The analysis of a set of radial velocities in planet searches typically involves a number of different steps. First, the best fitting Keplerian orbital parameters are found by minimizing χ 2, for example with a Levenberg-Marquardt algorithm
No takes yet. Share an insight, caveat, or question.
Cumming et al. (2009) studied this question.
Synapse has enriched 5 closely related papers on similar clinical questions. Consider them for comparative context: