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\begin{table}[t]
 \begin{center}
 \caption{Observations of the 6GHz OH maser transitions in AGB stars}
 \label{table1}
 \small
 \oddsidemargin -2cm
 \begin{tabular}{|c|c|c|c|c|c|c|}
 \hline
 \bf{IRAS Source}&\bf{Other Name}&\bf{Type\footnotemark}&\mc
{\bf{Observed Coordinates}}&\bf{Observed }&{\bf{Sensitivity
\footnotemark (Jy)}}\\ \bf{ }&\bf{ }&\bf{ }&\mc{\bf{J2000.0
\footnotemark}}&\bf{Velocity}&\bf{ (at 3$\sigma$) }\\
 \bf{ }&\bf{ }&\bf{ }&\bf{R.A.}&\bf{Dec.}&\bf{Range, LSR}&\bf{6GHz}\\
 \bf{ }&\bf{ }&\bf{ }&\bf{h m s}&\bf{${ }^0$ '
 ''}&\bf{(km.s$^{-1}$)}&\bf{LCP}\\
 \hline
 \rm
$02232+6138$ &W3(OH)&UCHII& 2:27:03.866 & $+$61:52:24.82 & -939/+998,($-$45.0)& E \\
$20081+3122$ &ON1&UCHII& 20:10:09.073 & $+$31:31:34.40 & -894/1043,($+$00.0)& E \\
 \hline
$00007+5524$ &Y Cas& Mira main& 00:03:21.605 & $+$55:40:48.21 & -911/1026,($-$17.0)&  0.08   \\
$01037+1219$ &IRC+10011& OH/IR Moderate& 01:06:25.965 & $+$12:35:53.07 & -886/1051,($+$08.0)&  0.07   \\
$02168-0312$ &OMI Cet& Mira main& 02:19:20.679 & $-$02:58:39.21 & -848/1089,($+$46.0)&  0.06   \\
$02192+5821$ &S Per& SG & 02:22:51.689 & $+$58:35:11.76 & -932/1005,($-$38.0)&  0.08   \\
$02251+5102$ &RR Per& Mira main& 02:28:29.318 & $+$51:16:17.60 & -894/1043,($+$00.0)&  0.08   \\
$02420+1206$ &RU Ari& Mira sat& 02:44:45.184 & $+$12:19:08.15 & -874/1063,($+$20.0)&  0.07   \\
$03206+6521$ &OH 138.0+7.2&OH/IR Moderate& 03:25:08.552 & $+$65:32:05.42 & -931/1006,($-$37.5)&  0.08   \\
$03293+6010$ &OH 141.0+3.5&OH/IR Moderate& 03:33:30.528 & $+$60:20:09.10 & -951/986,($-$57.2)&  0.07   \\
$03507+1115$ &IK Tau& Mira sat& 03:53:28.983 & $+$11:24:20.02 & -861/1076,($+$33.0)&  0.05   \\
$05073+5248$ &NV Aur&OH/IR Moderate& 05:11:19.747 & $+$52:52:27.79 & -891/1046,($+$02.9)&  0.08   \\
$05131+4530$ &RAFGL 712&OH/IR Moderate& 05:16:47.103 & $+$45:34:03.76 & -926/1011,($-$32.3)&  0.09   \\
$05528+2010$ &U\ Ori&Mira sat& 05:55:49.264 & $+$20:10:30.77 & -933/1004,($-$39.5)&  0.04   \\
$05559+7430$ &V Cam& Mira main& 06:02:32.779 & $+$74:30:27.26 & -887/1050,($+$06.5)&  0.07   \\
$06297+4045$ &OH 174.7+13.5&OH/IR Moderate& 06:33:14.921 & $+$40:42:49.71 & -910/1027,($-$16.3)&  0.08   \\
$06363+5954$ &U Lyn& Mira main& 06:40:46.320 & $+$59:52:00.23 & -904/1033,($-$10.0)&  0.07   \\
$06500+0829$ &GX Mon& Mira sat & 06:52:42.408 & $+$08:25:23.33 & -905/1032,($-$11.0)&  0.06   \\
$07209-2540$ &VY\ Cma&SG& 07:22:58.17 & $-$25:46:02.95 & -872/1065,($+$22.0)&  0.07   \\
$07399-1435$ &OH231.8+4.2& PPN & 07:42:16.738 & $-$14:42:14.04 & -878/1059,($+$16.0)&  0.06   \\ 
$07422+3054$ &AU Gem& Mira Main& 07:45:27.590 & $+$30:46:43.11 & -890/1047,($+$04.0)&  0.04   \\
$07585-1242$ &U Pup& Mira sat & 08:00:50.596 & $-$12:50:31.88 & -912/1025,($-$18.0)&  0.04   \\
