Detection, Measurement, and Gravitational Radiation
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Real-time inference for binary neutron star mergers using machine learning.
Dax M, Green S, Gair J, Gupte N, Purrer M, Raymond V Nature. 2025; 639(8053):49-53.
PMID: 40044889 PMC: 11882463. DOI: 10.1038/s41586-025-08593-z.
Imprints of massive black-hole binaries on neighbouring decihertz gravitational-wave sources.
Stegmann J, Zwick L, Vermeulen S, Antonini F, Mayer L Nat Astron. 2024; 8(10):1321-1331.
PMID: 39430610 PMC: 11486661. DOI: 10.1038/s41550-024-02338-0.
GW150914: First results from the search for binary black hole coalescence with Advanced LIGO.
Abbott B, Abbott R, Abbott T, Abernathy M, Acernese F, Ackley K Phys Rev D. 2020; 93(12).
PMID: 32818163 PMC: 7430253. DOI: 10.1103/PhysRevD.93.122003.
Relativistic dynamics and extreme mass ratio inspirals.
Amaro-Seoane P Living Rev Relativ. 2018; 21(1):4.
PMID: 29780279 PMC: 5954169. DOI: 10.1007/s41114-018-0013-8.
Quasi-Normal Modes of Stars and Black Holes.
Kokkotas K, Schmidt B Living Rev Relativ. 2017; 2(1):2.
PMID: 28191830 PMC: 5253841. DOI: 10.12942/lrr-1999-2.