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---

## Status: awaiting full input
This website has not loaded the original astrometry, covariance and corresponding ASD equation text required for full reproduction. It publishes no ASD orbit fit or residual plot.
## Independent calculation workflow
Obtain original measurements and conventions, check the Chapter 2 motion equations, integrate the orbit and project to the sky, fit with a common likelihood, inspect residuals and parameter degeneracies, then compare models on the same data.
## Conditions for detecting differences
Higher-order corrections are constrained only if data precision, observing duration and the background model can identify them. An undetected difference does not imply equivalence in every condition.
## High-gamma electric field case
The [Ota high-speed field open case](/tests/case-studies/high-gamma-charge-field) organizes paper sources and the order of source-field reconstruction and electro-optic response mapping. There is no quantitative ASD fit published here.