Table 3
Main data on new pair candidates.
| Properties of asteroid candidates | ||||||||
|---|---|---|---|---|---|---|---|---|
| No. | Asteroid name | Color index a* | Absolute magnitude H | Diameter ratio | dmean (m s−1) | est.age (kyr) | P1∕2 | P2∕Np |
| 1 | 2004 RF90 | 0.16 ± 0.07 | 17.1 | 1:2.2 | 13.5 |  |
1 | 0.068 |
| – | 2003 UT336 | 0.19 ± 0.13 | 18.8 | – | ||||
| 2 | 2000 HS9 | 0.10 ± 0.04 | 16.0 | 1:4.3 | 22.6 |  |
0.663 | 0.0003 |
| – | 2015 DF67 | −0.09 ± 0.25 | 19.2 | |||||
| 3 | 2003 RV20 | – | 17.7 | 1:1.5 | 9.39 |  |
0.012 | 0.047 |
| – | 2010 TH35 | – | 18.6 | |||||
| 4 | 1999 WM4 | – | 15.6 | 1:3.5 | 9.93 |  |
0.081 | 0.578 |
| – | 2017 QD23 | – | 18.3 | |||||
| 5 | 2002 CR55 | – | 15.9 | 1:3.6 | 6.94 |  |
0.423 | 0.002 |
| – | 2015 VP32 | – | 18.7 | |||||
| 6 | 2015 XO12 | −0.03 ± 0.05 | 17.8 | 1:1.3 | 1.86 |  |
1 | 8e-05 |
| – | 2001 WY4 | – | 18.4 | |||||
| 7 | 2006 BJ193 | 0.06 ± 1.08 | 17.5 | 1:2.1 | 23.5 |  |
0.154 | 0.071 |
| – | 2017 FE106 | – | 19.3 | |||||
| 8 | 1981 VL | – | 14.4 | 1:5 | 22.2 |  |
0.395 | 0.123 |
| – | 2013 CX44 | – | 17.9 | |||||
| 9 | 1999 XF200 | – | 14.7 | 1:1.8 | 14.9 |  |
0.345 | 0.083 |
| – | 2008 EL40 | 0.20 ± 0.04 | 16.3 | |||||
| 10 | 2000 XH16 | 0.14 ± 0.03 | 15.0 | 1:2 | 14.6 |  |
0.393 | 0.028 |
| – | 2002 TM148 | – | 16.7 | |||||
Notes. For the formation age estimates the uncertainties are calculated as 5th and 95th percentiles of the formation age distribution. Acceptable values for P1∕2 are considered to be 0.01 and larger for pairs with d < 10 m s−1, and 0.05 for pairs with greater d. For the ratio P2 ∕Np some contamination by coincidental pairs is expected with P2∕Np = 0.1 and higher.
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