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      Frequentist confidence intervals for orbits

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          Abstract

          The problem of efficiently computing the orbital elements of a visual binary while still deriving confidence intervals with frequentist properties is treated. When formulated in terms of the Thiele-Innes elements, the known distribution of probability in Thiele-Innes space allows efficient grid-search plus Monte-Carlo-sampling schemes to be constructed for both the minimum-\(\!\chi^{2}\) and Bayesian approaches to parameter estimation. Numerical experiments with \(10^{4}\) independent realizations of an observed orbit confirm that the \(1-\) and \(2\sigma\) confidence and credibility intervals have coverage fractions close to their frequentist values. \keywords{binaries: visual - stars: fundamental parameters - methods:statistical}

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          Journal
          10.1051/0004-6361/201423661
          1402.4330

          Solar & Stellar astrophysics
          Solar & Stellar astrophysics

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