LIGO Document G1800648-v1
- In the new era of gravitational wave astronomy, our primary goal is to measure source parameters and draw astrophysical inferences from observed signals. To do this effectively, we require an accurate calibrated estimate of the gravitational wave strain from our detectors. In this talk, I describe a broad overview of the scheme we use to calibrate the Advanced LIGO detectors, and report on the performance of calibration during the first two observing runs of Advanced LIGO.
- This update contains a proper first draft. The main file is a PDF, which is derived from a keynote presentation (also attached).
- ODW#1 held from 25 Mar 2018 to 27 Mar 2018 in Caltech
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