A mock data challenge shows that a phase-coherent search for the binary black hole background can recover injected signal fractions in realistic noise, using new treatments of noise uncertainty, finite-duration effects, and glitches.
For each segment, we compute the signal evidenceZ i s and the noise evidence Z i n using Bilby [50], which employs nested sampling with the dynesty sampler [51]
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Progress toward the detection of the gravitational-wave background from stellar-mass binary black holes: a mock data challenge
A mock data challenge shows that a phase-coherent search for the binary black hole background can recover injected signal fractions in realistic noise, using new treatments of noise uncertainty, finite-duration effects, and glitches.