B. P. Abbott coauthored the collaborative analyses of GW150914. Fitting general relativity waveforms to LIGO data constrained the properties of the merging binary black hole.[ref]
Properties of the Binary Black Hole Merger GW150914 by B. P. Abbott and others. Author list and abstract: coherent analysis across the detector network using compact-binary waveform models and inferred source parameters.
A companion study converted detector control-loop signals into gravitational wave strain, with an optomechanical response model and independent checks of its measurement uncertainty.[ref]Calibration of the Advanced LIGO detectors for the discovery of the binary black-hole merger GW150914 by B. P. Abbott and others. Author list and abstract: time-domain calibration filters, optomechanical/feedback response and validation with radiation-pressure actuation.
- Calibration of the Advanced LIGO detectors for the discovery of the binary black-hole merger GW150914 by B. P. Abbott and others
- Characterization of transient noise in Advanced LIGO relevant to gravitational wave signal GW150914 by B. P. Abbott and others
- GW150914: First results from the search for binary black hole coalescence with Advanced LIGO by B. P. Abbott and others
- LIGO: The Laser Interferometer Gravitational-Wave Observatory by B. P. Abbott and others
- Observation of Gravitational Waves from a Binary Black Hole Merger by B. P. Abbott and others
- Properties of the Binary Black Hole Merger GW150914 by B. P. Abbott and others
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