hspace{7mm} & \\
& & & 6.3(0.5) & $-$15.9(0.1)  & 2.2(0.2) & $-$9(2)  & 2(2) & P \hspace{7mm} & \\
& & & 4.2(1.2) & $-$20.7(0.7)  & 4.0(1.5) & $-$7(2)  & $-$15 &
\multicolumn{1}{c}{------} & \footnotemark[5]$^,$ \footnotemark[6] \\
& & & 0.4(0.1) & 1.3(0.1) & 0.4(0.1) & 
$-$7 & $-$15 &
\multicolumn{1}{c}{------} & \footnotemark[5]$^,$ \footnotemark[6] \\
& & & & & & & & & \\

S235B & 05 37 31.8 & 35 40 18
    & 2.1(0.3) & $-$16.7(0.1) & 0.4(0.1) & $-$2(2) & $-$9(2) & P \hspace{7mm} & \\
& & & 5.4(0.6) & $-$17.1(0.2) & 1.8(0.3) & 0(1) & 0(1) & P \hspace{7mm} & \\
& & & & & & & & & \\

NGC 2024 & 05 39 11.4 & $-$01 55 59
    & 1.7(0.5) & 9.9(0.4) & 2.1(0.8) & 0 & 0
& \multicolumn{1}{c}{------} & \footnotemark[5] \\
& & & & & & & & & \\

NGC 2071 & 05 44 30.0 & 00 20 40
    & 13.2(1.2) & 15.5(0.3) & 4.0(1.5) & 3(2) & $-$16(2) & 23(5) & 
\footnotemark[7] \\
& & & 8.0(0.6) & 14.5(0.1) & 0.4(0.1) & 2(2) & $-$16(2) & P \hspace{7mm} & \\
& & & 6.1(1.2) & 14.9(0.2) & 0.7(0.2) & 17(3) & $-$17(2) & P \hspace{7mm} & \\
& & & 5.4(0.4) & 15.9(0.1) & 0.5(0.1) & 10(2) & $-$16(2) & P \hspace{7mm} & \\
& & & 2.9(0.4) & 16.5(0.2) & 0.5(0.1) & 3(2) & $-$16(2) & P \hspace{7mm} & \\
& & & & & & & & & \\

G188.9 & 06 05 54.0 & 21 39 09
    & 4.6(1.1) & 3.8(0.4) & 3.3(0.6) & $-$15(2) & $-$24(2) & 10(3) & \\
& & & 4.9(1.1) & 2.8(0.3) & 1.3(0.4) & $-$22(2) & $-$30(2) & P \hspace{7mm} & \\
& & & 0.7(0.2) & 1.8(0.1) & 0.3(0.1) & $-$16(2) & $-$36(2) & P \hspace{7mm} & \\
& & & & & & & & & \\

NGC 2264 (IRS1) & 06 38 24.9 & 09 32 28
    & 4.3(0.3) & 7.1(0.1) & 0.3(0.1) & $-$9(1) & $-$2(1) & P \hspace{7mm} & \\
& & & 2.4(0.3) & 7.4(0.1) & 0.3(0.1) & $-$12(1) & 2(1) & P \hspace{7mm} & \\
& & & 4.3(1.0) & 7.6(0.6) & 3.1(0.9) & 
\multicolumn{1}{c}{------} &
\multicolumn{1}{c}{------} &
\multicolumn{1}{c}{------} & \footnotemark[7] \\
& & & & & & & & & \\

ROPHS1 & 16 23 32.7 & $-$24 16 44
    & 1.3(0.3) & 3.7(0.1) & 0.8(0.2) & 0 & 15 &
\multicolumn{1}{c}{------} & \footnotemark[5] \\
& & & & & & & & & \\

$\rho$ Oph & 16 24 10.0 & $-$24 22 42
   & 2.8(0.4) & 3.4(0.2) & 0.8(0.2) & 
\multicolumn{1}{c}{------} &
\multicolumn{1}{c}{------} &
\multicolumn{1}{c}{------} & \footnotemark[7] \\
& & & & & & & & & \\