$08005+2356$ &&OH/IR Late& 08:02:59.186 & $+$23:45:33.23 & -888/1049,($+$05.7)&  0.07   \\
$08357-1013$ &OH235.3+18.1& OH/IR Moderate & 08:38:08.805 & $-$10:24:16.95 & -894/1043,($+$00.0)&  0.07 \\
$09425+3444$ &R Lmi& Mira main& 09:45:34.314 & $+$34:30:42.91 & -894/1043,($+$00.0)&  0.14   \\
$09448+1139$ &R Leo& Mira main & 09:47:33.446 & $+$11:25:43.52 &-893/1044,($+$01.0)&  0.05   \\
$10580-1803$ &R Crt& SR & 11:00:33.822 & $-$18:19:29.54 & -884/1053,($+$10.0)&  0.05   \\
$12562+2324$ &T Com& Mira sat & 12:58:38.600 & $+$23:08:23.03 & -879/1058,($+$15.0)&  0.07   \\
$13001+0527$ &RT Vir& SR & 13:02:37.908 & $+$05:11:08.56 & -876/1061,($+$18.0)&  0.09   \\
$14247+0454$ &RS Vir &Mira sat & 14:27:16.393 & $+$04:40:40.38 & -894/1043,($+$00.0)&  0.08   \\
$15193+3132$ &S Crb& Mira main& 15:21:24.366 & $+$31:22:02.05 & -894/1043,($+$00.0)&  0.07   \\
$15255+1944$ &WX Ser& Mira sat & 15:27:47.009 & $+$19:34:02.33 & -888/1049,($+$06.0)&  0.08   \\
$16235+1900$ &U Her&Mira main& 16:25:47.411 & $+$18:53:32.98  & -907/1030,($-$13.0)&  0.05   \\
$18006-1734$ &GLMP 704&OH/IR Late& 18:03:36.581 & $-$17:34:00.59 & -870/1067,($+$23.9)&  0.10   \\
$18071-1727$ &OH 12.8 +.9&OH/IR Late& 18:10:05.813 & $-$17:26:35.22 & -868/1069,($+$25.9)&  0.09   \\
$18081-0338$ &&OH/IR Thick& 18:10:49.074 & $-$03:38:14.46 & -889/1049,($+$05.6)&  0.08   \\
$18100-1915$ &GLMP 740&OH/IR Thick& 18:13:02.725 & $-$19:14:20.42 & -876/1061,($+$17.6)&  0.09   \\
$18107-0710$ &&OH/IR Thick& 18:13:29.720 & $-$07:09:48.92 & -876/1061,($+$17.9)&  0.08   \\
$18135-1456$ &OH 15.7 +.8&OH/IR Late& 18:16:26.004 & $-$14:55:13.43 & -895/1042,($-$01.1)&  0.09   \\
\hline
\end{tabular}
\end{center}
\end{table}

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\begin{table}[t]
 \begin{center}
 \caption{(continue) Observations of the 6GHz OH maser transitions in AGB stars}
 \small
 \oddsidemargin -2cm
\begin{minipage}{\textwidth}
\renewcommand{\thempfootnote}{\arabic{mpfootnote}}
 \begin{tabular}{|c|c|c|c|c|c|c|}
 \hline
 \bf{IRAS Source}&\bf{Other Name}&\bf{Type \footnote{UCHII: Ultra
 Compact HII region, SG: Supergiante, SR: Semi Regular, PN: Planetary
 Nebulae, PPN: Proto Planetary Nebulae.}}&\mc{\bf{Observed Coordinates}}
 &\bf{Observed}& {\bf{Sensitivity \footnote{E = Emission; the upper
 limits correspond to 3$\sigma$.} (Jy)} }\\ \bf{ }&\bf{ }&\bf{
 }&\mc{\bf{J2000.0}\footnote {B1950 coordinates processed to J2000
 within GILDAS package.}}&\bf{Velocity}&\bf{ (at 3$\sigma$) } \\
 \bf{ }&\bf{ }&\bf{ }&\bf{R.A.}&\bf{Dec.}&\bf{Range, LSR}&\bf{6GHz}\\
 \bf{ }&\bf{ }&\bf{ }&\bf{h m s}&\bf{${ }^0$ '
 ''}&\bf{(km.s$^{-1}$)}&\bf{LCP}\\
 \hline
 \rm
$18152-0919$ &OH 20.8 +3.1&OH/IR Thick& 18:17:58.662 & $-$09:18:42.44  & -867/1070,($+$26.7)&  0.08   \\
