Image Details
Caption: Figure 3.
Mass–radius prior distributions for the PP (left panel) and CS (right panel) extensions with Bayesian χEFT uncertainties up to 1.5n0 without pQCD extensions (GP-N3LO, blue regions), with pQCD extensions (GP-N3LO with pQCD extension, solid red and orange lines), and uniformly sampled in the previous N3LO range (N3LO, black dashed lines). The dark (light) blue regions, the solid red (orange), and the inner (outer) black dashed lines encompass the 68% (95%) credible intervals. The regions at radii R ≲ 8 km in the orange/red contours are a result of softer EOSs being included in the prior by the pQCD extensions.
© 2026. The Author(s). Published by the American Astronomical Society.