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GW230814: Investigation of a Loud Gravitational-wave Signal Observed with a Single Detector
A. G. Abac et al 2026 The Astrophysical Journal Letters 1004 .
Caption: Figure 2.
The joint probability distributions for the two component masses, as measured in the source frame using the four indicated waveform models. The shading density indicates the combined posterior, averaging the posterior equally over the four waveform models. Vertical dashed lines in the one-dimensional marginals indicate the 90% credible intervals. The individual component masses of the source are well measured owing to the high SNR, with values given in Table 2.
© 2026. The Author(s). Published by the American Astronomical Society.