Table 2
Colour corrected fluxes and geometric conditions for the observed TNOs and Centaurs.
| Object | F 70 μm | F 100 μm | F 160 μm | F 250 μm | F 350 μm | F 500 μm | r | Δ | α | H v |
| (mJy) | (mJy) | (mJy) | (mJy) | (mJy) | (mJy) | (AU) | (AU) | (°) | ||
|
|
||||||||||
| (2060) Chiron | 70.8 ± 3.1 | 46.2 ± 2.3 | 22.8 ± 2.9 | 11.1 ± 1.9 | 1σ = 2.9 | 1σ = 3.2 | 16.282 | 16.635 | 3.3 | 5.92 ± 0.20a |
| (10199) Chariklo | 142.9 ± 5.9 | 99.1 ± 4.4 | 50.8 ± 4.3 | 26.0 ± 2.4 | 12.8 ± 1.9 | 1σ = 3.0 | 13.861 | 13.750 | 4.2 | 7.40 ± 0.25a |
| (38628) Huya | 47.6 ± 1.7 | 43.2 ± 1.9 | 25.6 ± 2.4 | 14.8 ± 1.9 | 9.0 ± 1.8 | 1σ = 3.2 | 28.665 | 28.767 | 2.0 | 5.04 ± 0.03bcd |
| (50000) Quaoar | 32.1 ± 2.4 | 41.5 ± 3.1 | 29.9 ± 2.4 | 17.3 ± 1.9 | 10.4 ± 1.8 | 7.3 ± 2.5 | 43.136 | 43.355 | 1.2 | 2.73 ± 0.06bc |
| (55637) 2002 UX25 | 25.8 ± 1.3 | 26.0 ± 1.5 | 20.2 ± 3.8 | 11.6 ± 2.8 | 1σ = 3.1 | 1σ = 3.3 | 41.609 | 41.334 | 1.4 | 3.87 ± 0.02b |
| (84522) 2002 TC302 | 9.1 ± 1.4 | 16.2 ± 1.9 | 6.0 ± 2.4 | 1σ = 3.1 | 1σ = 3.2 | 1σ = 3.4 | 46.230 | 46.503 | 1.2 | 4.17 ± 0.10ef |
| (90482) Orcus | 25.7 ± 1.3 | 34.2 ± 1.9 | 23.5 ± 2.2 | 16.4 ± 2.0 | 8.9 ± 1.8 | 1σ = 3.1 | 47.898 | 47.705 | 1.2 | 2.31 ± 0.03bg |
| (120347) Salacia | 30.0 ± 1.2 | 37.8 ± 2.0 | 28.1 ± 2.7 | 11.0 ± 1.7 | 7.3 ± 1.6 | 1σ = 2.8 | 44.213 | 44.281 | 1.3 | 4.25 ± 0.05hi |
| (136108) Haumea | 17.3 ± 3.4 | 23.5 ± 0.8 | 22.2 ± 1.4 | 16.3 ± 2.0 | 10.7 ± 1.8 | 1σ = 2.8 | 50.971 | 50.961 | 1.1 | 0.43 ± 0.01b |
Notes.r and Δ are the target heliocentric and Herschel-centric distances, respectively, and α is the phase angle, calculated at the middle time of the PACS and SPIRE observations. Fλ is the colour-corrected flux with its 1-σ uncertainty. Entries such as 1σ = 2.9 indicate that the object was not detected, with the corresponding 1-σ upper limit. For the HV magnitude values
Rabinowitz et al. 2007;
Romanishing & Tegler (2005);
Doressoundiram et al. (2005);
computed from Santos-Sanz et al. (2009) with linear coeff. = 0.122 mag/°;
computed from Sheppard (2010) with linear coeff. = 0.122 mag/°;
Perna et al. (2010);
Benecchi et al. (2009);
Perna et al. (2013).
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