Core noise and GW sensitivities of AMIGO
Author:
Affiliation:
1. National Astronomical Observatories, Chinese Academy of Sciences, Beijing, P. R. China
2. Innovation Academy of Precision Measurement Science and Technology (APM), Chinese Academy of Sciences, Wuhan 430071, P. R. China
Abstract
Funder
Strategic Priority Research Program of the Chinese Academy of Sciences
National Key Research and Development Program of China
Publisher
World Scientific Pub Co Pte Ltd
Subject
Space and Planetary Science,Astronomy and Astrophysics,Mathematical Physics
Link
https://www.worldscientific.com/doi/pdf/10.1142/S0218271822500390
Reference42 articles.
1. The astrophysical science case for a decihertz gravitational-wave detector
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3. The missing link in gravitational-wave astronomy: discoveries waiting in the decihertz range
4. Foreword
5. GW190521: A Binary Black Hole Merger with a Total Mass of 150 M⊙
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