D. Tuyenbayev
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View article: Reconstructing the calibrated strain signal in the Advanced LIGO detectors
Reconstructing the calibrated strain signal in the Advanced LIGO detectors Open
Advanced LIGO's raw detector output needs to be calibrated to compute dimensionless strain h(t). Calibrated strain data is produced in the time domain using both a low-latency, online procedure and a high-latency, offline procedure. The lo…
View article: Calibration uncertainty for Advanced LIGO’s first and second observing runs
Calibration uncertainty for Advanced LIGO’s first and second observing runs Open
Calibration of the Advanced LIGO detectors is the quantification of the detectors’ response to gravitational waves. Gravitational waves incident on the detectors cause phase shifts in the interferometer laser light which are read out as in…
View article: Making h(t) for Advanced LIGO
Making h(t) for Advanced LIGO Open
Advanced LIGO's raw detector output needs to be calibrated to compute dimensionless strain h(t). Calibrated gravitational-wave (GW) strain data is produced in the time domain using both a low-latency, online procedure and a high-latency, o…
View article: Calibration Uncertainty for Advanced LIGO's First and Second Observing Runs
Calibration Uncertainty for Advanced LIGO's First and Second Observing Runs Open
Calibration of the Advanced LIGO detectors is the quantification of the detectors' response to gravitational waves. Gravitational waves incident on the detectors cause phase shifts in the interferometer laser light which are read out as in…
View article: The Advanced LIGO photon calibrators
The Advanced LIGO photon calibrators Open
The two interferometers of the Laser Interferometry Gravitational-wave Observatory (LIGO) recently detected gravitational waves from the mergers of binary black hole systems. Accurate calibration of the output of these detectors was crucia…