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* - orbital type derived from osculating orbital elements
$ - diameter range derived from H and assumed albedo for C and S type - 0.04 and 0.20 respectively
# - absolute magnitude H derived from astrometric observation via orbit determination - G value assumed to be 0.15
! - quality code according to Lagerkvist et al. (1989) in "Asteroids II" (Eds. R.P.Binzel et al.), Univ.Ariz.Press, Tucson, USA, pp. 1162-1179.
(001) M.P.E.C. 2000-U29
(002) Whiteley, R.J. et al. (2002) Proceedings of ACM2002, ESA-SP500, pp. 473-480. (Monolithic fast-rotating asteroids) (H-values and rotation properties of 36 NEAs)
(003) Hergenrother, C.W. & R.J. Whiteley (2011) Icarus 214, 194-209. (A survey of small fast rotating asteroids among the near-Earth asteroid population) (new data for 53 NEAs)
(004) Whiteley, R.J. et al. (2002) Proceedings of ACM2002, ESA-SP500, pp. 473-480. (Monolithic fast-rotating asteroids) (H-values and rotation properties of 36 NEAs)
(005) Hergenrother, C.W. & R.J. Whiteley (2002) In preparation. (A Survey of Small Monolithic Fast-Rotating Asteroids) = published in 0B20!!
(006) Nolan, M.C. et al. (2001) LPSC 32, 2055. (Radar observations of near-Earth asteroids 2000 UG11 and 2000 UK11)
(007) JPL's NEO Radar Detection Program Webpage
(008) Nolan, M.C. et al. (2001) LPSC 32, 2055. (Radar observations of near-Earth asteroids 2000 UG11 and 2000 UK11)
NEODyS Page of 2000 UK11