Table 1 BBH parameters for Fig. 1

From: An interference-based method for the detection of strongly lensed gravitational waves

q

\({\bf{\mathcal{M}}}_{{\mathbf{obs}}}\)

zs

a1

a2

θjn

RA

dec.

Ψ

0.4

28.8

1

0.98

0.46

2.22

5.52

0.57

0.27

  1. q is the mass ratio, \({{\mathcal{M}}}_{{\rm{obs}}}\) is the chirp mass, zs is the redshift of the source, a1 is the spin magnitude of the primary black hole, a2 is the spin magnitude of the secondary black hole, θjn is the inclination, RA is the right ascension, dec. is the declination, and Ψ is the polarization angle.
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