We present a new method for exoplanet orbit fitting from direct observations, based on the unscented Kalman filter and a new set of orbital elements. These elements are nonsingular, and every possible set of values describes an elliptic orbit, making them well-suited to an unconstrained filter; they combine features of the Cohen-Hubbard nonsingular elements, as well as the Thiele-Innes constants. To obtain higher accuracy, we apply multiple filter passes with the same measurements, and we use a seventh-order Gaussian cubature rule to generate the sample points. We test this method using simulations of an exoplanet’s orbit and astrometric measurements.
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