Table 1: Distant minor planets observed at 250 GHz.
KBO alias epoch time [h] S [mJy] Observing dates
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
NOTE - Columns give the object name, provisional designation, epoch of scaled flux densities,
integration time, and flux density. Upper limits are $3\sigma$.


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