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Foil 17 Expected Signal versus Noise in Gravitational Wave Detectors

From Numerical Formulation and Solution of Collision 0f two Black Holes CPSP713 Case studies in Computational Science -- Spring Semester 1996. by Geoffrey C. Fox
Comparison between rms noise h/rms in LIGO's first and advanced detector systems and the characteristic amplitude h/c of gravitational wave bursts from several hypothesized sources
  • NS is a Neutron Star
  • BH is a Black Hole
Science 256,281-412, 17 April 92

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