Bayesian inference for orbital eccentricities

Abstract

Highest posterior density intervals (HPDI's) are derived for the true eccentricities of spectroscopic binaries with measured values e ~ 0. These yield upper limits when e is below the detection threshold e_th and seamlessly transform to upper and lower bounds when e > e_th. In the main text, HPDI's are computed with an informative eccentricity prior representing orbital decay due to tidal dissipation. In an appendix, the corresponding HPDI's are computed with a uniform prior and are the basis for a revised version of the Lucy-Sweeney test, with the previous outcome e = 0 now replaced by an upper limit. Sampling experiments with known prior confirm the validity of the HPDI's.

7 pages, 6 figures. Error in terminology corrected. Results unchanged. Accepted by Astronomy & Astrophysics

References in corpus (2)

• EXOFAST: A fast exoplanetary fitting suite in IDL
• A study of non-Keplerian velocities in observations of spectroscopic binary stars

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