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Table 2

Spitzer/MIPS observations.

Target PID Mid-time r Δ α MIPS 24 μm band MIPS 70 μm band
(AU) (AU) (°) Dur. (min) F24 (mJy) Dur. (min) F70 (mJy)
1995 SM55 55 2006-Feb-18 16:27 38.93 39.03 1.47 16.5 <0.045 22.4 <3.75
1996 TO66 55 2004-Dec-26 10:22 46.40 46.22 1.23 44.8 <4.66
2002 TX300 3283 2004-Dec-28 02:04 40.98 40.73 1.37 5.3 <0.025 5.6 <5.59
2003 OP32 30081 2006-Dec-07 00:49 41.19 41.15 1.41 57.5 <0.015 33.6 <4.80

1999 KR16 55 2006-Feb-18 05:51 36.73 36.65 1.56 44.8 <2.24

Notes. PID is the Spitzer programme identifier. Observing geometry (heliocentric distance r, Spitzer-target distance Δ, and Sun-target-Spitzer phase angle α) is averaged over the individual observations. The “Dur.” column gives the total observing time (2002 TX300 and 2003 OP32 had more than one visit). Targets above the horizontal line are confirmed Haumea family members and 1999 KR16 is a probable dynamical interloper.

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