$18198-1249$ &OH 18.3 +.4&OH/IR Late& 18:22:43.046 & $-$12:47:40.94 & -846/1091,($+$48.0)&  0.10   \\
$18262-0735$ &&OH/IR Thick& 18:28:59.446 & $-$07:33:25.44 & -815/1122,($+$78.9)&  0.08   \\
$18268-1117$ &OH 20.4 -.3&OH/IR Thick& 18:29:35.755 & $-$11:15:53.97 & -852/1085,($+$41.8)&  0.08   \\
$18266-1239$ &V435 Sct&OH/IR Thick& 18:29:28.605 & $-$12:37:40.55 & -844/1093,($+$50.0)&  0.08   \\
$18348-0526$ &V437 Sct&OH/IR Thick& 18:37:31.986 & $-$05:23:59.35 & -867/1070,($+$27.2)&  0.06   \\
$18432-0149$ &V1360 Aql&OH/IR Thick& 18:45:52.691 & $-$01:46:43.27 & -828/1109,($+$66.2)&  0.08   \\
$18460-0254$ &V1362 Aql&OH/IR Late& 18:48:40.999 & $-$02:50:22.29 & -795/1142,($+$99.0)&  0.09   \\
$18488-0107$ &V1363 Aql&OH/IR Late& 18:51:25.772 & $-$01:03:54.48 & -818/1119,($+$75.8)&  0.08   \\
$18525+0210$ &&OH/IR Thick& 18:55:04.815 & $+$02:14:41.21 & -823/1113,($+$70.2)&  0.07   \\
$18549+0208$ &OH 35.6 -.3&OH/IR Thick& 18:57:26.573 & $+$02:12:11.24 & -816/1121,($+$77.9)&  0.09   \\
$18560+0638$ &V1366 Aql&OH/IR Moderate& 18:58:30.142 & $+$06:42:55.91 & -874/1063,($+$19.7)&  0.10   \\
$19039+0809$ &R Aql& Mira sat & 19:06:22.196 & $+$08:13:48.16 & -846/1091,($+$48.0)&  0.09   \\
$19065+0832$ &OH 42.6 +.0&OH/IR Late& 19:08:58.368 & $+$08:37:47.08 & -841/1096,($+$53.1)&  0.07   \\
$19071+0946$ &OH 43.8 +.5&OH/IR Thick& 19:09:31.065 & $+$09:51:54.41 & -885/1052,($+$09.1)&  0.12   \\
$19161+2343$ &&OH/IR Moderate& 19:18:14.537 & $+$23:49:26.23 & -865/1072,($+$28.6)&  0.07   \\
$19219+0947$ &Vy\ 2-2&PN    & 19:24:22.078 & $+$09:53:55.82 & -956/981,($-$44.3)&  E/0.02   \\
$19244+1115$ &V1302 Aql&OH/IR Moderate& 19:26:47.588 & $+$11:21:14.77 & -849/1088,($+$45.0)&  0.08   \\
$19343+2926$ &M1-92& PPN & 19:36:16.768& $+$29:32:15.80& -894/1043,($+$0.00)& 0.24  \\
$19352+2030$ &&OH/IR Thick& 19:37:23.395 & $+$20:39:21.86 & -889/1048,($+$05.0)&  0.20   \\
$20043+2653$ &GLMP 972&OH/IR Thick& 20:06:22.890 & $+$27:02:11.23 & -898/1039,($-$04.6)&  0.08   \\
$20047+1248$ &SY Aql& Mira sat & 20:07:05.694 & $+$12:57:07.39 & -943/994,($-$49.0)&  0.08   \\
NML Cyg  &&SG & 20:46:25.941 & $+$40:06:56.09 & -894/1043,($+$00.0)&  0.02   \\
$20491+4236$ &OH 83.4 -.9&OH/IR Moderate& 20:50:57.766 & $+$42:48:04.31 & -932/1005,($-$38.4)&  0.05   \\
$21554+6204$ &GLMP 1048&OH/IR Thick& 21:56:58.184 & $+$62:18:43.62 & -914/1022,($-$20.6)&  0.06   \\
$22177+5936$ &NSV 25875&OH/IR Moderate& 22:19:27.806 & $+$59:51:21.74 & -919/1017,($-$25.6)&  0.07   \\
$23041+1016$ &R Peg &Mira main& 23:06:38.829  & $+$10:32:37.94 & -870/1067,($+$24.0)&  0.09   \\
$23558+5106$ &R\ Cas&Mira main& 23:58:24.683 & $+$51:23:18.18 & -870/1067,($+$24.0)&  0.06   \\
\hline
\end{tabular}
\end{minipage}

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\end{table}

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