Sgr A-G & 17 42 27.3 & $-$29 04 36 
    & 144(22) & 10.7(2.8) & 8.2(1.3) & $-$15 & 0 & 
\multicolumn{1}{c}{------} & \footnotemark[6]$^,$ \footnotemark[8] \\
& & & 70(12) & 2.7(2.5) & 11.1(3.0) & 0 & 0 & 
\multicolumn{1}{c}{------} & \footnotemark[8] \\
& & & 85(11) & 12.5(0.4) & 4.9(1.2) & 0 & 0 &
\multicolumn{1}{c}{------} & \footnotemark[8] \\
& & & 70(5) & 10.8(0.2) & 2.6(0.7) & $-$15 & 15 & 
\multicolumn{1}{c}{------} & \footnotemark[6]$^,$ \footnotemark[8] \\
& & & 44(7) & 6.7(0.2) & 2.9(0.3) & $-$15 & $-$15 &
\multicolumn{1}{c}{------} & \footnotemark[6]$^,$ \footnotemark[8] \\
& & & & & & & & & \\

Sgr A-F & 17 42 27.4 & $-$29 02 18 
    & 21.7(1.5) & 16.3(0.1) & 0.5(0.1) & $-$12(2) & $-$10(2) & P \hspace{7mm} & 
\footnotemark[9] \\
& & & 19.9(1.6) & 27.4(0.1) & 0.5(0.1) & $-$9(2) & $-$14(2) & P \hspace{7mm} & \\
& & & 12.9(1.4) & 20.4(0.1) & 0.4(0.1) & 2(2) & $-$13(2) & P \hspace{7mm} & \\
& & & 9.3(1.3) & 20.0(0.1) & 0.4(0.1) & 2(2) & $-$16(2) & P \hspace{7mm} & \\
& & & 7.5(1.5) & 16.9(0.1) & 0.7(0.1) & $-$13(1) & $-$13(2) & P \hspace{7mm} & \\
& & & 7.4(1.0) & 26.9(0.1) & 0.4(0.1) & $-$13(2) & $-$17(2) & 13(2) & \\
& & & & & & & & & \\
\hline
\end{tabular}
\end{table*}
\clearpage
\begin{table*}[ht]
\begin{center}
{\bf Table~1.} --- continued
\end{center}
\begin{tabular}{lrrrrrrrrl}
\hline
& & & & & & & & & \\
Source & \multicolumn{1}{c}{$\alpha_{1950}$} & 
\multicolumn{1}{c}{$\delta_{1950}$}
& \multicolumn{1}{c}{$\int {\rm S} dv$\footnotemark[1]} & 
\multicolumn{1}{c}{$v_{LSR}$\footnotemark[2]} & 
\multicolumn{1}{c}{$\Delta v$\footnotemark[2]} & 
\multicolumn{1}{c}{$\Delta \alpha ('')$\footnotemark[3]} & 
\multicolumn{1}{c}{$\Delta \delta ('')$\footnotemark[3]} & 
\multicolumn{1}{c}{$\theta ('')$\footnotemark[4]} & Notes \\
& & & \multicolumn{1}{c}{(Jy.kms$^{-1}$)} & 
\multicolumn{1}{c}{(kms$^{-1}$)} & 
\multicolumn{1}{c}{(kms$^{-1}$)} & & & & \\
& & & & & & & & & \\
\hline
& & & & & & & & & \\

Sgr A-A & 17 42 41.3 & $-$28 58 18 & 
\multicolumn{7}{c}{see Table~4} \\
& & & & & & & & & \\

Sgr B2 & 17 44 10.6 & $-$28 22 03 & 
\multicolumn{7}{c}{see Table~3} \\
& & & & & & & & & \\

Sgr D & 17 45 32.1 & $-$28 00 45
    & 16.0(1.1) & 75.0(0.8) & 9.9(1.5) & 30 & 30 & 
\multicolumn{1}{c}{------} & \footnotemark[6] \\
& & & 5.6(0.8) & $-$15.7(0.2) & 3.0(0.4) & 0(3) & $-$6(3) & P \hspace{7mm} & weak \\
& & & & & & & & & \\

