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Third-generation gravitational-wave detectors, such as the Einstein Telescope and the Cosmic Explorer, are projected to be not only extremely sensitive instruments for detecting compact binary coalescences but also the cosmological gravitational-wave background. However, in order to delineate the stochastic cosmological gravitational-wave background in the observed data, the astrophysical foreground needs to be subtracted. This paper proposes a method to achieve this to make these new GW detectors instruments of cosmology.
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J. Harms (2020) studied this question.
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