Table B.2
Values of ɛ1, ɛ2, and χ for the asteroids with χ ≥ 1.
| Ast. | A2 |  |
S/N |  |
 |
S/NJPL | JPL Model | ɛ1 | ɛ2 | χ |
|---|---|---|---|---|---|---|---|---|---|---|
| 65717 | 4.33 | 0.99 | 4.3 | 7.74 | 1.04 | 7.4 | 1 | 3.42 | 3.26 | 2.36 |
| 2003 AF23 | −4.44 | 0.32 | 13.7 | −5.48 | 0.34 | 15.6 | 1 | 3.21 | 2.96 | 2.18 |
| 2011 PU1 | −44.44 | 6.68 | 6.6 | −30.30 | 4.99 | 6.0 | 1 | 2.11 | 2.83 | 1.69 |
| 2062 | −1.40 | 0.16 | 8.3 | −1.06 | 0.11 | 9.2 | 1 | 2.04 | 3.00 | 1.69 |
| 1998 KY26 | −22.99 | 3.96 | 5.7 | −13.77 | 5.66 | 2.4 | 3 | 2.32 | 1.62 | 1.33 |
| 4179 | −0.61 | 0.06 | 8.8 | −0.77 | 0.09 | 7.9 | 2 | 2.24 | 1.60 | 1.30 |
| 2018 CW2 | −49.22 | 2.39 | 20.5 | −55.01 | 3.85 | 14.2 | 1 | 2.41 | 1.50 | 1.27 |
| 1685 | −0.44 | 0.10 | 4.3 | −0.30 | 0.04 | 6.5 | 1 | 1.39 | 3.08 | 1.27 |
| 163000 | −3.48 | 0.55 | 6.2 | −2.46 | 0.60 | 4.0 | 1 | 1.84 | 1.70 | 1.25 |
| 85990 | −3.15 | 0.21 | 14.4 | −3.56 | 0.26 | 13.4 | 1 | 1.87 | 1.54 | 1.19 |
| 2018 GY | −30.67 | 4.18 | 7.3 | −39.49 | 6.32 | 6.2 | 1 | 2.10 | 1.39 | 1.16 |
| 306383 | −2.50 | 0.44 | 5.6 | −1.71 | 0.54 | 3.1 | 1 | 1.79 | 1.47 | 1.13 |
| 2010 VK139 | −14.71 | 2.12 | 6.9 | −9.81 | 3.80 | 2.5 | 1 | 2.30 | 1.28 | 1.12 |
| 363599 | −6.37 | 0.49 | 12.8 | −5.51 | 0.60 | 9.1 | 1 | 1.72 | 1.42 | 1.09 |
| 2005 VL1 | −21.68 | 2.33 | 9.2 | −83.20 | 56.12 | 1.4 | 3 | 26.36 | 1.09 | 1.09 |
| 524522 | −5.98 | 0.10 | 56.9 | −5.82 | 1.12 | 51.8 | 1 | 1.49 | 1.40 | 1.02 |
Notes. Columns are: Ast = Designation of the asteroid; A2 = Transversal nongravitational component estimated by NEOCC; 
= Error in A2 estimated by NEOCC; S/N = Signal-to-noise ratio of the NEOCC detection; 
= Transversal nongravitational component estimated by JPL; 
= Error in A2 estimated by JPL; S/NJPL = Signal-to-noise ratio of the JPL detection; JPL Model = Dynamical model used by JPL (1 = A2; 2 = A1 and A2; 3 = A1, A2 and A3); ɛ1 = Relative error w.r.t. NEOCC; ɛ2 = Relative error w.r.t. JPL; χ = Chi value. The full list in extended precision is available at the CDS. The A2 and σ(A2) values are given in 10−14 au d−2.
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