\begin{table}%t1
\par
\caption{\label{kbotable}Distant minor planets observed at 250~GHz.                        }
%\centerline
{
\begin{tabular}{llllll}             
\hline
\hline 
KBO   &   alias   & epoch   &time [h]& $S$ [mJy] & Observing dates \\ 
\hline  
24835 & 1995 SM55 &2001 01 21.0&2.72& $<$0.83& 2000 Dec. 16, 17, 19; 2001 \\
      &           &          &    &        & Jan. 21; Feb. 11, 18, 21 \\         
19308 & 1996 TO66 &2001 01 21.0&2.56& $<$0.90& 2000 Dec. 15, 16, 19; 2001 \\
      &           &         &     &        & Jan. 20, 21; Feb. 11, 18 \\
Chaos & 1998 WH24 &2001 01 21.0&3.64& $<$0.80& 2000 Dec 15, 17; 2001 Jan. 20, \\
      &           &         &     &        & Feb. 12, 13, 16, 17, 21 \\
47171 & 1999 TC36 &2003 01 12.0&4.06& $1.11\pm0.26$& 2000 Dec. 16, 2001 Jan. 20, 21, 22; \\
      &           &         &     &        & Feb. 11, 18; Dec. 5, 9, 20, 27; \\
      &           &         &     &        & 2002 Feb. 10, 11; May 19; Dec. 7; \\
      &           &         &     &        & 2003 Jan. 11, 12, 15, 16; Mar. 3  \\
Huya  & 2000 EB173&2001 01 21.0&2.43& $<$1.04& 2000 Dec. 13; 2000 Jan. 12, 14, 21, 22 \\
Ixion & 2001 KX76 &2002 07 02.0&4.77& $<$0.92& 2001 Dec. 9; 2002 Feb. 1, 9; May 19; \\
      &           &         &     &        & Jul. 2; 2003 Jan. 12; Feb. 4, 5, 6, 7; \\
      &           &         &     &        & Mar. 4 \\
--    & 2002 TC302&2003 01 11.0&1.84& $<$1.47& 2002 Dec. 6, 7; 2003 Jan. 11, 12, 13 \\[1pt] 
\hline
\end{tabular}}
\smallskip
NOTE -- Columns give the object name, provisional designation, 
epoch of scaled flux densities, integration time,
and flux density. Upper limits are~$3\sigma$. 
\end{table}