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 6.
The differential binary merger rate as a function of the mass of the primary component using the BINNED GAUSSIAN PROCESS model (top panel) and the POWER LAW + DIP + BREAK model (bottom panel) for the full compact binary population (solid curves: mean; shaded regions: 90% credible interval) with (teal) and without (gray) GW230529.
© 2024. The Author(s). Published by the American Astronomical Society.