Foreground signals minimally affect inference of high-mass binary black holes in next-generation gravitational-wave detectors

Keyphrases

• Gravitational Wave Detectors 100%
• Binary Black Holes 100%
• Detection Sensitivity 50%
• Parameter Estimation 50%
• Low Frequency Range 50%
• System Parameters 50%
• Minimal Impact 50%
• Gravitational Wave Observatory 50%
• Multiple Signals 50%
• Binary Neutron Stars 50%
• Compact Binary Coalescence 50%
• Gaussian Noise 50%
• Parameter Estimation Method 50%
• Global Fit 50%
• Noise Power Spectrum 50%
• Overlapping Signals 50%

Physics

• Parameter Estimation 100%
• Gravitational Wave Detectors 100%
• Black Hole 100%
• Neutron Stars 50%
• Gravitational Wave 50%
• Power Spectra 50%
• Random Noise 50%
• Observatory 50%
• Detectors 50%