G5.89--0.39 & 17 57 26.8 & $-$24 03 56
    & 4.2(0.7) & 9.0(0.1) & 0.5(0.2) & 11(3) & 12(2) & P \hspace{7mm} & \\
& & & 2.5(0.4) & 8.4(0.2) & 0.7(0.2) & 1(2) & 2(2) & P \hspace{7mm} & \\
& & & 1.9(0.4) & 8.3(0.1) & 0.4(0.1) & 17(2) & 5(2) & P \hspace{7mm} & \\
& & & 2.4(0.6) & 11.5(0.1) & 0.4(0.1) & $-$20(2) & 10(2) & P \hspace{7mm} & \\
& & & 1.8(0.4) & 12.22(0.05) & 0.35(0.05) & $-$15(2) & 7(2) & P \hspace{7mm} & \\
& & & & & & & & & \\

G8.67--0.36 & 18 03 18.7 & $-$21 37 53
    & 16.6(1.0) & 35.6(0.8) & 6.8(1.4) & $-$3(2) & 3(2) & 33(3) & \\
& & &  7.5(1.0) & 35.5(0.2) & 1.6(0.4) & 6(1) & 7(1) & P \hspace{7mm} & \\
& & &  2.1(0.4) & 35.7(0.1) & 0.4(0.1) & $-$1(2) & 7(2) & P \hspace{7mm} & \\
& & &  1.3(0.3) & 37.6(0.1) & 0.4(0.1) & 4(1) & 9(1) & P \hspace{7mm} & \\
& & & & & & & & & \\

G10.30--0.15 & 18 05 57.9 & $-$20 06 26
    & 24.4(1.3) & 10.8(0.6) & 6.8(1.8) & $-$10(1) & $-$15(1) & 15(2) & \\
& & & 2.3(0.7) & 12.4(1.6) & 1.7(0.4) & $-$15(2) & 0(2) & P \hspace{7mm} & \\
& & & 0.8(0.2) & 13.4(0.1) & 0.5(0.1) & $-$15(2) & $-$11(2) & P \hspace{7mm} & \\
& & & & & & & & & \\

G10.6--0.4 & 18 07 30.7 & $-$19 56 29 
    & 15.4(1.6) & $-$6.8(1.4) & 5.4(2.0) & $-$3(3) & $-$2(3) & 
$\sim$25 & elongated \\
& & & 8.5(1.4) & $-$5.9(0.1) & 0.6(0.2) & 5(2) & 8(2) & P \hspace{7mm} & \\
& & & 6.9(1.6) & $-$6.5(0.2) & 0.9(0.2) & 6(2) & 8(2) & P \hspace{7mm} & \\
& & & 2.1(0.5) & $-$2.0(0.2) & 0.8(0.2) & $-$13 & 8 & 
\multicolumn{1}{c}{------} & \footnotemark[5]$^,$ \footnotemark[6] \\
& & & & & & & & & \\

G11.94--0.62 & 18 11 04.4 & $-$18 54 20 
    & 1.0(0.3) & 38.2(0.2) & 0.7(0.3) & $-$15 & $-$15 & 
\multicolumn{1}{c}{------} & \footnotemark[5] \\
& & & & & & & & & \\

W33-Met	  & 18 11 15.7 & $-$17 56 53 
    & 12.5(2.1) & 36.3(1.7) & 7.3(1.9) & 38 & 7 & 
\multicolumn{1}{c}{------} & \footnotemark[6] \\
& & & 5.9(0.5) & 32.5(0.1) & 0.5(0.1) & $-$4(1) & 1(1) & P \hspace{7mm} & \\
& & & 2.9(0.4) & 35.9(0.2) & 0.3(0.1) & $-$30(2) & $-$7(2) & P \hspace{7mm} & \\
& & & 1.0(0.2) & 27.3(0.2) & 0.3(0.1) & 27(1) & 0(1) & P \hspace{7mm} & \\
& & & & & & & & & \\

W42	  & 18 33 30.3 & $-$07 14 42 
    & 19.1(1.0) & 110.5(1.5) & 6.3(2.6) & 2(2) & 2(2) & 26(3) & 
\footnotemark[7] \\
& & & 4.0(0.3) & 114.7(0.1) & 0.4(0.1) & 2(1) & 14(1) & P \hspace{7mm} & \\
& & & 3.4(0.5) & 109.7(0.1) & 0.5(0.1) & $-$10(2) & 0(2) & P \hspace{7mm} & \\
& & & 1.4(0.3) & 113.8(0.1) & 0.3(0.1) & 0(1) & 15(1) & P \hspace{7mm} & \\
& & & 1.1(0.3) & 107.9(0.1) & 0.5(0.2) & 8(2) & $-$4(2) & P \hspace{7mm} & \\
& & & & & & & & & \\

