Compact binaries through a lens: Silent versus detectable microlensing for the LIGO-Virgo-KAGRA gravitational wave observatories

INIS

• compacts 100%
• lenses 100%
• gravitational waves 100%
• probability 60%
• maps 40%
• sensitivity 40%
• signals 40%
• signal-to-noise ratio 40%
• noise 40%
• power 20%
• images 20%
• curves 20%
• banks 20%
• red shift 20%
• dark matter 20%
• black holes 20%
• wave forms 20%
• amplification 20%
• waveforms 20%
• spectral density 20%
• gravitational wave detectors 20%
• gravitational lenses 20%
• frequency dependence 20%

Physics

• Gravitational Microlensing 100%
• Signal-to-Noise Ratio 100%
• Observatory 100%
• Gravitational Wave 100%
• Black Holes 50%
• Gravitational Wave Detectors 50%
• Dark Matter 50%
• Line of Sight 50%
• Machine Learning 50%
• Gravitational Lens 50%
• Power Spectral Density 50%