Table 2
Observational circumstances of the Damocloids included.
| Object | H | G | TJ | W1 | W2 | W3 | W4 | r | Δ | θ |
|
|
||||||||||
| (330759) 2008 SO218 | 12.80 | 0.15 | –1.395 | 0 | 0 | 8 | 8 | 3.687 | 4.049 | 14.083 |
| (336756) 2010 NV1 | 10.50 | 0.15 | –2.911 | 0 | 0 | 1 | 4 | 9.468 | 8.644 | 3.775 |
| (342842) 2008 YB3 | 9.30 | 0.15 | –0.248 | 7 | 1 | 12 | 12 | 6.643 | 7.454 | 4.799 |
| 2009 QY6 | 14.80 | 0.15 | –0.848 | 0 | 2 | 10 | 10 | 3.042 | 3.591 | 14.731 |
| 2009 YS6 | 14.20 | 0.15 | –1.051 | 0 | 0 | 6 | 5 | 3.778 | 3.343 | 14.474 |
| 2010 BK118 | 10.20 | 0.15 | –2.458 | 0 | 0 | 8 | 8 | 8.225 | 9.016 | 3.908 |
| 2010 CG55 | 14.20 | 0.15 | –1.549 | 0 | 0 | 6 | 6 | 3.820 | 4.156 | 13.319 |
| 2010 CR140 | 15.50 | 0.15 | 1.428 | 1 | 0 | 12 | 2 | 4.197 | 4.044 | 13.608 |
| 2010 EJ104 | 17.10 | 0.15 | 1.561 | 0 | 0 | 11 | 9 | 2.315 | 2.001 | 25.898 |
| 2010 FH92 | 11.40 | 0.15 | 1.533 | 0 | 0 | 9 | 9 | 5.786 | 5.695 | 9.901 |
| 2010 GW64 | 14.90 | 0.15 | –0.537 | 0 | 0 | 9 | 6 | 3.703 | 4.077 | 13.729 |
| 2010 JH124 | 14.60 | 0.15 | 1.258 | 0 | 0 | 8 | 0 | 4.127 | 3.923 | 14.126 |
| 2010 JC147 | 14.70 | 0.15 | 1.968 | 0 | 0 | 8 | 6 | 3.452 | 3.205 | 16.954 |
| 2010 OR1 | 16.20 | 0.15 | –1.216 | 0 | 6 | 8 | 8 | 2.050 | 1.222 | 21.433 |
| 2010 OA101 | 18.60 | 0.15 | 1.291 | 0 | 6 | 10 | 8 | 1.504 | 1.109 | 42.496 |
| 2010 OM101 | 17.00 | 0.15 | –0.652 | 0 | 0 | 9 | 5 | 2.244 | 1.821 | 26.398 |
Notes. We include each object’s absolute magnitude H, assumed slope parameter G, and Tisserand’s parameter TJ. Columns “Wn” (n = 1 to 4) list the number of useful images in that particular WISE band. Final columns show the heliocentric distance r in AU, distance of the asteroid to WISE spacecraft Δ in AU, and phase angle θ in degrees at the midpoint time of the observation.
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