G29.96--0.02 & 18 43 27.1 & $-$02 42 36 
    & 3.9(1.0) & 96.8(1.0) & 8.0(3.0) & 0 & 0 & 
\multicolumn{1}{c}{------} & \footnotemark[5] \\
& & & & & & & & & \\

G30.8--0.1   & 18 45 11.0 &  $-$01 57 57 
    & 106.0(1.2) & 98.1(1.0) & 4.9(0.9) & 0(2) & 10(2) & 13(2) & 
\footnotemark[7] \\
& & & 15.0(1.4) & 101.8(0.2) & 1.2(0.5) & 0(1) & $-$4(1) & P \hspace{7mm} & \\
& & & 6.1(0.4) & 96.4(0.1) & 0.5(0.2) & 0(1) & 17(1) & P \hspace{7mm} & \\
& & & 6.3(1.3) & 98.5(0.1) & 0.6(0.3) & 8(1) & $-$3(1) & P \hspace{7mm} & \\
& & & 2.0(0.5) & 94.9(0.1) & 0.8(0.1) & $-$27 & $-$15 & 
\multicolumn{1}{c}{------} & \footnotemark[5] \\
& & & & & & & & & \\

G34.3+0.2   & 18 50 46.2 &  01 11 12 
    & 12.4(2.1) & 58.4(0.6) & 4.8(1.9) & 
\multicolumn{1}{c}{------} &
\multicolumn{1}{c}{------} &
\multicolumn{1}{c}{------} & \footnotemark[7] \\
& & & 1.5(0.3) & 56.3(0.1) & 0.5(0.1) & $-$22(2) & 15(1) & P \hspace{7mm} & \\
& & & & & & & & & \\

G35.05--0.5  & 18 54 37.1 &  01 35 01 
    & 2.5(0.3) & 49.9(0.1) & 0.5(0.2) & $-$1(1) & 13(1) & P \hspace{7mm} & \\
& & & & & & & & & \\

W49N	  & 19 07 49.8 &  09 01 17 
    & 7.2(1.1) & 13.1(0.5) & 6.2(1.3) & $-$15 & $-$15 & 
\multicolumn{1}{c}{------} & \footnotemark[6] \\
& & & & & & & & & \\

G43.8--0.1	  & 19 09 31.2 &  09 30 51 
    & 3.2(0.7) & 44.4(0.5) & 4.6(1.1) & 0 & $-$15 & 
\multicolumn{1}{c}{------} & \footnotemark[5] \\
& & & & & & & & & \\
\hline
\end{tabular}
\end{table*}
\clearpage
\begin{table*}[ht]
\begin{center}
{\bf Table~1.} --- continued
\end{center}
\begin{tabular}{lrrrrrrrrl}
\hline
& & & & & & & & & \\
Source & \multicolumn{1}{c}{$\alpha_{1950}$} & 
\multicolumn{1}{c}{$\delta_{1950}$}
& \multicolumn{1}{c}{$\int {\rm S} dv$\footnotemark[1]} & 
\multicolumn{1}{c}{$v_{LSR}$\footnotemark[2]} & 
\multicolumn{1}{c}{$\Delta v$\footnotemark[2]} & 
\multicolumn{1}{c}{$\Delta \alpha ('')$\footnotemark[3]} & 
\multicolumn{1}{c}{$\Delta \delta ('')$\footnotemark[3]} & 
\multicolumn{1}{c}{$\theta ('')$\footnotemark[4]} & Notes \\
& & & \multicolumn{1}{c}{(Jy.kms$^{-1}$)} & 
\multicolumn{1}{c}{(kms$^{-1}$)} & 
\multicolumn{1}{c}{(kms$^{-1}$)} & & & & \\
& & & & & & & & & \\
\hline
& & & & & & & & & \\

