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Table 2:

Summary of the results.

Asteroid 		P $\Delta {P}$ A a/b D
  [h] [h] [mag]   [km]
2007 CX50 1.45 $\pm$0.3 $\geq$0.8 $\geq$1.6 0.035
2007 EO 2.4 $\pm$0.4 $\geq$1.2 $\geq$1.7 0.082
2007 GU1 4.5 $\pm$1 $\geq$0.8 $\geq$1.6 0.030
2007 HL4 1.48 $\pm$0.02a 0.55 $\geq$1.5 0.043
2007 RE2 1.0 $\pm$0.2 0.5 $\geq$1.3 0.081
2007 UC2 0.527 $\pm$0.016a 0.40 $\geq$1.2 0.075
2007 RY9 1.2 $\pm$0.2 0.60 $\geq$1.3 0.062
2007 TS24 1.0 $\pm$0.3 1.3 $\geq$2.8 0.039
2007 UG6 1.82 $\pm$0.07 0.8 $\geq$1.6 0.073
2007 XN16 1.7 $\pm$0.2 1.4 $\geq$1.9 0.023
2008 CP116 0.330 $\pm$0.003a 0.15 $\geq$1.1 0.082
Possible NPA rotation asteroid  
2007 RQ12 0.23 -- 1.9 $\geq 2.4$ 0.059

Notes. P is the synodic period of rotation, $\Delta {P}$ is its systematic uncertainty (maximal error), A is the peak-to-peak lightcurve amplitude, a/b is the elongation of the asteroid and D denotes its effective diameter computed with the geometric albedo $p_{{\rm V}}=0.2$.
(a) The quoted uncertainty is the standard deviation $\sigma$.


Source LaTeX | All tables | In the text

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