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Table 3

Spitzer-MIPS colour corrected fluxes at 23.68 and 71.42 μm, and, for Chariklo, WISE colour corrected fluxes at 11.6 and 22.1 μm.

Object Obs. start F11.6 μm [mJy] F22.1 μm [mJy] F24 μm [mJy] F71 μm [mJy] rh (AU) Δ (AU) α (o)

(2060) Chiron 2005-May-16 01:16:33 54.44 ± 1.641 147.50 ± 10.701 13.462 13.238 4.2
(10199) Chariklo 2006-Feb-15 15:13:04 61.02 ± 1.861 179.41 ± 11.501 13.164 12.890 4.2
(10199) Chariklo 2010-Feb-16 19:39:59 0.61 ± 0.17 39.57 ± 5.12 13.760 13.716 4.1
(38628) Huya 2004-Jan-27 09:32:09 3.45 ± 0.111 55.03 ± 4.201 29.326 29.250 2.0
(50000) Quaoar 2006-Apr-03 23:09:45 0.22 ± 0.022,3 28.96 ± 3.672,3 43.311 43.086 1.3
(50000) Quaoar 2005-Apr-07 09:17:49 0.26 ± 0.062,3 26.99 ± 4.902,3 43.345 42.974 1.2
(55637) 2002 UX25 2005-Jan-26 18:56:15 0.44 ± 0.041,2 23.51 ± 4.431,2 42.369 42.382 1.4
(84522) 2002 TC302 2005-Jan-23 20:03:15 0.13 ± 0.032 47.741 47.654 1.2
(90482) Orcus 2007-May-30 04:35:16 0.36 ± 0.021,2 29.27 ± 2.251,2 47.779 47.539 1.2
(120347) Salacia 2006-Dec-03 14:34:48 0.55 ± 0.024 36.60 ± 3.704 43.819 43.390 1.2
(136108) Haumea 2007-July-13 11:01:22 no data 15.83 ± 1.202 51.152 50.926 1.1

Notes.For 2002 TC302, the 24 μm flux is unreliable since the object is merged with a background source.

Reference. (1) Stansberry et al. (2008); (2) Mueller et al. (2012); (3) Brucker et al. (2009); (4) Stansberry et al. (2012).

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