Using standard Rayleigh-Rice and ABC spectral fitting, the authors produce a model scattering profile for KAGRA's core mirrors: dP/dΩ ≈ 2.5×10^2 [1+(θ/7.1×10^-5)^2]^{-1.6} per steradian.
Observation of Gravitational Waves from the Coalescence of a 2.5–4.5𝑀⊙ Compact Object and a Neutron Star,
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Modeling of optical scattering from topographic surface measurements of high-quality mirrors
Using standard Rayleigh-Rice and ABC spectral fitting, the authors produce a model scattering profile for KAGRA's core mirrors: dP/dΩ ≈ 2.5×10^2 [1+(θ/7.1×10^-5)^2]^{-1.6} per steradian.