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Table A.2

Proper frequencies of longitude of node and perihelion (and their formal uncertainties) of the Adelaide family members.

Asteroid g δg s δs
[′′ yr−1] [′′ yr−1] [′′ yr−1] [′′ yr−1]
525 Adelaide 32.912 0.019 −36.938 0.017
422 494 2014 SV342 32.910 0.016 −36.934 0.017
452 322 2000 GG121 32.945 0.017 −36.986 0.017
463 394 2013 GV28 32.905 0.018 −36.932 0.016
475 474 2006 SZ152 32.912 0.019 −36.926 0.017
486 081 2012 UX41 32.919 0.019 −36.935 0.018
504 375 2007 VV73 32.915 0.013 −36.941 0.017
517 580 2014 UZ170 32.925 0.018 −36.952 0.017
534 611 2014 UC204 32.926 0.023 −36.945 0.023
545 614 2011 SA45 32.914 0.012 −36.935 0.019
2004 HU76 32.917 0.014 −36.936 0.018
2004 HJ85 32.903 0.014 −36.945 0.017
2005 UF193 32.911 0.013 −36.953 0.016
2005 UK370 32.919 0.014 −36.969 0.017
2005 VP83 32.918 0.017 −36.953 0.019
2006 SK449 32.937 0.019 −36.966 0.017
2007 VT345 32.910 0.018 −36.940 0.016
2008 ET179 32.926 0.015 −36.965 0.016
2008 US17 32.919 0.017 −36.965 0.018
2008 UR182 32.912 0.014 −36.946 0.018
2009 WJ157 32.932 0.019 −36.947 0.017
2010 UF125 32.921 0.017 −36.960 0.018
2010 VC228 32.918 0.013 −36.977 0.016
2010 VF260 32.911 0.010 −36.982 0.019
2010 XB115 32.930 0.016 −36.958 0.015
2012 TM342 32.906 0.018 −36.936 0.016
2014 AD31 32.911 0.018 −36.942 0.016
2014 EM164 32.906 0.018 −36.935 0.016
2014 JA2 32.919 0.014 −36.964 0.016
2014 JY105 32.941 0.019 −36.962 0.017
2014 WM167 32.929 0.016 −36.959 0.015
2015 BE285 32.913 0.019 −36.928 0.017
2015 HU72 32.918 0.022 −36.924 0.022
2015 RM186 32.945 0.019 −36.983 0.018
2015 TD44 32.892 0.018 −36.918 0.016
2015 UR18 32.906 0.015 −36.947 0.017
2015 XZ90 32.905 0.018 −36.931 0.016
2016 AL322 32.909 0.019 −36.934 0.016
2016 CX104 32.891 0.018 −36.919 0.016
2016 FA34 32.911 0.019 −36.936 0.017
2016 GO11 32.895 0.018 −36.924 0.016
2016 QE71 32.919 0.024 −36.927 0.024
2017 AU38 32.920 0.013 −36.963 0.016
2017 HL72 32.945 0.019 −36.971 0.018
2017 TG26 32.906 0.018 −36.939 0.016
2017 UF65 32.904 0.018 −36.933 0.016
2017 WP50 32.901 0.018 −36.931 0.016
2016 UO110 32.910 0.018 −36.917 0.019
2017 RS100 32.894 0.018 −36.926 0.016
2019 TC62 32.944 0.018 −36.979 0.018
2019 YE29 32.936 0.019 −36.965 0.017

Notes. The third and fourth columns give the proper perihelion frequency g and its formal uncertainty; the fifth and sixth columns give the proper nodal frequency s and its formal uncertainty. The asteroids whose data are listed in roman font are multi-opposition, while the last four (in italics) are single-opposition.

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