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Bayesian Inferences on the Twin-star Scenario from NICER Pulsars

Xieyuan Dong et al 2026 The Astrophysical Journal 1011 .

Caption: Figure 5.

Same as Figure 3, but with the phase transition density set to 2.5 n₀. The Δϵ values are Δϵ_cr + 450, 650, and 950 MeV.