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[2] | EARN | 1.) Michaël Marsset et al 2022 AJ 163 165 |
[3] | EARN | 1.) Thomas, C.A. et al. (2014) Icarus 228, 217-246. (Physical characterization of Warm Spitzer-observed near-Earth objects) |
[4] | EARN | 1.) A. V. Sergeyev, B. Carry et al A&A, 658 (2022) A109 |
[5] | EARN | Earth Asteroids Research Node: https://earn.dlr.de |
[6] | EARN | 1.) Cruikshank, D.P. et al. (1991) Icarus 89, 1-13. (Three basaltic earth-approaching asteroids and the source of the basaltic meteorites) 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.) 3.) Whiteley, R.J. (2001) PhD. Thesis, University of Hawaii. (A Compositional and Dynamical Survey of the Near-Earth Asteroids) 4.) 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) 5.) Thomas, C.A. et al. (2014) Icarus 228, 217-246. (Physical characterization of Warm Spitzer-observed near-Earth objects) |
[7] | EARN | 1.) Warner, B.D. (2015) MPB 42, 256-266. (NEAR-EARTH ASTEROID LIGHTCURVE ANALYSIS AT CS3-PALMER DIVIDE STATION: 2015 MARCH-JUNE)(35 NEAs) 2.) Warner, B.D. et al. (2014) MPB 41, 157-168. (NEAR-EARTH ASTEROID LIGHTCURVE ANALYSIS AT CS3-PALMER DIVIDE STATION: 2014 JANUARY-MARCH) (1943,4055,4954,25916,35107,40267,53435,68031,85990,86039,138127,143409,243566,275677,277570,294739,357622,377097,1995CR,2006DP14,2009CT,2009QF31,2011BT15,2012AU10,2013XV8,2013YZ13,2013PD21,2013XF22,2013YZ37,2013WT44,2014CR,2014EM,2014BR8,2014CG13,2014CU13,2014EY24,2014AY28,2014EL45,2014BR57,2014DX110) 3.) Petr Pravec's Ondrejov NEO Photometric Program Webpage "Prepublished Periods" 4.) Delbo, M. et al. (2003) Icarus 166, 116-130. (Keck observations of near-Earth asteroids in the thermal infrared) 5.) Sada, P.V. et al. (2016) MPB 43, 154-156. (RESULTS OF THE 2015 MEXICAN ASTEROID PHOTOMETRY CAMPAIGN)(..,4055) |
[8] | ESA Aegis | ESA orbit determination and impact monitoring system |
[9] | EARN | 1.) Petr Pravec's Ondrejov NEO Photometric Program Webpage "Prepublished Periods" |
[10] | EARN | 1.) Joseph R. Masiero et al 2021 Planet. Sci. J. 2 162 |
[11] | EARN | 1.) Nugent, C.R. et al. (2016) Astron. J. 152_63 (12pp) (NEOWISE Reactivation Mission Year Two: Asteroid Diameters and Albedos) (207 NEOs) |
[12] | EARN | 1.) Mainzer, A. et al. (2011) ApJ 743, 156. (NEOWISE Observations of Near-Earth Objects: Preliminary Results) (albedo and diameters of 428 NEOs) 2.) Delbo, M. et al. (2003) Icarus 166, 116-130. (Keck observations of near-Earth asteroids in the thermal infrared) 3.) Cruikshank, D.P. et al. (1991) Icarus 89, 1-13. (Three basaltic earth-approaching asteroids and the source of the basaltic meteorites) 4.) Mainzer, A.; Grav, T.; Masiero, J.; Hand, E.; et al. (2011) Astrophys. J. 741, A90. See also Grav 2012b and Masiero 2012. 5.) Mainzer, A.; Grav, T.; Masiero, J.; Bauer, J.; et al. (2012) Astrophys. J. Let. 760, L12. |
[13] | EARN | 1.) Mainzer, A. et al. (2011) ApJ 743, 156. (NEOWISE Observations of Near-Earth Objects: Preliminary Results) (albedo and diameters of 428 NEOs) 2.) 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) 3.) Delbo, M. et al. (2003) Icarus 166, 116-130. (Keck observations of near-Earth asteroids in the thermal infrared) 4.) Cruikshank, D.P. et al. (1991) Icarus 89, 1-13. (Three basaltic earth-approaching asteroids and the source of the basaltic meteorites) 5.) Mainzer, A.; Grav, T.; Masiero, J.; Hand, E.; et al. (2011) Astrophys. J. 741, A90. See also Grav 2012b and Masiero 2012. 6.) Mainzer, A.; Grav, T.; Masiero, J.; Bauer, J.; et al. (2012) Astrophys. J. Let. 760, L12. |
[14] | EARN | 1.) Lin, C-H. et al. (2018) P&SS 152, 116-135. (Photometric survey and taxonomic identifications of 92 near-Earth asteroids) |
[15] | EARN | 1.) Cruikshank, D.P. et al. (1991) Icarus 89, 1-13. (Three basaltic earth-approaching asteroids and the source of the basaltic meteorites) |
[16] | 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.) Binzel, R.P. et al. (2006) LPSC 37, 1491. (The MIT-Hawaii-IRTF joint campaign for NEO spectral reconnaissance.) 3.) Binzel, R.P. et al. href="http://smass.mit.edu/minus.html"> Webpage 4.) Burbine, T.H. et al. (2008) ACM2008, 8274. (DETERMINING THE PYROXENE MINERALOGIES OF NEAR-EARTH, MIDDLE-BELT, AND OUTER-BELT VESTOIDS) 5.) deLeon, J. et al. (2010) Astron. Astrophys 517, A23. (Observations, compositional, and physical characterization of near-Earth and Mars-crosser asteroids from a spectroscopic survey) 6.) Sanchez, J.A. et al. (2013) Icarus 225, 131-140. (Surface composition and taxonomic classification of a group of near-Earth and Mars-crossing asteroids) (,4055,19764,89830,138404,143381,159609,164121,241662,2007ML13) 7.) Thomas, C.A. et al. (2014) Icarus 228, 217-246. (Physical characterization of Warm Spitzer-observed near-Earth objects) 8.) Takir, D. et al. (2015) DPS47-106.05. (astract) (Are near-Earth Vestoids volatile-rich asteroids?) |