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Table 2:

Summary of the results.
Asteroid P $\sigma_{P}$ A a/b D
  [h] [h] [mag]   [km]
2006 XY 0.0829783 $\pm$0.0000003 0.8 1.4 0.047
(2nd solution) 0.0831226 $\pm$0.0000004      
2006 YH14 0.4251 $\pm$0.0045 1.1 1.7 0.068
2007 DD 0.07429 $\pm$0.00007 0.8 1.7 0.021
2007 DX 0.212400 $\pm$0.000007 1.0 2.0 0.082
2007 HD84 0.2754 $\pm$0.0007 0.7 1.6 0.057
(2nd solution) 0.1381 $\pm$0.0004      
2007 KE 0.731 $\pm$0.003 0.9 1.6 0.094
2007 KE4 0.021408 $\pm$0.000007 0.4 1.3 0.027
2007 LT 0.044583 $\pm$0.000022 0.5 1.3 0.094
2007 LW19 0.10169 $\pm$0.00014 0.6 1.2 0.059
2007 RS146 0.03209 $\pm$0.00004 0.4 1.3 0.065
(2nd solution) 0.0642 $\pm$0.0001      
2007 TU18 0.271 $\pm$0.001 0.5 1.5 0.033
2007 VV83 0.15392 $\pm$0.00045 0.9 1.4 0.033
2007 XO3 0.2530 $\pm$0.0015 0.6 1.4 0.082
2008 DG4 0.2179 $\pm$0.0005 0.3 1.2 0.052

P is the synodic period, A is the lightcurve amplitude, a/b is the minimum elongation and D is the effective diameter.


Source LaTeX | All tables | In the text

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