68% (blue) 95% (green), and 99% (brown) quantiles for the posterior distributions of the pairing gap as a function of the baryonic density of beta-equilibrated matter for Set B. We show the results for the posterior without assumptions on the dUrca threshold (top left), as well as when the Sometimes (1.3 M_⊙ ≤ M_dUrca ≤ 2.1 M_⊙) assumption for the dUrca threshold is made for a star at T = 10⁸ K (top right), T = 10⁹ K (bottom left), and T = 10¹⁰ K (bottom right).