W51e1/e2 & 19 21 26.2 &  14 24 37
    & 38.4(2.1) & 55.6(0.8) & 6.3(2.1) & $-$4(2) & 2(2) & 20(3) & \\
& & & 7.0(0.4) & 54.1(1.0) & 3.6(1.2) & 35(3) & $-$45(1) & 15(3) & (MM3) \\
& & & 1.8(0.2) & 56.5(0.1) & 0.3(0.1) & 40 & $-$65 & 
\multicolumn{1}{c}{------} & \footnotemark[6] \\
& & & 2.1(0.3) & 53.7(0.1) & 0.5(0.2) & 44(2) & $-$53(2) & P \hspace{7mm} & (MM2-MM3) \\
& & & 1.3(0.3) & 54.0(0.1) & 0.3(0.1) & 44(2) & $-$47(2) & P \hspace{7mm} & (MM2-MM3) \\
& & & 1.6(0.4) & 52.9(0.1) & 0.4(0.1) & 1(2) & 11(2) & P \hspace{7mm} & \\
& & & 1.2(0.2) & 64.0(0.1) & 0.3(0.1) & $-$10(1) & 65(1) & P \hspace{7mm} & (MM4) \\
& & & & & & & & & \\

W51-MM5	  & 19 21 20.5 &  14 24 12 
    & 20.4(0.7) & 67.3(0.8) & 6.5(1.6) & $-$4 & 15 & 
\multicolumn{1}{c}{------} & \footnotemark[6] \\
& & & 1.1(0.2) & 66.5(0.1) & 0.3(0.1) & $-$17 & 2 & 
\multicolumn{1}{c}{------} & \footnotemark[6] \\
& & & 0.6(0.2) & 67.2(0.1) & 0.2(0.1) & $-$17 & 5 & 
\multicolumn{1}{c}{------} & \footnotemark[5]$^,$ \footnotemark[6] \\
& & & & & & & & & \\

ON1	  & 20 08 09.9 &  31 22 42 
    & 2.6(0.4) & 10.9(0.2) & 2.6(0.6) & $-$15 & $-$15 & 
\multicolumn{1}{c}{------} & \footnotemark[6] \\
& & & & & & & & & \\

ON2	  & 20 19 50.0 &  37 16 30 
    & 2.9(0.4) & $-$2.2(0.2) & 2.5(0.4) & $-$15 & $-$15 & 
\multicolumn{1}{c}{------} & \footnotemark[6] \\
& & & & & & & & & \\

W75N	  & 20 36 50.4 &  42 27 01 
    & 5.3(0.7) & 9.3(0.5) & 2.6(0.9) & $-$1(2) & 2(2) & 30(3) & \\
& & & 1.8(0.4) & 10.0(0.2) & 0.6(0.2) & $-$20 & 0(1) & P \hspace{7mm} & \\
& & & & & & & & & \\

DR21-MM	  & 20 37 07.6 &  42 08 46 
    & 13.0(0.2) & $-$2.73(0.05) & 0.35(0.05) & $-$3(1) & 2(1) & P \hspace{7mm} & \\
& & & & & & & & & \\

DR21(OH)  & 20 37 14.1 &  42 12 12
    & 10.8(0.4) & $-$3.6(0.9) & 3.2(0.9) & 17(1) & $-$18(1) & 22(3) & \\
& & &  6.0(0.5) & $-$2.5(0.7) & 3.5(1.2) & 5(1) & $-$22(1) & 14(3) & \\
& & &  5.4(0.4) & 0.31(0.05) & 0.4(0.1) & $-$21(1) & $-$1(1) & P \hspace{7mm} & \\
& & &  4.4(0.8) & $-$0.2(0.1) & 0.6(0.2) & $-$10(1) & $-$1(1) & P \hspace{7mm} & \\
& & &  2.0(0.2) & $-$4.3(0.2) & 0.4(0.1) & 0(1) & $-$46(1) & P \hspace{7mm} & \\
& & &  1.6(0.3) & $-$1.7(0.1) & 0.6(0.2) & $-$10(1) & $-$7(1) & P \hspace{7mm} & \\ 
& & & & & & & & & \\

