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Home All issues Volume 506 / No 2 (November I 2009) A&A, 506 2 (2009) 935-954 Full HTML
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Table 5:

Results of the photometric inversion of simulated Eros-like shaped asteroids on different asteroidal orbits.
Simulated N $\lambda$(pole) $\beta$(pole) Period b/a c/a k $\epsilon$
Orbit   (deg) (deg) (h)     (mag/$^{\circ}$) (mag)
15 85 $59.8\pm0.3$ $54.0\pm0.7$ $19.150029\pm0.000024$ $0.24\pm0.02$ $0.22\pm0.01$ $0.018\pm0.001$ 0.054
24 84 $45.5\pm0.1$ $44.1\pm0.2$ $19.150292\pm0.000002$ $0.28\pm0.01$ $0.28\pm0.01$ $0.022\pm0.001$ 0.058
311 62 $50.4\pm0.2$ $53.0\pm0.1$ $19.150183\pm0.000005$ $0.41\pm0.00$ $0.41\pm0.00$ $0.026\pm0.000$ 0.091
319 64 $50.5\pm0.6$ $47.2\pm0.2$ $19.150310\pm0.000013$ $0.42\pm0.01$ $0.42\pm0.01$ $0.021\pm0.000$ 0.060
320 48 $43.4\pm0.9$ $42.7\pm1.4$ $19.150424\pm0.000021$ $0.34\pm0.03$ $0.34\pm0.03$ $0.024\pm0.001$ 0.068
326 97 $49.3\pm0.4$ $50.4\pm0.7$ $19.149266\pm0.000012$ $0.40\pm0.01$ $0.40\pm0.01$ $0.025\pm0.000$ 0.058
363 44 $45.1\pm0.4$ $54.0\pm0.3$ $19.149646\pm0.000037$ $0.41\pm0.00$ $0.41\pm0.00$ $0.021\pm0.001$ 0.073
391 81 $55.2\pm0.8$ $51.4\pm0.2$ $19.150162\pm0.000021$ $0.47\pm0.00$ $0.44\pm0.00$ $0.022\pm0.000$ 0.077
433 88 $49.0\pm0.2$ $53.4\pm0.3$ $19.149835\pm0.000006$ $0.43\pm0.00$ $0.40\pm0.00$ $0.024\pm0.000$ 0.143
472 62 $44.7\pm0.5$ $52.0\pm0.3$ $19.149876\pm0.000008$ $0.43\pm0.00$ $0.43\pm0.00$ $0.023\pm0.000$ 0.081

Note:
N is the number of simulated Gaia detections for each case. The spin parameters adopted to compute the simulated cases are: Pole $= (48.5^\circ, 51.0^\circ)$, Period = 19.150000 h.

Source LaTeX | All tables | In the text

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