| [1] | EARN | 1.) Binzel, R.P. et al. (2004) Icarus 170, 259-294. (Observed spectral properties of near-Earth objects: results for population distribution, source regions, and space weathering processes.) |
| [2] | EARN | 1.) McFadden, L.A. et al. (1989) in "Asteroids II" (Eds. R.P.Binzel et al.), Univ.Ariz.Press, Tucson, USA, pp. 442-467. (Physical properties of Aten, Apollo and Amor asteroids) 2.) Tholen, D.J. (1989) in "Asteroids II" (Eds. R.P.Binzel et al.), Univ.Ariz.Press, Tucson, USA, pp. 1139-1150. 3.) Bus, S.J. & Binzel, R.P. (2002) Icarus 158,106-145. (Phase II of the Small Main-Belt Asteroid Spectrographic Survey: A Feature-Based Taxonomy.) 4.) Binzel, R.P. et al. (2004) Icarus 170, 259-294. (Observed spectral properties of near-Earth objects: results for population distribution, source regions, and space weathering processes.) |
| [3] | EARN | 1.) Warner, B.D. (2015) MPB 42, 115-127. (NEAR-EARTH ASTEROID LIGHTCURVE ANALYSIS AT CS3-PALMER DIVIDE STATION: 2014 OCTOBER-DECEMBER)(43NEAs) 2.) href="http://echo.jpl.nasa.gov/asteroids/index.html">JPL's NEO Radar Detection Program Webpage |
| [4] | ESA Aegis | ESA orbit determination and impact monitoring system |
| [5] | EARN | 1.) Tedesco, E.F. (1989) in "Asteroids II" (Eds. R.P.Binzel et al.), Univ.Ariz.Press, Tucson, USA, pp. 1090-1138. 2.) Chapman, C.R. et al. (1994) in "Hazards due to asteroids and comets", (T.Gehrels, ed.), Univ. Arizona Press, Tucson, USA, pp. 537-549. |
| [6] | EARN | 1.) Tedesco, E.F. (1989) in "Asteroids II" (Eds. R.P.Binzel et al.), Univ.Ariz.Press, Tucson, USA, pp. 1090-1138. |
| [7] | EARN | 1.) Giorgini, J.D. et al. (2014) I.A.U. Circ. HREF="http://www.cbat.eps.harvard.edu/iauc/09200/09272.html"> 9272. (2340 Hathor) (Radar obs., detection of Yarkovsky drift) 2.) Chapman, C.R. et al. (1994) in "Hazards due to asteroids and comets", (T.Gehrels, ed.), Univ. Arizona Press, Tucson, USA, pp. 537-549. 3.) Binzel, R.P. et al. (2002) in "Asteroids III" (Eds. W.F.Bottke et al.), Univ.Ariz.Press, Tucson, USA, pp. 255-271. (Physical Properties of NEOs) |
| [8] | EARN | 1.) Thomas, C.A. et al. (2011) Astron. J. 142, 85. (ExploreNEOs. V. AVERAGE ALBEDO BY TAXONOMIC COMPLEX IN THE NEAR-EARTH ASTEROID POPULATION) (new albedos data for 118 NEOs) 2.) Binzel, R.P. et al. (2002) in "Asteroids III" (Eds. W.F.Bottke et al.), Univ.Ariz.Press, Tucson, USA, pp. 255-271. (Physical Properties of NEOs) |
| [9] | EARN | 1.) href="http://echo.jpl.nasa.gov/asteroids/index.html">JPL's NEO Radar Detection Program Webpage 2.) Giorgini, J.D. et al. (2014) I.A.U. Circ. HREF="http://www.cbat.eps.harvard.edu/iauc/09200/09272.html"> 9272. (2340 Hathor) (Radar obs., detection of Yarkovsky drift) |
| [10] | EARN | 1.) Bus, S.J. & Binzel, R.P. (2002) Icarus 158,106-145. (Phase II of the Small Main-Belt Asteroid Spectrographic Survey: A Feature-Based Taxonomy.) 2.) Binzel, R.P. et al. (2004) Icarus 170, 259-294. (Observed spectral properties of near-Earth objects: results for population distribution, source regions, and space weathering processes.) |