W75S(3)	  & 20 37 16.7 &  42 15 15 
    & 23.5(1.3) & $-$0.17(0.05) & 0.5(0.1) & $-$16(1) & $-$2(1) & P \hspace{7mm} & \\
& & & 12.1(1.9) & 0.3(0.1) & 1.1(0.3) & $-$16(1) & $-$4(2) & 20(3) & \\
& & & 7.8(0.6) & $-$4.2(0.5) & 2.8(1.2) & $-$7(2) & $-$3(1) & 15(3) & \\
& & & 2.7(0.3) & $-$3.4(0.1) & 0.5(0.1) & $-$3(1) & $-$15(1) & P \hspace{7mm} & \\
& & & 1.1(0.3) & $-$5.3(0.1) & 0.3(0.1) & 0(1) & 3(2) & P \hspace{7mm} & \\
& & & 0.4(0.1) & $-$4.3(0.1) & 0.2(0.1) & $-$15 & $-$30 & 
\multicolumn{1}{c}{------} & \footnotemark[5] \\
& & & & & & & & & \\

S140	  & 22 17 41.2 &  63 03 43 
    & 0.8(0.2) & $-$7.8(0.2) & 1.3(0.4) & 7 & $-$15 & 
\multicolumn{1}{c}{------} & \footnotemark[5] \\
& & & & & & & & & \\

NGC 7538  & 23 11 36.7 &  61 11 49 
    & 19.0(0.4) & $-$55.8(0.6) & 3.8(1.2) & 8(2) & $-$93(2) & 30(5) & 
NGC7538(S) \\
& & & 6.3(0.7) & $-$57.0(0.8) & 4.5(1.5) & $-$15(3) & $-$32(3) & 
\multicolumn{1}{c}{------} & \footnotemark[7] \\
& & & 1.7(0.3) & $-$57.2(0.1) & 0.5(0.2) & $-$35(2) & $-$47(1) &  
\multicolumn{1}{c}{------} & \footnotemark[7] \\
& & & 1.4(0.3) & $-$57.7(0.1) & 0.3(0.1) & $-$46(2) & $-$53(1) & P \hspace{7mm} & \\
& & & 2.2(0.5) & $-$54.3(0.3) & 1.2(0.4) & $-$24(3) & $-$47(2) & P \hspace{7mm} & \\
& & & 1.5(0.5) & $-$56.7(0.2) & 0.5(0.2) & $-$8(3) & $-$17(3) & P \hspace{7mm} & \\
& & & 0.7(0.1) & $-$51.5(0.1) & 0.3(0.1) & $-$29(2) & $-$50(1) & P \hspace{7mm} & \\
& & & & & & & & & \\
\hline
\end{tabular}
\vspace{0.2cm}

{\footnotesize $^1$ The integrated flux density (determined from 
spectral gaussian fit is the one at the peak position. If no
peak position was determined, it is the maximum integrated area at the 
different positions observed.}

{\footnotesize $^2$ 
The velocity (with respect to the l.s.r.) and width is the mean over
          the all the observed positions and the error is the
          statistical error of this mean.}

{\footnotesize $^3$ The position of the emission peak of the feature has been 
          determined by a spatial 2-dimension gaussian fit on the integrated 
          area of the line. The error is the error of the fit and does not 
          include pointing errors. When no fit was performed (line too weak, 
          extended or on the edge of the map), the position given is the 
          position where the maximum flux density has been detected.}

{\footnotesize $^4$ $\theta$ is the mean size of the source assuming a 
gaussian shape, 
          calculated from the mean of the minor and major axis half power width 
          of the elliptical 2-dimensional gaussian fitted on the line area 
          contour map (assuming a $26''$ HPBW for the telescope beam). 
A ``P" means a point-like source in our beam (i.e. $< 10''$).$\theta$ is not
given when the peak of the detected emission is on the edge of the map,
or when the 2-dimension gaussian fit was not performed (2 peaks, 
too extended, line too weak, ...).}

{\footnotesize $^5$ tentative detection. }

{\footnotesize $^6$ peak of the detected emission on the edge of the 
map. }

{\footnotesize $^7$ extended emission.}

{\footnotesize $^8$ map uncomplete.}

{\footnotesize $^9$ only the strongest narrow features are given 
(see text).}
\end{table*}


\end{document}

