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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. 2007-D15
(002) Statler, T.S. et al. (2013) Icarus 225, 141-155. (Size matters: The rotation rates of small near-Earth asteroids) (phtometry of 83 NEAs, 20 new rotation periods )
(003) Kwiatkowski, T. et al. (2010) Astron. Astrophys. 509, A94. (Photometric survey of the very small near-Earth asteroids with the SALT telescope I. Lightcurves and periods for 14 objects) (K06XY,K06YH14,K07DD,K07DX,K07HD84,K07KE,K07KE4,K07LT,K07LW19,K07RS146,K07TU18,K07VV83,K07XO3,K08DG4)
NEODyS Page of 2007 DD