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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 3:

Results of the photometric inversion of simulated Eunomia-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 $57.8\pm0.4$ $72.9\pm0.1$ $19.150448\pm0.000015$ $0.81\pm0.01$ $0.60\pm0.00$ $0.022\pm0.000$ 0.045
24 (1) 84 $45.8\pm0.1$ $49.2\pm0.1$ $19.150410\pm0.000001$ $0.66\pm0.00$ $0.59\pm0.00$ $0.023\pm0.000$ 0.033
24 (2) 84 $227.8\pm0.1$ $49.1\pm0.1$ $19.150411\pm0.000002$ $0.66\pm0.01$ $0.59\pm0.00$ $0.023\pm0.000$ 0.033
311 62 $59.5\pm0.3$ $55.6\pm0.3$ $19.150247\pm0.000008$ $0.70\pm0.00$ $0.65\pm0.00$ $0.024\pm0.000$ 0.038
319 64 $46.1\pm0.3$ $50.4\pm0.1$ $19.150375\pm0.000009$ $0.68\pm0.00$ $0.64\pm0.00$ $0.021\pm0.000$ 0.033
320 48 $45.6\pm0.2$ $43.0\pm0.1$ $19.150362\pm0.000009$ $0.67\pm0.00$ $0.63\pm0.00$ $0.024\pm0.000$ 0.042
326 97 $47.2\pm0.2$ $49.1\pm0.1$ $19.149561\pm0.000009$ $0.69\pm0.00$ $0.66\pm0.00$ $0.019\pm0.000$ 0.040
363 (1) 44 $248.1\pm0.1$ $47.9\pm0.3$ $19.149723\pm0.000011$ $0.67\pm0.00$ $0.67\pm0.00$ $0.020\pm0.000$ 0.040
363 (2) 44 $55.8\pm0.4$ $51.5\pm0.1$ $19.149674\pm0.000013$ $0.67\pm0.00$ $0.64\pm0.01$ $0.022\pm0.010$ 0.041
391 81 $58.5\pm0.3$ $51.5\pm0.2$ $19.149986\pm0.000006$ $0.71\pm0.00$ $0.65\pm0.00$ $0.021\pm0.000$ 0.057
433 88 $59.3\pm0.4$ $63.7\pm0.2$ $19.149860\pm0.000003$ $0.73\pm0.00$ $0.60\pm0.00$ $0.024\pm0.000$ 0.084
472 62 $46.4\pm0.2$ $48.7\pm0.2$ $19.150094\pm0.000007$ $0.70\pm0.00$ $0.66\pm0.00$ $0.024\pm0.000$ 0.042

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

Source LaTeX | All tables | In the text

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