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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 6:

Results of the photometric inversion of simulated Golevka-like shaped asteroids on two different asteroidal orbits.
Simulated $\sigma $ $\lambda$(pole) $\beta$(pole) Period b/a c/a k $\epsilon$
Orbit   (deg) (deg) (h)     (mag/$^{\circ}$) (mag)
319 0.01 $45.8\pm0.2$ $49.4\pm0.1$ $19.150083\pm0.000003$ $0.63\pm0.00$ $0.63\pm0.00$ $0.026\pm0.00$ 0.039
319 0.02 $48.5\pm0.3$ $50.7\pm0.0$ $19.150092\pm0.000005$ $0.64\pm0.00$ $0.64\pm0.00$ $0.025\pm0.00$ 0.041
319 0.03 $45.5\pm0.3$ $50.5\pm0.3$ $19.150048\pm0.000007$ $0.63\pm0.00$ $0.63\pm0.00$ $0.025\pm0.00$ 0.041
319 (1) 0.04 $190.1\pm0.6$ $59.2\pm0.7$ $19.150129\pm0.000008$ $0.65\pm0.00$ $0.62\pm0.00$ $0.026\pm0.00$ 0.054
319 (2) 0.04 $45.5\pm0.5$ $48.8\pm0.1$ $19.150096\pm0.000006$ $0.63\pm0.00$ $0.63\pm0.00$ $0.025\pm0.00$ 0.055
319 (1) 0.05 $195.9\pm1.0$ $54.7\pm0.6$ $19.150815\pm0.000010$ $0.63\pm0.00$ $0.63\pm0.01$ $0.025\pm0.00$ 0.076
319 (2) 0.05 $46.9\pm0.0$ $46.3\pm0.0$ $19.150810\pm0.000000$ $0.63\pm0.00$ $0.63\pm0.00$ $0.024\pm0.00$ 0.077
363 0.01 $46.9\pm0.6$ $51.9\pm0.2$ $19.149544\pm0.000006$ $0.65\pm0.00$ $0.63\pm0.00$ $0.024\pm0.00$ 0.046
363 0.02 $45.0\pm0.8$ $54.4\pm0.3$ $19.149647\pm0.000007$ $0.66\pm0.00$ $0.63\pm0.00$ $0.024\pm0.00$ 0.047
363 0.03 $42.2\pm4.6$ $54.6\pm2.5$ $19.149698\pm0.000050$ $0.66\pm0.00$ $0.62\pm0.03$ $0.026\pm0.00$ 0.051
363 0.04 $42.4\pm3.1$ $65.1\pm2.5$ $19.149276\pm0.000040$ $0.68\pm0.01$ $0.50\pm0.04$ $0.022\pm0.00$ 0.055
363 0.05 $48.0\pm0.4$ $48.3\pm0.1$ $19.149446\pm0.000005$ $0.65\pm0.00$ $0.65\pm0.00$ $0.026\pm0.00$ 0.054

Note:
Simulated photometric errors were superimposed on each simulated observation. The errors are Gaussian, with different $\sigma $. 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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