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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.
( 1) M.P.E.C. 2003-C63
( 2) Petr Pravec's Ondrejov NEO Photometric Program Webpage
NEODyS Page of (163693) Atira