Image Details
Caption: Figure 4.
Marginalized posterior distribution for the secondary mass obtained using a suite of waveform models. The vertical lines indicate the 90% credible bounds for each waveform model. The labels Phenom/EOBNR PHM (generic spin directions + higher multipoles), Phenom/EOBNR HM (aligned-spin + higher multipoles), and Phenom/EOBNR (aligned-spin, quadrupole only) indicate the different physical content in each of the waveform models.
© 2020. The American Astronomical Society.