Image Details
Caption: Figure A3.
Posterior distributions of key orbital parameters for the independent fit of 70 Oph A’s orbit around 70 Oph B (Section 4), analogous to Figure 4 for the primary joint fit. The panels show marginalized one- and two-dimensional posteriors for the primary and secondary masses (Mpri and ﹩{M}_{{\rm{\sec }}}﹩, respectively), semimajor axis (a), eccentricity (e), and inclination (i). Contours represent 1σ, 2σ, and 3σ credible regions, while vertical dashed lines mark the median and 68% CIs.
© 2026. The Author(s). Published by the American Astronomical Society.