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Table A.5

Detections including both the Yarkovsky effect and SRP, which is the set of asteroids for which the parameter A1 was reliably determined with a .

Asteroid A2 A1 D
(10−15 au d−2) (10−15 au d−2) (m2 ton−1) (m)
2009 BD −1152 ± 82 14.0 0.2 57663 ± 8674 6.7 0.3 4
2012 LA −4907 ± 12832 0.4 2.2 81216 ± 16312 5.0 0.4 10*
2011 MD −2006 ± 3049 0.7 0.5 75074 ± 24396 3.1 0.3 6
2015 TC25 −4433 ± 2754 1.6 1.4 160079 ± 20065 8.0 0.7 3*

2006 RH120 −50469 ± 3787 13.3 9.0 124099 ± 4747 26.1 0.6 4*

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