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Fig. 4.

image

Asteroid (425387) 2010 CZ61, with three transits. Comparison of Keplerian elements as a result of orbital inversion with different methods and codes. Left column, from top to bottom panels: Keplerian elements e, i, Ω, ω and M as a function of a for independent observations. Middle column: same elements, but for Java code with normal-point treatment. Right column: OpenOrb with normal-point treatment. The red cross denotes the correct position of the object.

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