Image Details
Caption: Figure 10.
Prior (unfilled) and posterior (filled) distributions for the L parameter for the GP-N3LO EOS extended up to 1.1 or 1.5 n0 with the PP (left) and CS (right) high-density extensions; the 1.5 n0 results are as in Figure 9.
© 2026. The Author(s). Published by the American Astronomical Society.