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| [10] | EARN | 1.) Harris, A.W. (DLR) (1998) Icarus 131, 291-301. (A Thermal Model for Near-Earth Asteroids) 2.) Harris, A.W. (DLR) & J.S.V Lagerros (2002) in "Asteroids III" (Eds. W.F.Bottke et al.), Univ.Ariz.Press, Tucson, USA, pp. 205-218. (Asteroids in the thermal infrared) 3.) Lebofsky, L.A. et al. (1981) Icarus 48, 335-338. (The albedo and diameter of 1862 Apollo) 4.) Delbo, M. et al. (2011) Icarus 212, 138-148. (The cool surfaces of binary near-Earth asteroids) (5381,153591,164121) 5.) Nugent, C.R. et al. (2015) Astrophys. J. 814_117 (13pp) (NEOWISE Reactivation Mission Year One: Preliminary Asteroid Diameters and Albedos)(201 NEOs) |
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| [13] | EARN | 1.) Goldstein, R.M. (1981) Icarus 48, 59-61. (Radar observations of Apollo) 2.) Ostro, S.J. et al. (1991) Astron. J. 102, 1490-1502. (Asteroid radar astrometry) 3.) Ostro, S.J. et al. (2002) Icarus 156, 580-583. (Radar Observations of Asteroid 1862 Apollo) 4.) Ostro, S.J. et al. (2005) I.A.U. Circ. HREF="http://www.cbat.eps.harvard.edu/iauc/08600/08627.html"> 8627. (1862 Apollo) (Radar observations, binary detection) |
