Acernese, F; Barone, F; Bose, S; Danilishin, S L; Sathyaprakash, B; Rabeling, David; Strigin, S; Tarabrin, S.; Van Den Brand, J.; Yamamoto, K.
Advanced gravitational wave interferometers, currently under realization, will soon permit the detection of gravitational waves from astronomical sources. To open the era of precision gravitational wave astronomy, a further substantial improvement in sensitivity is required. The future space-based Laser Interferometer Space Antenna and the third-generation ground-based observatory Einstein Telescope (ET) promise to achieve the required sensitivity improvements in frequency ranges. The vastly...[Show more]
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