Image Details
Caption: Figure 4.
Left: marginalized 2D and 1D sections of the posterior distribution for the fitted parameters. In the 2D regions, the contours indicate the 1σ and 2σ credible regions, and the black circle marks the mode of each marginalized case. Right: the best-fit (MAP) rotation curve with an NFW dark matter halo (﹩{\delta }_{\star }=1.10,\,{\rm{\Delta }}i=0.01,\,\mathrm{log}c=0.75,\,\mathrm{log}({r}_{200}/\,\rm{kpc}\,)=2.64﹩).
© 2026. The Author(s). Published by the American Astronomical Society.