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\begin{document}
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\begin{planotable}{lll lll}
\tablenum{10}
\tablewidth{7.0in}
\tablecaption{MILLIMETRE FLUXES}
\tablehead{
\colhead{Object} &
\colhead{$\lambda$(mm)} &
\colhead{S(mJy)} &
\colhead{Date} &
\colhead{Telescope} &
\colhead{Ref} \\
}
\startdata
Q0003+199 & 1.3 & $<$852 & 1983 & NRAO & 5\\%
Q0007+106 & 3.3 & 1600$\pm$100 & 1979 & NRAO & 8\\
          & 3.3 & 2600$\pm$400 & 1978 & NRAO & 8\\
          & 1.0 & 800$\pm$200 & 1979 & Hale & 7\\%
Q0026+129 & 1.0 & $<$1600 & 1982 & UKIRT & 11\\
          & 1.0 & $<$1000 & 1979 & Hale & 7\\%
          & 3.3 & 190$\pm$40 & 1980 & NRAO & 10\\
Q0050+124 & 1.3 & $<$672 & 1983 & NRAO & 5\\%
          & 1.3 & $<$222 & 1986 & NRAO & 2\\%
          & 3.3 & $<$141 & 1986 & NRAO & 2\\%
          & 0.15& 1900$\pm0.8$ & 1987 & KAO & 6\\%
Q0054+144 & 3.3 & $<$360 & 1980 & NRAO & 10\\
          &1.3 & $<$3.0 & 1988 & IRAM& 3\\%
Q0134+329 & 1.0 & $<$700 & 1979 & Hale & 7\\%
          & 3.3 & 300 & 1986 & IRAM & 12\\
Q0205+024 & 3.3 & $<$60   & 1984 & UKIRT & 11\\
Q0837-120 & 1.3 & 55.0$\pm$6.3 & 1989 & IRAM & 1\\%
Q0844+349& 1.3 & $<$3.4 &1988 & IRAM & 3\\%
Q1028+313 & 3.3 & 140$\pm$30 &1980 & NRAO & 10\\
Q1100+772 & 1.3 & 4.2$\pm$1.8 & 1989 & IRAM & 1\\%
Q1137+660 & 3.3 & 140$\pm$90 & 1980 & NRAO & 10\\
Q1202+281 & 3.3 & $<$210 & 1980 & NRAO & 10\\
Q1211+143 & 1.3 & $<$2.8 & 1988 & IRAM & 3\\%
Q1219+755 & 3.3 & $<$90  & 1980 & NRAO & 10\\
          & 1.0 & $<$900 & 1978 & Hale & 7\\%
Q1226+023 & 3.3 & 20280$\pm1960$&1977 & VLA & 9\\
          & 3.3 & 12900$\pm$1000&1978 & NRAO & 8\\
	  & 3.3 & 14800$\pm$900 & 1979& NRAO & 8\\
          & 3.3 & 16320$\pm$1640&1980 & NRAO & 10\\
          & 3.3 & 31300$\pm$400 & 1982& NRAO&4\\%
          & 1.9 & 19000$\pm$2000&1982 &NRAO &4\\%
          & 1.1 & 11000$\pm$1000&1982 &UKIRT &4\\%
          & 1.0 & 10200$\pm$2100&1977 & Hale & 7\\%
          & 0.8 & 8700$\pm$1500 &1982 &UKIRT&4\\%
          &0.4 & 4900$\pm$900 & 1982 &UKIRT&4\\%
Q1351+695 & 1.3 & $<$1548 & 1983 & NRAO & 5\\%
Q1426+015 &1.3 & $<$4.3 & 1988 & IRAM & 3\\%
Q1613+658& 1.3 & $<$3.1 & 1988 & IRAM & 3\\%
Q1704+608 & 3.3 & $<$180 & 1980 & NRAO & 10\\
          & 1.3 & $<$6.0 & 1989 & IRAM & 1\\%OK
          & 1.0 & $<$1000&1979 & Hale & 7\\%
Q2128-123 & 3.3 & 1.3$\pm$0.1 & 1986 & IRAM &5\\%
         & 1.3 & 0.35$\pm$0.1 & 1986 & IRAM & 5\\%
Q2130+099 & 1.3 & 2.1$\pm$0.7 & 1988& IRAM & 12\\
Q2135-147 & 3.3 & 230$\pm$50  & 1980 & NRAO & 10\\
          & 1.0 & $<$800 & 1979 & Hale & 7\\%
\tablerefs{
1) Antonucci,Barvainis and Alloin (1990); 
2) Barvainis and Antonucci (1989);
3) Chini, Kreysa and Biermann (1989); 
4) Clegg, et al (1983);
5) Edelson, Malkan and Rieke (1987);
6) Engargiola et al, (1988); 
7) Ennis, Neguebauer and Werner (1982);  
8) Landau, Epstein and Rather (1980);
9) Owen, etal (1978);
10) Owen and Puschell (1982);  
11) Robson, et al (1985); 
12) Steppe, et al. (1988); 
}
\end{planotable}
\end{document}

\par
\smallskip
1) Robson, et al (1985); 2) Owen, etal (1978);
3) Owen and Puschell (1982); \\ 4) Landau, Epstein and Rather (1980);
5) Ennis, Neguebauer and Werner (1982); \\ 6) Clegg, et al (1983);
7) Chini, Kreysa and Biermann (1989).



