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Table A.1

Yarkovsky detections with and with .

Asteroid H A2 da∕dt pv D Tax.
(10−15 au d−2) (10−4 au My−1) (km) class
(101955) Bennu 20.6 −46.20 ± 0.24 194.27 −18.98 ± 0.10 1.0 0.046 0.492 B
(480883) 2001 YE4 20.9 −69.87 ± 0.61 113.66 −50.95 ± 0.45 0.7 0.154d 0.229*
(2340) Hathor 20.2 −29.94 ± 1.18 25.32 −17.34 ± 0.69 0.6 0.6 0.21 S
(483656) 2005 ES70 23.7 −140.17 ± 5.59 25.08 −80.11 ± 3.19 0.4 0.154d 0.061*
(152563) 1992 BF 19.7 −24.85 ± 1.17 21.17 −11.96 ± 0.56 0.3 0.287 0.272 Xc
2012 BB124 21.1 71.14 ± 4.05 17.58 29.42 ± 1.67 0.6 0.154d 0.201*
(85990) 1999 JV6 20.2 −30.62 ± 2.19 13.98 −14.34 ± 1.03 0.6 0.095 0.451 Xk
(437844) 1999 MN 21.2 44.56 ± 4.26 10.46 41.35 ± 3.95 0.7 0.154d 0.195* S
(480808) 1994 XL1 20.8 −45.13 ± 4.35 10.38 −32.37 ± 3.12 0.5 0.154d 0.237*
2007 TF68 22.7 −184.07 ± 17.91 10.28 −70.90 ± 6.90 0.8 0.154d 0.099*
(1566) Icarus 16.3 −3.75 ± 0.39 9.73 −4.85 ± 0.50 0.4 0.14 1.44 S
(4179) Toutatis 15.2 −5.95 ± 0.65 9.20 −2.63 ± 0.29 1.1 0.13 2.45 S
(468468) 2004 KH17 21.9 −65.83 ± 8.08 8.15 −44.11 ± 5.41 0.6 0.072 0.197 C
(138175) 2000 EE104 20.3 −106.50 ± 11.89 8.95 −49.37 ± 5.51 1.4 0.154d 0.297*
(1862) Apollo 16.1 −3.70 ± 0.42 8.76 −1.89 ± 0.22 0.4 0.26 1.4 Q
(2062) Aten 17.1 –13.18 ± 1.53 8.64 –5.89 ± 0.68 1.4 0.2 1.3 S
(162004) 1991 VE 18.1 26.97 ± 3.35 8.04 21.73 ± 2.70 1.0 0.154d 0.824*
2006 TU7 21.9 166.67 ± 21.55 7.73 98.51 ± 12.74 1.0 0.154d 0.141*
2011 PU1 25.5 −375.52 ± 49.66 7.56 −148.60 ± 19.65 0.4 0.154d 0.027*
(6489) Golevka 19.0 −12.04 ± 1.67 7.21 −5.10 ± 0.71 0.5 0.151 0.53 Q
2011 EP51 25.3 −359.14 ± 51.20 7.01 −185.09 ± 26.39 0.5 0.154d 0.029*
(33342) 1998 WT24 17.8 −27.87 ± 4.05 6.88 −16.91 ± 2.46 1.4 0.75 0.415 Xe
(3361) Orpheus 19.2 18.27 ± 2.70 6.77 7.88 ± 1.16 0.5 0.357 0.348 Q
(364136) 2006 CJ 20.1 –29.16 ± 4.52 6.46 −34.99 ± 5.42 0.4 0.154d 0.317*
(499998) 2011 PT 24.0 −234.96 ± 37.16 6.32 –91.30 ± 14.44 0.5 0.154d 0.053*
(138404) 2000 HA24 19.1 45.05 ± 7.15 6.30 19.95 ± 3.17 1.8 0.154d 0.517* S
2006 CT 22.3 − 112.43 ± 18.09 6.22 − 48.14 ± 7.74 0.6 0.154d 0.119*
(3908) Nyx 17.3 25.45 ± 4.20 6.06 9.86 ± 1.63 1.4 0.23 1 V
(363599) 2004 FG11 21.0 − 59.90 ± 10.17 5.89 − 42.39 ± 7.20 0.8 0.306 0.152 V
1999 UQ 21.7 –110.45 ± 18.77 5.88 –44.85 ± 7.62 0.7 0.154d 0.152*
2003 YL118 21.6 − 172.62 ± 29.42 5.87 − 90.31 ± 15.39 1.3 0.154d 0.165*
(154590) 2003 MA3 21.6 –77.01 ± 13.11 5.87 –37.11 ± 6.32 0.3 0.530 0.086
2005 EY169 22.1 − 137.02 ± 23.70 5.78 − 53.80 ± 9.30 0.8 0.154d 0.128*
(10302) 1989 ML 19.4 74.98 ± 13.09 5.73 28.76 ± 5.02 0.8 0.51 0.248
2000 PN8 22.1 123.75 ± 22.26 5.56 49.28 ± 8.87 0.7 0.154d 0.131*
(506590) 2005 XB1 21.9 92.68 ± 17.54 5.28 44.88 ± 8.49 0.6 0.154d 0.143*
(350462) 1998 KG3 22.1 –61.35 ± 11.79 5.21 –24.52 ± 4.71 0.3 0.154d 0.129*
(216523) 2001 HY7 20.5 58.55 ± 11.23 5.21 31.33 ± 6.01 0.7 0.154d 0.267*
(363505) 2003 UC20 18.3 − 7.48 ± 1.44 5.20 −4.05 ± 0.78 0.7 0.028 1.9 C
(99907) 1989 VA 17.9 16.51 ± 3.19 5.18 12.71 ± 2.46 0.7 0.24 0.55 S
(66400) 1999 LT7 19.3 –43.09 ± 8.33 5.18 − 29.44 ± 5.69 0.8 0.182 0.411
(377097) 2002 WQ4 19.5 − 23.66 ± 4.61 5.13 − 10.37 ± 2.02 0.4 0.154d 0.423*
2000 CK59 24.2 − 192.46 ± 37.77 5.10 − 74.48 ± 14.62 0.4 0.154d 0.05*

Notes. The table is sorted by , in decreasing order. The columns contain the asteroid name, absolute magnitude H, A2 parameter with its uncertainty and , semimajor axis drift d a∕dt with its uncertainty, indicator parameter , geometric albedo pv, diameter D, and taxonomic class. Asteroids with no available information about the diamater are denoted with an asterisk (*). Asteroids with albedo assigned according to Binzel et al. (2002) since no direct estimate is available are indicated with a “d”. Asteroids with no albedo information are denoted with a dagger (†). A remarkable detection is that of asteroid (480883) 2001 YE4. This detection was not in the list of valid detections provided in Chesley et al. (2016), whereas in the present work it has a very high value. The substantial difference lies in the radar observations of December 2016, confirming that radar is a very powerful tool in getting specifically high S/N Yarkovsky detections.

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