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* - orbital type derived from osculating orbital elements
# - absolute magnitude H derived from astrometric observation via orbit determination - G value assumed to be 0.15
(001) M.P.E.C. 2004-X40
(002) Busch, M.W. et al. (2012) DPS 44 302-05. (abstract) (Radar Imaging Of 11066 Sigurd, 2000 YF29, And 2004 XL14 And The Obliquity Distribution Of Contact Binary Near-Earth Asteroids)
(003) JPL's NEO Radar Detection Program Webpage
(004) Busch, M.W. et al. (2012) DPS 44 302-05. (abstract) (Radar Imaging Of 11066 Sigurd, 2000 YF29, And 2004 XL14 And The Obliquity Distribution Of Contact Binary Near-Earth Asteroids)
(005) Binzel, R.P. et al. (2006) LPSC 37, 1491. (The MIT-Hawaii-IRTF joint campaign for NEO spectral reconnaissance.)
(006) Binzel, R.P. et al. Webpage
NEODyS Page of 2004 XL14