RIT Logo with Text
Exploring the Sensitivity of Next Generation Gravitational Wave Detectors
By B P Abbott et. al
Published in Classical and Quantum Gravity 34, 044001 (Friday, January 27, 2017)


The second-generation of gravitational-wave detectors are just starting operation, and have already yielding their first detections. Research is now concentrated on how to maximize the scientific potential of gravitational-wave astronomy. To support this effort, we present here design targets for a new generation of detectors, which will be capable of observing compact binary sources with high signal-to-noise ratio throughout the Universe.