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Table 2

Spitzer color-corrected fluxes at 23.68 and 71.42 μm for the “new” objects presented in this work.

Object Mid-time rh[AU] Δ [AU] Flux24[mJy] Flux70[mJy] Reference
Varuna 2004-Sep.-22 42.9294 43.2342 0.044 ± 0.035 8.217 ± 2.903 1
(55636) 2002 TX300 2004-Dec.-27 40.7280 40.9780 <0.026 <4.428 1
(120348) 2004 TY364 2007-Aug.-17 39.5979 39.6670 0.145 ± 0.008 7.727 ± 1.312 2
(15820) 1994 TB 2004-Dec.-31 28.3204 28.5620 0.067 ± 0.037 <3.08 1
Ixion 2004-Sep.-27 42.4525 42.7366 0.525 ± 0.041 18.897 ± 5.064 1
(33340) 1998 VG44 2004-Sep.-24 29.5494 29.8421 0.260 ± 0.070 15.501 ± 3.471 2
(26308) 1998 SM165 2005-Sep.-06 35.9554 36.3023 0.100 ± 0.004 5.403 ± 0.667 1
(26375) 1999 DE9 2005-May-14 34.4685 34.9803 0.895 ± 0.084 21.811 ± 3.219 1
(119979) 2002 WC19 2008-Oct.-25 42.5165 42.7381 0.090 ± 0.009 4.103 ± 0.753 2
(44594) 1999 OX3 2004-Oct.-07 24.6652 25.0840 0.630 ± 0.122 2.794 ± 3.323 2
(48639) 1995 TL8 2008-Sep.-25 43.3742 43.6947 0.017 ± 0.007 <0.785 2
Phoebe 2005-Apr.-04 9.1012 8.7643 268.4 ± 8.09 402.13 ± 25.60 2

Notes.Mid-time: mean date of the observation. Note that this “mean” value may reflect observations performed several months apart. r [AU]: heliocentric distance (AU) for the observation date. Δ [AU]: distance object-Spitzer (AU) for this date. Error bars and upper limits on fluxes are 1σ.

Reference. 1) Revised fluxes from Stansberry et al. (2008); 2) previously unpublished data.

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