A Second LIGO Gravitational Wave Observation?

GW150914: First results from the search for binary black hole coalescence with Advanced LIGO, The LIGO Scientific Collaboration, the Virgo Collaboration

"In addition to possible gravitational-wave signals, the detector strain contains a stationary noise background that primarily arises from photon shot noise at high frequencies and seismic noise at low frequencies."

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This page contains a single entry by Keith Cowing published on February 15, 2016 1:51 PM.

Gravitational Waves Detected was the previous entry in this blog.

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