Waveform modeling uncertainties can distort features in the binary black hole mass distribution inferred from gravitational-wave data more than statistical uncertainties.
Using theGWSim[79] package, we simulate a universe consistent with ΛCDM cosmology, where BBH merger rates follow the Madau-Dickinson star formation history [80]
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Is the Binary Black Hole Population Inference from Gravitational-Wave Data Robust?
Waveform modeling uncertainties can distort features in the binary black hole mass distribution inferred from gravitational-wave data more than statistical uncertainties.