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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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