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Table 4

Spitzer-MIPS color corrected fluxes at 23.68 and 71.42 μm available for our SDOs/detached sample.

Object Mid-time rh[AU] Δ [AU] α[deg] Flux24[mJy] Flux70[mJy]

(15874) 1996 TL66 2008-Feb.-17 04:27:11 35.4370 34.9378 1.4 0.324  ±  0.0202 10.12  ±  1.402
(82158) 2001 FP185 2004-Jun.-20 22:51:52 34.2594 34.0927 1.7 0.395  ±  0.0963 Contaminated flux
(73480) 2002 PN34 2006-Jul.-16 11:00:56 14.6074 14.1524 3.6 10.144  ±  0.1172 30.34  ±  1.592
(127546) 2002 XU93 2006-Nov.-04 20:09:23 21.0896 20.8251 2.7 2.431  ±  0.0523 14.12  ±  1.193
(65489) Ceto 2006-Jul.-19 03:19:41 27.9924 27.6753 2.0 1.419  ±  0.0472 14.6  ±  2.61
(42355) Typhon 2008-Jun.-26 22:18:45 17.6784 17.5110 3.3 4.974  ±  0.1253 27.46  ±  3.432
(120132) 2003 FY128 2007-Jul.-14 07:30:00 38.3556 38.1281 1.5 0.427  ±  0.0513 19.38  ±  3.163
(136199) Eris 2005-Aug.-24 22:13:07 96.9049 96.4083 0.5  <0.0051 2.7  ±  0.71

Notes. Mid-time: mean date and UT time of the observation. rh [AU]: heliocentric distance (AU) for the observation date. Δ [AU]: distance object-Spitzer (AU) for this date. α [deg]: phase angle–degrees. Flux24, Flux70: Spitzer-MIPS color-corrected flux densities (mJy) at 23.68 μm and 71.42 μm. Upper limits are 1σ.

References. 

(2)

Revised data from Stansberry et al. (2008);

(3)

previously unpublished data.

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