Table 1
Herschel color-corrected fluxes at 70, 100 and 160 μm and H-magnitudes for the “new” objects presented in this work.
| Object | ObsID | Mid-time | rh[AU] | Δ [AU] | Flux70[mJy] | Flux100[mJy] | Flux160[mJy] | H V |
|
|
||||||||
| Varuna | 1342205140/...5190 | 10-09-27 08:16 | 43.5317 | 43.8432 | 8.3 ± 2.0 | 12.8 ± 2.0 | 9.6 ± 3.6 | 3.760 ± 0.035 |
| (55636)2002 TX300 | 1342212764/...2802 | 11-01-17 03:46 | 41.6809 | 41.7619 | 0.9 ± 0.8 | 1.4 ± 0.8 | 5.5 ± 2.2 | 3.509 ± 0.076 |
| (120348)2004 TY364 | 1342202885/...2945 | 10-08-12 09:43 | 39.4873 | 39.1725 | 12.8 ± 0.8 | 12.2 ± 1.4 | 12.4 ± 1.7 | 4.520 ± 0.070 |
| (15820)1994 TB | 1342213518/...3569 | 11-01-31 06:22 | 27.5066 | 27.6563 | <1.05 | 1.5 ± 1.5 | <1.8 | 7.934 ± 0.354 |
| Ixion | 1342227033/...7152 | 11-08-23 00:00 | 41.0852 | 40.7822 | 22.7 ± 1.2 | 25.4 ± 1.4 | 20.5 ± 3.4 | 3.828 ± 0.039 |
| (33340)1998 VG44 | 1342216446/...6559 | 11-03-21 07:52 | 29.4064 | 29.5116 | 8.0 ± 0.8 | 9.9 ± 1.2 | 1.5 ± 1.4 | 6.670 ± 0.040 |
| (26308)1998 SM165 | 1342199499/...9622 | 10-07-01 11:11 | 37.9847 | 38.3707 | 4.1 ± 1.25 | 4.8 ± 1.8 | <4.0 | 6.023 ± 0.075 |
| (26375)1999 DE9 | 1342223635/...3670 | 11-07-04 03:39 | 36.7526 | 37.0316 | 10.1 ± 1.1 | 9.4 ± 1.3 | 4.1 ± 3.5 | 5.154 ± 0.046 |
| (119979)2002 WC19 | 1342204317/...4437 | 10-09-12 05:14 | 42.2869 | 42.2487 | 5.8 ± 1.6 | 8.0 ± 1.8 | 7.6 ± 1.8 | 4.880 ± 0.070 |
| (44594)1999 OX3 | 1342220559/...0578 | 11-05-04 05:08 | 21.5007 | 21.9481 | 10.9 ± 0.7 | 6.7 ± 0.9 | 6.2 ± 1.1 | 7.718 ± 0.092 |
| (48639)1995 TL8 | 1342214043/...4165 | 11-02-11 08:21 | 44.1223 | 44.2789 | 2.1 ± 0.8 | 2.3 ± 0.8 | <2.1 | 5.290 ± 0.060 |
| Phoebe | 1342212481/ | 11-01-10 16:41 | 9.5751 | 9.4804 | 301.3 ± 9.7 | 207.3 ± 7.3 | 113.2 ± 11.2 | 6.63 ± 0.011 |
| Sycorax | 1342221837/...1875 | 11-01-29 07:00 | 20.0843 | 20.5195 | 17.0 ± 1.0 | 15.3 ± 1.8 | 5.5 ± 3.2 | 7.83 ± 0.062 |
Notes.ObsID: Herschel ObsID of the first AOR of a sequence of four AORs of two consecutive observations (first visit/follow-on observation), respectively (no follow-on for Phoebe). Mid-time: Mean date and UT time of the observation. r [AU]: heliocentric distance (AU) for the observation date. Δ [AU]: object-Herschel distance (AU) for this date. Error bars and upper limits on fluxes are 1σ. The last column gives the HV magnitude, as compiled in this work (see text for details) or from literature.
Reference. 1)Mainzer et al. (2011b); 2)Romon et al. (2001).
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