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Table 1

Observational circumstances of the ACOs in JFC orbits.

Object H G TJ W1 W2 W3 W4 r Δ θ
(944) Hidalgo 10.77 0.15 2.067 0 0 5 5 9.067 9.014 6.262
(5164) Mullo 13.00 0.15 2.787 0 0 5 4 5.347 5.248 10.904
(6144) Kondojiro 11.50 0.15 2.867 0 0 10 10 6.489 6.354 8.705
(20898) Fountainhills 11.10 0.15 2.349 11 11 0 15 2.270 1.974 26.234
(30512) 2001 HO8 12.50 0.15 2.819 0 0 10 10 4.484 4.357 13.021
(32511) 2001 NX17 12.80 0.15 2.791 0 0 10 10 5.324 5.144 10.878
(52007) 2002 EQ47 13.30 0.15 2.923 0 0 11 10 4.354 4.155 13.342
(70032) 1999 CZ13 13.20 0.15 3.011 1 0 18 15 4.757 4.650 12.335
(90572) 2004 GN17 13.80 0.15 2.991 0 0 11 11 3.869 3.635 15.075
(96177) 1984 BC 16.00 0.15 2.780 23 13 24 23 1.644 1.219 37.721
(119039) 2001 FZ91 13.30 0.15 2.933 0 0 4 4 3.548 3.296 16.461
(145627) 2006 RY102 11.00 0.15 2.830 2 0 13 13 4.943 4.750 11.647
(228862) 2003 GX31 14.30 0.15 2.937 0 0 6 3 4.736 4.546 11.978
(237838) 2002 EV71 14.80 0.15 2.906 0 0 14 12 2.938 2.691 19.807
(248590) 2006 CS 16.60 0.15 2.441 0 0 4 1 2.974 2.811 19.963
(249047) 2007 TC91 14.10 0.15 2.944 0 0 9 5 4.249 4.040 13.590
(275618) 2000 AU242 13.90 0.15 2.736 0 0 11 10 3.293 3.046 17.493
(301964) 2000 EJ37 13.50 0.15 2.441 0 1 9 10 3.204 2.957 18.383
(306173) 2010 NK83 13.70 0.15 2.569 0 0 11 11 3.795 3.674 15.532
(306461) 1999 LY5 14.80 0.15 2.887 0 0 14 13 2.889 2.719 20.415
2003 BM1 18.30 0.15 2.840 0 0 14 0 1.877 1.502 32.355
2003 BU35 16.40 0.15 2.773 8 18 33 26 1.759 1.370 34.050
2004 EB 17.20 0.15 2.755 0 0 13 3 2.132 1.885 28.505
2005 EZ92 17.30 0.15 3.021 0 13 19 15 1.506 1.061 40.709
2005 NA56 16.90 0.15 2.983 0 0 15 0 1.565 1.214 39.692
2008 SK220 15.30 0.15 3.005 0 0 6 2 3.457 3.233 16.746
2008 UD253 14.30 0.15 2.721 0 0 9 5 4.068 3.848 14.213
2009 DK12 18.30 0.15 2.352 0 0 7 3 2.994 2.816 19.838
2009 SR143 16.40 0.15 2.806 0 0 4 0 2.814 2.586 20.436
2009 UA17 15.90 0.15 2.801 0 0 21 18 2.485 2.206 23.258
2009 WF104 17.20 0.15 2.799 0 9 13 11 1.807 1.434 32.928
2009 WO6 17.30 0.15 2.784 17 11 18 18 1.363 0.876 45.908
2009 XY21 15.60 0.15 2.815 0 0 11 0 3.215 2.963 18.083
2010 AN39 15.50 0.15 2.861 0 0 9 6 3.127 2.887 18.563
2010 AZ60 15.70 0.15 2.737 0 0 13 11 2.869 2.605 20.335
2010 BD15 15.70 0.15 2.752 0 0 8 6 3.020 2.785 18.965
2010 CU139 17.30 0.15 2.818 0 0 14 4 2.377 2.057 25.171
2010 HQ 15.70 0.15 2.750 0 0 2 1 4.706 4.590 12.311
2010 KG43 14.50 0.15 2.697 0 0 7 1 2.934 2.752 20.170
2010 LR68 18.30 0.15 2.923 0 0 18 3 1.943 1.641 31.491
2010 LV121 14.80 0.15 2.694 0 0 16 16 2.974 2.789 19.955
2010 MK43 15.60 0.15 2.888 0 0 15 14 2.361 2.137 25.493
2010 CC132 15.90 0.15 2.851 0 17 21 19 1.894 1.609 31.425
2010 DD2 17.30 0.15 2.930 0 0 4 0 1.674 1.254 36.883
2010 DD58 16.30 0.15 2.619 0 2 11 8 2.033 1.709 29.063
2010 FJ81 20.80 0.15 2.340 0 13 46 2 1.240 0.703 55.814
2010 LB71 16.20 0.15 2.809 0 0 9 0 2.984 2.791 19.883
2010 MB52 17.90 0.15 2.805 0 1 8 2 1.876 1.583 32.806
2010 OE101 17.80 0.15 2.868 50 13 65 64 1.377 0.940 47.479

Notes. We also 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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