Table B.3
Asteroids with measured Yarkovsky effect for the JPL SBDB, not identified or rejected by our procedure.
Ast. | da/dt | σ(da/dt) | S/N | YM | da/dtJPL | σ(da/dtJPL) | S/NJPL | JPL Model |
---|---|---|---|---|---|---|---|---|
523599 | 829.24 | 19.95 | 41.5 | 21.83 | 1292.37 | 22.09 | 58.4 | 1 |
66391 | −3.12 | 2.25 | 1.384 | 13.53 | −5.47 | 0.29 | 18.7 | 1 |
2006 CT | −38.88 | 2.08 | 18.67 | 94.22 | −38.51 | 2.09 | 18.39 | 1 |
65803 | 16.41 | 6.39 | 2.57 | 12.46 | −4.04 | 0.25 | 16.0 | 1 |
2011 CL50 | 1949.59 | 138.59 | 14.0 | 340.71 | 2023.44 | 135.40 | 14.9 | 1 |
2009 BD | −667.46 | 20.97 | 31.8 | 285.39 | −473.66 | 34.58 | 13.6 | 2 |
2004 JN1 | −164.31 | 11.51 | 14.2 | 123.80 | −159.28 | 11.80 | 13.4 | 1 |
2001 BB16 | 153.56 | 11.37 | 13.4 | 133.76 | 150.48 | 12.25 | 12.2 | 1 |
613995 | −95.23 | 8.76 | 10.8 | 63.79 | −94.35 | 9.00 | 10.4 | 1 |
3200 | −6.90 | 2.48 | 2.78 | 4.19 | −12.11 | 1.44 | 8.3 | 1 |
2006 RH120 | −54628.00 | 1438.9 | 37.96 | 1406.22 | −21205.10 | 2664.47 | 7.9 | 3 |
2013 GZ7 | −24.48 | 2.82 | 8.67 | 103.88 | −23.11 | 2.97 | 7.78 | 1 |
2000 AA6 | 71.40 | 9.46 | 7.5 | 40.78 | 76.07 | 10.00 | 7.6 | 1 |
87024 | 9.41 | 5.83 | 1.61 | 27.04 | 9.33 | 1.25 | 7.4 | 1 |
2008 DB | −588.54 | 65.53 | 8.9 | 222.81 | −455.24 | 62.16 | 7.3 | 1 |
2012 UU136 | 40.45 | 6.00 | 6.73 | 60.55 | 40.58 | 6.09 | 6.65 | 1 |
2018 KC2 | 127.86 | 18.24 | 7.0 | 97.81 | 122.98 | 18.69 | 6.5 | 1 |
2009 EM1 | −118.36 | 14.56 | 8.1 | 62.99 | −122.27 | 18.62 | 6.5 | 1 |
162004 | 20.48 | 2.29 | 8.9 | 16.18 | 18.31 | 2.78 | 6.5 | 1 |
2018 HG2 | −186.27 | 18.76 | 9.9 | 152.22 | −186.85 | 29.04 | 6.4 | 1 |
2015 XC352 | −323.04 | 49.74 | 6.4 | 218.19 | −332.22 | 55.54 | 5.9 | 1 |
337248 | −24.04 | 4.13 | 5.8 | 11.33 | −23.73 | 4.64 | 5.1 | 1 |
2013 BA74 | 307.24 | 0.71 | 5.0 | 145.09 | 619.07 | 124.18 | 4.9 | 1 |
267759 | −11.43 | 2.31 | 4.94 | 19.04 | −10.99 | 2.31 | 4.74 | 1 |
491007 | −42.92 | 9.04 | 4.74 | 38.79 | −40.38 | 9.16 | 4.40 | 1 |
68950 | −2.02 | 1.04 | 1.93 | 8.97 | −2.99 | 0.68 | 4.3 | 1 |
397326 | 9.76 | 2.05 | 4.75 | 18.84 | 9.86 | 2.26 | 4.35 | 1 |
2012 TC4 | −16.48 | 16.32 | 1.01 | 1165.75 | −106.88 | 26.05 | 4.1 | 2 |
2004 FH | 50.16 | 31.56 | 1.58 | 374.62 | 85.37 | 21.15 | 4.0 | 1 |
65679 | −18.50 | 4.38 | 4.22 | 17.96 | −19.71 | 4.89 | 4.02 | 1 |
153201 | −23.52 | 4.22 | 5.5 | 15.80 | −18.59 | 4.69 | 3.9 | 1 |
5381 | −0.18 | 2.94 | 0.060 | 12.23 | 2.70 | 0.69 | 3.9 | 1 |
7482 | 1.35 | 3.96 | 0.34 | 8.15 | −2.22 | 0.61 | 3.6 | 1 |
526826 | −56.99 | 19.35 | 2.94 | 74.76 | −66.69 | 18.68 | 3.5 | 1 |
163899 | −1.42 | 2.51 | 0.56 | 4.93 | −6.94 | 2.01 | 3.4 | 1 |
5604 | −12.27 | 3.90 | 3.14 | 16.03 | −14.00 | 4.20 | 3.33 | 1 |
2003 MS2 | −22.11 | 7.50 | 2.94 | 61.85 | −27.63 | 8.36 | 3.3 | 1 |
2021 QH2 | 407.83 | 95.41 | 4.2 | 219.79 | 354.44 | 107.61 | 3.2 | 1 |
2016 GE1 | −394.54 | 112.11 | 3.5 | 123.95 | −582.52 | 177.24 | 3.2 | 1 |
25143 | −7.84 | 4.86 | 1.61 | 24.69 | −11.09 | 3.38 | 3.2 | 1 |
2014 QL390 | −45.92 | 16.27 | 2.82 | 52.65 | −51.76 | 15.99 | 3.2 | 1 |
138947 | −13.20 | 4.61 | 2.86 | 21.90 | −18.10 | 5.67 | 3.1 | 1 |
369984 | −52.58 | 26.60 | 1.97 | 23.11 | −11.65 | 3.68 | 3.1 | 1 |
22753 | −8.69 | 3.345 | 2.59 | 19.28 | −10.35 | 3.28 | 3.1 | 1 |
483423 | −51.54 | 18.22 | 2.82 | 88.76 | −58.96 | 18.97 | 3.1 | 1 |
396593 | 12.29 | 4.56 | 2.69 | 29.31 | 14.89 | 4.83 | 3.0 | 1 |
417210 | −15.02 | 5.23 | 2.87 | 54.46 | −16.46 | 5.34 | 3.0 | 1 |
22099 | 3.19 | 2.27 | 1.40 | 16.45 | 5.02 | 1.65 | 3.0 | 1 |
Notes. Columns are: Ast = Designation of the asteroid; da/dt = Semi-major axis drift computed by the NEOCC; σ(da/dt) = Uncertainty in the semi-major axis drift computed by the NEOCC; S/N = Signal-to-noise ratio of semi-major axis drift detection of NEOCC measurement; YM = 95-th percentile of the expected maximum Yarkovsky semi-major axis drift; da/dtJPL = Semi-major axis drift computed by JPL; σ(da/dtJPL) = Uncertainty in the semi-major axis drift computed by JPL; S/NJPL = Signal-to-noise ratio of semi-major axis drift detection of JPL measurement; JPL Model = Dynamical model used by JPL (1 = A2; 2 = A1 and A2; 3 = A1, A2 and A3). The full list in extended precision is available at the CDS. The values of da/dt, σ(da/dt) and YM are given in 10−4 au My−1.
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