Most reported discrepancies between orbital fits for wide companions trace to data selection, conventions, and posterior sampling, not to the F19/F23 method itself, which the paper shows is equivalent to orvara.
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Lessons learned from the detection of wide companions by radial velocity and astrometry
Most reported discrepancies between orbital fits for wide companions trace to data selection, conventions, and posterior sampling, not to the F19/F23 method itself, which the paper shows is equivalent to orvara.