Current Noise at LHO Worst wire loss inferred from in situ violin mode measurements: =
2 Thermal Noise in Initial LIGO
3 Sensitivity Effects of Suspension Thermal Noise Binary Neutron Star Binary Black Holes (10 M o ) Stochastic Crab Pulsar SRD16 Mpc60 Mpc = Typical in situ 19 Mpc75 Mpc = Wire material limit 27 Mpc120 Mpc Thermoelastic limit 29 Mpc135 Mpc Single Interferometer Values