Posterior not run for this galaxy and halo model.
Monte Carlo viewRun the chains to populate covariance, trace mixing and autocorrelation. The diagnostic plots below are deliberately compact and linked to the same samples.
Run posterior chains to create marginal distributions and a halo-parameter covariance plot.
Model-dependent inference
The rotation plot gains a 68% posterior predictive interval after sampling. It combines fitted-parameter uncertainty with the quoted SPARC random velocity errors. The current distance and inclination sensitivity settings are held fixed rather than marginalised, and correlated systematics remain outside this browser model. A posterior-predictive p-value near 0 or 1 can flag mismatch; it is not the probability that a halo model is true.