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Observation of Gravitational Waves from the Coalescence of a 2.5–4.5 M ⊙ Compact Object and a Neutron Star
A. G. Abac et al 2024 The Astrophysical Journal Letters 970 .
Caption: Figure 7.
Posterior distributions of GW230529 under various prior assumptions. The solid teal curve shows the posterior distributions using the default high-spin priors described in Appendix D. The various dashed and dotted curves show posteriors obtained using population priors based on the NSBH-POP model (orange), BINNED GAUSSIAN PROCESS (blue), and POWER LAW + DIP + BREAK (red) models.
© 2024. The Author(s). Published by the American Astronomical Society.