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The next generation of gravitational-wave observatories will reach low frequency limits on the orders of a few Hz, thus enabling the detection of gravitational wave signals of very long duration.
1904
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2016
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R. Smith, S. E. Field, K. Blackburn, C. Haster, M. M. Pürrer, V. Raymond, and P. Schmidt, “Fast and accurate inference on gravitational waves from precessing compact binaries,” Phys. Rev. D 94
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2018
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2020
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2020
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2020
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R. Abbott et al. (LIGO Scientific, Virgo), “Observation of Gravitational Waves from Two Neutron Star–Black Hole Coalescences,” The Astrophysical Journal Letters 915
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Zu-Cheng Chen, Hong Qi, and Vivien Raymond, “Systematic Effects of LIGO-Virgo Design Noise on the Inference of Gravitational Waves from Neutron Star-Black Hole Mergers,” In prep. (2021)
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Massimo Tinto and Sanjeev V. Dhurandhar, “Time-delay interferometry,” Living Rev. Rel. 24
2021
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