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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 4:

Results of the photometric inversion of simulated Golevka-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 $41.8\pm0.2$ $54.7\pm0.3$ $19.149624\pm0.000004$ $0.66\pm0.00$ $0.64\pm0.00$ $0.027\pm0.000$ 0.044
24 (1) 84 $229.6\pm0.2$ $49.2\pm0.1$ $19.150124\pm0.000002$ $0.61\pm0.00$ $0.61\pm0.00$ $0.026\pm0.000$ 0.041
24 (2) 84 $47.9\pm0.1$ $49.3\pm0.1$ $19.150115\pm0.000001$ $0.61\pm0.00$ $0.61\pm0.00$ $0.026\pm0.000$ 0.042
311 62 $46.0\pm0.5$ $53.8\pm0.2$ $19.150163\pm0.000003$ $0.63\pm0.00$ $0.60\pm0.00$ $0.029\pm0.000$ 0.045
319 64 $45.8\pm0.2$ $49.2\pm0.1$ $19.150106\pm0.000003$ $0.64\pm0.00$ $0.64\pm0.00$ $0.026\pm0.000$ 0.040
320 48 $44.0\pm0.1$ $46.8\pm0.1$ $19.150330\pm0.000009$ $0.63\pm0.00$ $0.63\pm0.00$ $0.024\pm0.000$ 0.045
326 97 $43.5\pm0.2$ $51.6\pm0.2$ $19.149358\pm0.000006$ $0.65\pm0.00$ $0.65\pm0.00$ $0.018\pm0.000$ 0.056
363 44 $47.0\pm0.8$ $53.3\pm0.5$ $19.149573\pm0.000008$ $0.65\pm0.00$ $0.62\pm0.01$ $0.024\pm0.000$ 0.045
391 81 $62.1\pm0.2$ $51.6\pm0.1$ $19.149814\pm0.000003$ $0.64\pm0.00$ $0.64\pm0.00$ $0.021\pm0.000$ 0.044
433 88 $57.1\pm0.0$ $52.5\pm0.0$ $19.149919\pm0.000001$ $0.64\pm0.00$ $0.64\pm0.00$ $0.024\pm0.000$ 0.101
472 62 $46.2\pm0.0$ $45.7\pm0.0$ $19.150169\pm0.000002$ $0.63\pm0.00$ $0.63\pm0.00$ $0.023\pm0.000$ 0.047

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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