Image Details
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 3.
Posterior on the merger rates of NSBH systems. The solid and dashed lines represent the broad population-based rate calculation and the event-based rate calculation, respectively.
© 2024. The Author(s). Published by the American Astronomical Society.