par Abbott, B. P.;Collette, Christophe ; [et al.]
Référence Classical and quantum gravity, 34, 4, 044001
Publication Publié, 2017-01
Article révisé par les pairs
Résumé : 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.