Table 2
Observational circumstances and photometric results of this work’s data.
| Object | Dyn. class* | Telescope | UT date | r[AU] | Δ[AU] | α [°] | R | B − R | HR(α) | |
|
|
||||||||||
| (130391) | 2000 JG81 | 2:1 | Subaru | 20080702UT07:24:58 | 34.073 | 34.817 | 1.2 | 23.12 ± 0.03 | 1.42 ± 0.06 | 7.75 ± 0.06 |
| (136120) | 2003 LG7 | 3:1 | Subaru | 20080702UT09:42:53 | 32.815 | 33.659 | 1.0 | 23.54 ± 0.05 | 1.27 ± 0.09 | 8.32 ± 0.05 |
| (149560) | 2003 QZ91 | SDO | Subaru | 20080702UT13:08:33 | 25.849 | 26.509 | 1.7 | 22.48 ± 0.03 | 1.30 ± 0.05 | 8.30 ± 0.03 |
| 2006 RJ103 | Nep. Trojan | Subaru | 20080702UT14:07:50 | 30.760 | 30.534 | 1.9 | 22.27 ± 0.02 | 1.90 ± 0.04 | 7.40 ± 0.02 | |
| 2006 SQ372 | SDO | Subaru | 20080702UT11:45:34 | 23.650 | 24.287 | 1.9 | 21.55 ± 0.02 | 1.78 ± 0.03 | 7.71 ± 0.05 | |
| 2007 JK43 | SDO | Subaru | 20080702UT08:08:13 | 23.113 | 23.766 | 1.9 | 20.73 ± 0.02 | 1.40 ± 0.03 | 7.03 ± 0.02 | |
| 2007 NC7 | SDO | Subaru | 20080702UT11:30:49 | 20.090 | 20.916 | 1.7 | 21.19 ± 0.02 | 1.28 ± 0.03 | 8.07 ± 0.02 | |
| (281371) | 2008 FC76 | Cent | Subaru | 20080702UT11:13:05 | 11.119 | 11.793 | 3.8 | 19.79 ± 0.02 | 1.76 ± 0.02 | 9.18 ± 0.04 |
| 2007 RH283 | Cent | UH2.2 m | 20080929UT12:43:47 | 17.081 | 17.956 | 1.6 | 20.85 ± 0.03 | 1.20 ± 0.05 | ||
| 2007 RH283 | Cent | UH2.2 m | 20080929UT12:57:51 | 17.081 | 17.956 | 1.6 | 20.90 ± 0.03 | 1.28 ± 0.06 | ||
| mean... | 1.24 ± 0.07 | 8.44 ± 0.04 | ||||||||
| 2007 UM126 | Cent | UH2.2 m | 20080929UT08:56:52 | 10.191 | 11.177 | 0.9 | 20.43 ± 0.03 | 1.21 ± 0.05 | ||
| 2007 UM126 | Cent | UH2.2 m | 20080929UT09:06:41 | 10.191 | 11.177 | 0.9 | 20.53 ± 0.03 | 0.92 ± 0.04 | ||
| 2007 UM126 | Cent | UH2.2 m | 20080929UT09:16:17 | 10.191 | 11.177 | 0.9 | 20.38 ± 0.02 | 1.12 ± 0.04 | ||
| mean... | 1.08 ± 0.10 | 10.16 ± 0.04 | ||||||||
Notes.
Dynamical classes are: Centaur, scattered disk object (SDO), Neptune Trojan (object located in 1:1 mean motion resonance with Neptune), 2:1, and 3:1 (objects located in 2:1 or 3:1 mean motion resonance with Neptune, respectively). For details of our classification, see Appendix A.
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